When brand new entry-level telescopes start at a few hundred dollars, the idea of getting anything decent for pocket change sounds like a pipe dream. Yet the secondhand market often hides real bargains for those willing to hunt them down. Deals like this appear because people buy on impulse, then quickly lose interest for various reasons.

Facebook Marketplace seemed like the best bet for such a deal, so I opted to keep an eye on the site for potential local bargains on the best telescopes I could find.

Finding quality gear on a shoestring budget

Amateur astronomy has a reputation for expensive equipment, but the used market flips that script somewhat. New telescopes in the $50 range are usually tiny 50- to 70-millimeter refractors that struggle with faint objects. I wanted more light-gathering power so I focused on searching for larger-aperture Newtonians.

The Celestron AstroMaster 130mm offered a decent 130 millimeters of aperture — more than double many cheap department store refractors. That extra size collects far more light, sharpens detail (especially on planets) and gives brighter views of fainter deep sky objects.

After about a week of scrolling on Marketplace I spotted a Celestron AstroMaster 130mm Newtonian reflector listed for just $50 by a local seller about 15 miles away. The photos showed it was in good condition complete with box and all parts. The seller said it had seen little use.

Hopeful, I drove across town to inspect the scope. Everything was present with no missing parts, and the optics were clean with no scratches. That was enough for me, and off I went with my bargain basement telescope!

Over the next few days I collimated, aligned and tested the scope on solar system targets and bright deep-sky objects. The results pleasantly surprised me. My $50 telescope delivered crisp planetary views and revealed many deep sky objects. It was not perfect but it proved that, with the right find and a bit of know-how, a tight budget need not limit the fun. Here is a breakdown of my experience.

Accessories that made the deal even better

The telescope came with everything needed to start observing that same night. Two Plössl eyepieces provided different magnifications, and there was also a red-dot finderscope and a manual equatorial mount with slow-motion cables.

For beginners, the red-dot finder is a lifesaver. It projects a red bull’s-eye on the sky so you simply center your target and look through the main eyepiece. The equatorial mount tilts to match Earth’s axis, allowing smooth tracking by turning two cables instead of pushing the tube constantly. The lack of motors meant I had to adjust manually, but the slow-motion controls made fine pointing easy even at higher power.

Those two eyepieces gave me roughly 33x and 65x magnification — enough for wide lunar views and tighter planetary shots. Nothing fancy but perfectly usable. One useful item not included was a Barlow lens to increase magnification on the planets, but I decided to use a 2x Barlow I already had. Just as a side note, Barlow lenses are widely available at very modest prices — especially secondhand.

Collimation: A simple step for sharp images

Newtonian reflectors require occasional collimation. This involves aligning the primary and secondary mirrors so light reflects properly to the eyepiece. Out of the box, my scope was slightly off, probably from travel or shipping. Luckily, the fix took less than 10 minutes.

I used a simple collimation tool with a tiny hole that fits in the focuser, but this isn’t essential — it can be done simply by eye sighting through the focuser. Looking through it, I adjusted the three screws on the primary mirror until the reflection of the primary mirror looked centered and symmetrical. The secondary mirror needed no adjustment.

A quick star test that evening confirmed pinpoint star images with no flares. Beginners often fear collimation but it is straightforward and essential. Skip it, and views will be blurry no matter how good the optics.

First light: Crisp views of Venus and Jupiter

With the scope collimated, I pointed it at Venus on the first clear evening. The planet showed a sharp gibbous disk phase, clearly visible even at moderate power. Edges stayed crisp with no false color, which is a common issue in cheaper refractors. Venus appeared almost three-dimensional against the twilight sky. The 130mm aperture gathered enough light to show subtle shading I had not expected at this price.

Jupiter, which was much higher in the evening sky, showed some detail on its disk. The Great Red Spot was visible, with its reddish colour quite obvious. All four moons were on view alongside the planet and looked sharp and point-like.

I then moved to a nearby bright star to test the optical quality. Racking the star inside and outside of focus at moderate power revealed well-corrected optics free of any major optical problems. I was most impressed overall — this felt like an amazing win for a $50 outlay!

Astrophotography on a budget: Sun, moon and planets

Without a motorized drive, long-exposure deep-sky photography was off the table but the sun, the moon and the brighter planets remained fair game. I crafted a simple solar filter from some Baader safety film I had stretched over a cardboard cell that fit snugly over the front of the tube. Safety first: NEVER point any telescope at the sun without proper filtration! Use the best solar viewing kit!

The filter revealed several nice sunspot groups, with umbra and penumbra detail visible as I tracked manually as best I could. This kind of telescope is ideal for solar work, being a good size aperture to reveal fine detail, but not so large as to be severely affected by daytime atmospheric turbulence.

Later that day, as the sun was nearing the horizon, I prepared to try and capture some images of Venus and Jupiter. I attached my Player One Uranus-C USB camera to the focuser and recorded short video clips of Venus and Jupiter over about an hour. Manual tracking was tricky, but I nudged the Right Ascension slow-motion cable every few seconds to keep the planet centered. Still, the results were surprisingly reasonable, and they are presented here.

The moon was available and I shot a handful of views. Through the scope it looked great, with sharp views across the lunar landscape with many fine details visible. I shot a few videos, but the one of the bright Tycho crater came out best. This is a great entry-level telescope to photograph the moon with, as it offers notably better resolving power than small refractors, as was obvious on some of the smaller lunar features I examined.

I was running my usual imaging setup at the same time, so managing both systems added an extra challenge. However, once the main rig was up and running, it largely looked after itself, giving me time to image with the smaller scope.

Jupiter showed cloud bands and its Great Red Spot could be seen just slipping off the edge, with three of its moons also in the field. The shadow of Ganymede could be seen on the planet which was impressive. Lunar images came out even better: crater rims and mountain shadows popped in high contrast, with the crater Tycho being my target of choice to capture – its brilliant ray system a striking sight.

These were certainly not observatory-grade results but they proved even a super-cheap $50 scope plus a decent camera can still capture good detail, as long as you have patience and a steady hand.

Deep-sky observing under darker skies

City light pollution hides fainter objects, so I drove 45 minutes to a darker site to do some visual observing. The manual mount and red-dot finder let me star-hop efficiently. Some degree of night sky knowledge is essential here: either that, a decent star atlas or a laptop with planetarium software.

Messier 13, the Hercules globular cluster, looked impressive. Its core was partly resolved into a sparkling ball of stars with faint outliers visible even in the 130mm aperture. Messier 5 appeared similar. The bright galaxy pair Messier 81 and 82 showed distinct shapes side by side. I also had a good look at the Double Cluster in Perseus, which was a stunning sight, revealing a field of pin-point stars, far too many to count!

I also had a quick look at the Virgo cluster — the largest nearby galaxy cluster to the Milky Way— and several of the bright galaxies were easily observed. I also tracked down NGC 4565 —the Spindle Galaxy in Coma Berenices — and its long, elongated shape was obvious, appearing like a long ghostly sliver of light.

Overall, the experience was most enjoyable, and the views surprisingly good. One slight frustration was the lack of tracking, which means you frequently have to counter the drift through the eyepiece by turning the slow motion controls. I have become too spoiled over the years by tracking mounts!

Lessons learned: Pros, cons and beginner advice

A $50 telescope obviously has limits. Having no motor drive meant constant manual tracking, which rules out long-exposure astrophotography of nebulae or galaxies. And packing no GoTo computer requires at least a rudimentary knowledge of the night sky and a star atlas or planetarium software.

Still, the scope outperformed anything new you could buy at this price. The larger aperture delivered light and detail that would be impossible in tiny department-store refractors.

Select carefully when buying used equipment. Inspect mirrors or lenses for damage, test the mount for smooth motion and ask about usage history. Also make sure all parts are present, and ask to see the telescope set-up if possible.

With patience and selectivity, a tight budget can still open up the universe. This somewhat surprised me given the general expense of things these days. I was also surprised how many used telescopes are available on public social media marketplaces like this. There were many telescopes available in the $50-200 range, with even better options available toward the upper end of this budget.

If you are looking to buy a first telescope, or perhaps a telescope as a gift, I’d strongly urge looking at the secondhand market. With some searching and patience, and if you follow the key buying points I’ve outlined here, there are some amazing deals just waiting to be found!

With a total solar eclipse on Aug. 12, an annular solar eclipse on Feb 6, 2027 and another total solar eclipse on Aug. 2, 2027, solar telescopes are about to be in hot demand. After all, why peer at the eclipsed sun when you can see it in close-up? However, the Sky-Watcher Heliostar 76mm offers something a little different to a telescope wearing a solar filter — and it’s just as good when there’s no eclipse at all. Built around a standard, small-aperture refracting telescope, it has an H-alpha etalon (an ultra-narrowband filter used to observe the sun) and a diagonal blocking filter, which together let you safely see features in the sun’s chromosphere, a layer of its atmosphere above the surface (photosphere) and below its corona (outer atmosphere). It’s a layer that’s invisible in standard white light, but it glows in the very specific 656.28 nm wavelength of light, called hydrogen alpha (about 92% of all the atoms in the sun are hydrogen).

Costing around US$3,395/UK£2,399, the Sky-Watcher Heliostar 76mm isn’t specifically an eclipse telescope, being unable to show you anything of the precious but short totality phase, when the corona comes into view. Although it’s a great way to get a unique look at the partial phases of a solar eclipse, it’s actually best seen as a solar telescope fit for studying our star at any time. It can show incredible features such as prominences (which look red to the naked eye during totality), filaments, bright plage regions and even solar flares (if you’re lucky with timing!), but can be used at any time of the day.

Read: The best solar telescopes for an HD view of the solar surface

Sky-Watcher Heliostar 76mm H-alpha solar telescope: Design

• Purpose-built H-alpha solar refractor
• Relatively portable 76mm tube
• Safety-critical blocking-filter diagonal

At first glance, the appeal of the Sky-Watcher Heliostar 76mm is obvious. A 76mm aperture is large enough to offer meaningful solar detail, but the 8.4 lbs/3.8kg tube remains easy to mount. The 630mm focal length gives a useful image size, while the included finder, eyepiece, diagonal, sunshade and case make it feel like an all-in-one solar observing package, albeit an expensive one.

It comes with all the scaffolding firmly attached, from carry handle and tube rings to a V-style dovetail, which is simple to attach to a mount. It also comes with a diagonal containing the 11.5mm blocking filter, which looks like an add-on, but is a critical part of the safe optical system that must be in place when using the Sky-Watcher Heliostar 76mm.

Is it portable? Kind of. It’s hardly a grab-and-go gadget, but it’s light enough to take in and out of a backyard and, if you’ve a mind to, on trips once in its protective case.

Build quality is mostly excellent, which also applies to most of its accessories. Notably, its dual-speed Crayford focuser on the scope is firm and precise, with a fine-tuner to easily get a sharp image. We also liked the rugged design of the solar finder, which makes it easy to use and dependable. Lastly, it comes with a small, sturdy sunshade that attaches to the tube and keeps the observer in the shade while observing.

Sky-Watcher Heliostar 76mm H-alpha solar telescope: Performance

• Bright images of the surface, filaments and prominences
• Uneven contrast across the sun’s disk
• Trifid Tuner helps bring out solar features

Remember that time you first saw Saturn and its rings in a telescope? Prepare for something similar when you first look through the Sky-Watcher Heliostar 76mm at what’s happening on the surface of our star. What you’ll see is an orangey disk that, once brought into focus, is scarred by bubbles and grain on its surface, plus giant dark tears called filaments, with plenty of contrast bringing the entire scene to life. Around the edge, we spotted some prominences. It truly is a superb view — we couldn’t take our eyes off it.

The only issue we had with the Sky-Watcher Heliostar 76mm, from a visual observing point of view, was the uniformity of the image. Although it’s perfect in some areas, it’s less so in others, with some patches too bright and others lacking contrast. Luckily, there’s a mechanical lever on the optical tube known as a Trifid Tuner, which applies micro-pressure to the etalon, slightly changing the contrast levels.

The Trifid tuner allows you to alter exactly what you see of the solar disk and the prominences, though it never completely solves that uniformity issue. We found that the best way was to nudge the tuner slightly, wait for the scope to settle, and take another look through the eyepiece. That way, you can look for granulation, dark filaments and bright prominences, all of which demand different levels of contrast.

Sky-Watcher Heliostar 76mm H-alpha solar telescope: Functionality

• Quick setup and easy alignment
• Great for visual observing
• Imaging requires time and patience

The Heliostar 76mm is fairly straightforward by H-alpha standards, with the Trifid tuner a simple way to tune it to observe different solar features. The 20mm eyepiece in the box worked well, as did the dual-speed focuser. In fact, the only thing getting in the way of setting up the Sky-Watcher Heliostar 76mm in mere minutes is the recommendation that a solar telescope should be left outside in the shade for at least 30 minutes before use, so its etalon can reach thermal equilibrium (otherwise you can expect uneven contrast and even distortion).

The Sky-Watcher Heliostar 76mm is designed primarily for optical solar astronomy, but it’s also good for anyone taking their first steps into solar imaging. This is a highly specialized niche of astrophotography, and not one to be taken lightly; expect to spend many hours learning to use myriad software packages (none of which are supplied or even suggested by the manufacturer) and post-processing images. We gave solar photography a try with a ZWO ASI174MM monochrome planetary camera, which we used to capture videos of the sun with FireCapture software. The task then is to extract, stack and process frames.

If none of those desk-based tasks appeal — and to many visual astronomers, they won’t — Sky-Watcher does include a smartphone adapter. We tried it out and although it was easy to use and worked well, it obtained only very basic images of the sun.

How we tested the Sky-Watcher Heliostar 76mm H-alpha solar telescope

We tried the Sky-Watcher Heliostar 76mm for about two weeks from a suburban backyard, always with a SkyWatcher SolarQuest mount head (which is sometimes bundled with the telescope). We largely used it to visually observe prominences, filaments, sunspots and texture on the sun in H-Alpha using the provided 20mm eyepiece, always leaving the scope outside for a while to acclimatize before use. We also experimented with taking full-disc solar images using a ZWO ASI174MM planetary camera.

Should I buy the Sky-Watcher Heliostar 76mm H-alpha solar telescope?

Buy the Sky-Watcher Heliostar 76mm if you want a dedicated H-alpha solar telescope that prioritizes visual observing, portability and ease of use. It’s perfect for anyone who wants to see prominences and filaments in far more detail than white-light solar viewing can provide. The only real issue is a slight lack of uniformity in contrast in its field of view, which necessitates tweaking its Trifid Tuner as you observe different features — something that potentially creates issues if you’re planning to image the solar disk using a planetary camera.

If the Sky-Watcher Heliostar 76mm H-alpha solar telescope isn’t for you

If your priority is simple, inexpensive solar observing, a certified front-mounted white-light solar filter on a suitable telescope is a cheaper route, but it will primarily show sunspots rather than the more dramatic H-alpha prominences and filaments. Similar H-alpha telescopes typically considered as rivals to the Sky-Watcher Heliostar 76mm include the Coronado PST and the much more expensive Lunt LS80MT B1200.

Mention that a total solar eclipse is coming, and almost nobody will say, "Wow, we get to see the solar corona!" That's despite the sun's tenuous outer atmosphere being the number one sight during totality — a genuine jaw-dropper.

Instead, the focus on social media is always on the darkness during the day, arguably the least interesting — but easiest to grasp — aspect of a total solar eclipse. It's no wonder that many people misunderstand and underestimate them, and think of eclipse chasers as a little odd.

But that's not the half of it. There are dozens of things to see and experience during a total solar eclipse, so many that we've put together a checklist of things to see as you're swallowed by the moon's shadow. Here's what you may experience during the solar eclipse on Aug. 12, 2026, roughly in the order they occur from first contact — when the moon begins to eclipse the sun — to fourth contact, when it departs.

1. Sunspots

Here's one everyone in both the partial and total eclipse zones can see on Aug. 12, 2026. As the moon's silhouette moves across the sun, look through your ISO-certified safe solar eclipse glasses/solar filters. With luck, you'll see the edge of the moon move across dark spots on the solar surface. These are sunspots, cool patches where the sun's magnetic field is concentrated and complex. They're where solar flares come from.

2. Planets

You'll often hear someone shout, "There's Venus!" during the totality phase of a total solar eclipse, to which your response should rightly be: "Who cares?" as you focus on the much rarer sight of the solar corona. The correct time to look for planets is about 15 minutes before totality, when — on Aug. 12, 2026 — Jupiter will appear about 11 degrees west-northwest, with tiny Mercury about 4 degrees beyond. Venus will be much farther away, about 46° east-southeast of the sun, but easy to see. Mars will be low in the west, but much more difficult to see.

3. Crescent-shaped shadows

Here's another one everyone can look out for during a deep partial solar eclipse. When over 50% of the sun is eclipsed, crescent-shaped shadows begin to appear on the ground beneath trees. It's sunlight passing through tiny gaps, which act like the aperture control on a camera. The best way to see them is to grab a colander or spaghetti spoon — or anything with small, defined holes. Failing that, cross your fingers in a waffle pattern and you'll project diffuse crescents.

4. Shadow bands

Here's one for eclipse chasers in Spain. About two minutes before and after totality, it's sometimes possible to see wavy lines on white surfaces. It's the reduced light from the crescent sun being refracted by atmospheric turbulence, and, for some reason, it's much more noticeable when the eclipse is low in the sky — as it will be from Spain. They're called shadow bands or "shadow snakes". Pack as large a white sheet as you can (or borrow one from your bemused hotel).

5. Plunging light and heat

As the partial eclipse reaches about 80%, you'll begin to notice it getting cooler. By the time it's just seconds before totality, it will be chilly as the light levels around you crash like nothing else you have experienced. "Darkness in the day" does not do it justice — it's as if the world is ending. Even experienced eclipse chasers get a knot in their stomach about now as a primordial fear kicks in. That feeling is not helped by looking at the others around you, who, in the eerie, silvery light, suddenly look almost ghoulish.

6. The moon's shadow

This is a tricky thing to see. The prelude to totality is the arrival of the moon's umbral shadow, which will race across observers at about 2,200 mph (Greenland and Iceland) to about 12,000 mph (in eastern Spain, where the shadow is by then oblique and about to skip off the Earth). You'll need an elevated position — perhaps the side of a valley — looking northwest for this sight, and preferably a relatively uniform landscape. It's something you can attempt to capture using a GoPro or similar.

7. Diamond rings and Baily's beads

These are trademarks of totality, but require care to see. As the eclipse nears totality, a spectacular drop of sunlight (the diamond ring) breaks into tiny so-called Baily's beads of light streaming through the moon's valleys. When the final bead vanishes, totality begins. The opposite happens a few minutes later at the end of totality, when a Baily's bead appears, then a few more, quickly coalescing into a second diamond ring. Do what experienced eclipse chasers do and ignore the first round — you'll just end up with an after-image in your eyes, which will affect your vision just as the corona pops into view. Besides, it's the second diamond ring that's the real "wow" moment that ends totality. Its arrival means it's time to put your solar eclipse glasses back on.

8. Solar corona

This is what you came to see. The sun's corona, its outer atmosphere, is where solar flares and coronal mass ejections come from. It's the hottest part of the sun. It's always there — but hidden from view by the much brighter surface of the sun, its photosphere. Only when the photosphere is blocked by the moon — totality — can the corona be seen. During this time, it's essential that you remove your solar eclipse glasses to see the tenuous halo around the silhouette of the moon. It's a surreal and remarkable sight. Should you bring binoculars just to look at the corona during totality, even if it's only for a few seconds? Yes! This may be the most beautiful thing you will ever see.

9. Solar chromosphere

Just after totality begins and just before it ends, a thin crimson line appears where the diamond ring just was and is about to be. This is the chromosphere, a layer of the sun's atmosphere just above the photosphere. It's a fleeting sight used by scientists to capture a "flash" spectrum that shows exactly what chemical elements are in the sun's atmosphere.

10. Solar prominences

One of the most surprising aspects of witnessing a total solar eclipse is a view of prominences during totality, bright pink spikes or loops that appear around the moon's silhouette. These are cool plasma structures extending from the chromosphere into the corona, usually lasting days or weeks. They're particularly obvious when the sun is close to solar maximum — as it is right now.

11. Totality 'sunset'

Totality will be short for many eclipse chasers on Aug. 12, 2026, but if you can take your eyes off the solar corona, glance at the colors in the sky close to the horizon — it looks like a 360-degree sunset. If it's cloudy and you miss the corona, the colors around you can be particularly memorable.

12. Meteors

By remarkable coincidence, the total solar eclipse on Aug. 12, 2026, comes only a few hours before the peak of the annual Perseid meteor shower. Expect about 20-40 "shooting stars" to be visible every hour around midnight and into the early hours of Aug. 13, though among eclipse chasers, those in rural Spain will have a better chance since there are more hours of darkness than in Iceland and Greenland. Could there be a "shooting star" during totality? It's possible — but to see it, you'd have to be looking away from the solar corona, which would be a mad thing to do.

13. Aurora borealis

Is it a long shot? Yes. Is it possible? Also yes. The specter of the aurora borealis appearing during totality in the skies above Iceland and Greenland during totality is getting eclipse chasers excited. The reality is that totality is never as dark as people think — it's a twilight — plus aurora on the day-side of Earth is not nearly as strong as on the night-side. It could happen — though more likely is a display of the northern lights late at night, particularly in Iceland, where the night sky does get sufficiently dark in mid-August, and auroras are commonly seen at that time of year.

Spotting scopes are typically used by birders and for hunting, but under a dark sky, the Nocs Provisions Lite View reveals a different personality. With a 56mm objective lens and a versatile 9x-27x zoom range, this compact spotting scope is surprisingly capable when turned toward not just the moon, but bright star clusters, too.

Key to its attraction is its small size, carry case and shoulder strap, which makes it possible to sling over a shoulder. Its rugged, wave-textured housing and bright color options? Not so much. However, with just enough optical performance to satisfy casual astronomers — particularly those focused on lunar observing — it makes a good option for astro-travel. Is it a replacement for one of the best telescopes? Absolutely not — but for close-up views of the lunar disk (particularly lunar eclipses), Jupiter and its moons, and bright open star clusters such as the Pleiades — this lightweight scope offers an appealing balance between portability and power if, and only if, you mount it on a tripod.

Nocs Provisions Lite View spotting scope review

Nocs Provisions Lite View spotting scope: Design

• Compact, travel-friendly size
• Rugged rubberized grip
• Integrated tripod mount

What's immediately noticeable about the Lite View is its rubberized, wave-textured exterior, which feels solid and secure in the hand. It's impact-absorbing and confidence-inspiring — important if you're heading out to a field for a late-night lunar eclipse, perhaps — though it will jar with anyone used to the mono, metallic designs favored by telescope designers. As a bonus, the IPX4 water-resistant rating means it will tolerate drizzle and damp conditions, though it's not fully waterproof or fogproof. Are we fans of its two color choices, Ochre Yellow and Saguaro Green? Not so much, though; with the popularity of stargazing-themed travel, the differing tones of astronomy scopes and spotting scopes no longer make sense.

At 192 mm long and weighing 567 g / 1.2 lb, the Lite View lives up to its name. It's small enough to fit into a larger jacket pocket and comes with a protective carrying case and shoulder strap, making it ideal for grab-and-go observing sessions. Its focus wheel and eyepiece zoom ring are logically placed, but while the former can feel slightly stiff at first, the latter is much looser. After some use, the focus wheel loosens and becomes smoother to operate. Meanwhile, the twist-up eyecups offer 18 mm of eye relief, making it comfortable to wear with spectacles.

Crucially for astronomy, the scope includes an integrated tripod mount. At higher magnifications, it proves essential.

Nocs Provisions Lite View spotting scope: Performance

• Excellent lunar detail
• Visible Galilean moons of Jupiter
• Some chromatic aberration

Turn the Lite View toward a first-quarter moon, and it quickly justifies its place in a basic travel astronomy kit. At 9x magnification, the lunar disk appears crisp and bright against the night sky, with strong contrast across the dark maria and a pleasingly wide field of view that makes locating and centering it effortless. Increase the magnification to around 20x, and the view becomes more immersive, with crater chains and rugged terrain along the terminator snapping into satisfying relief as shadows sculpt the surface into dramatic texture.

At the full 27x magnification, crater rims and fissures become more pronounced, and for a 56mm spotting scope, the overall sharpness remains impressive. However, this is also where the scope’s limitations begin to surface. A trace of purple fringing and faint yellow coloration appear along the lunar limb in high-contrast areas, but it's not severe. Sharpness softens slightly compared to the sweet spot around 20x magnification, and in darker conditions, chromatic aberration becomes more noticeable around the moon.

Beyond the moon, it performs surprisingly well on bright deep-sky targets. The Beehive Cluster (M44) appears as a sparkling spray of stars, while the Orion Nebula (M42) shows a soft, misty glow under darker skies. The Pleiades (M45) particularly benefit from the generous field of view at lower magnifications, presenting a striking cluster framed against a black sky. Even Jupiter offers a rewarding sight. Though the planet remains small and surface detail is not visible, its four Galilean moons are clearly visible.

Optics-wise, the Lite View is not going to rival premium top-end ED-glass optics or a dedicated refractor telescope, but its HiFi fully multi-coated lenses and XDR roof prisms deliver bright, reasonably sharp views overall, particularly at mid-range magnifications. Overall, it meets expectations for its size and price.

Nocs Provisions Lite View spotting scope: Functionality

• Smooth zoom control
• Tripod use is essential
• Handy carry case

Key to the appeal of the Lite View are its 56mm objectives and 27x magnification, which you won't find in most lightweight binoculars. However, like large astronomy binoculars, this spotting scope — despite being very lightweight — is best used with some stability. While technically possible to use handheld at 9x, stability becomes an issue beyond 12x. At 27x, even slight movements blur the image significantly. For serious lunar observing, a tripod is mandatory. Annoyingly, the scope comes with a large rubber mount covering the undercarriage's tripod thread, which needs to be removed using an (included) Allen key. It appears to serve no purpose.

The great thing about the Lite View's zoom range is that it's smooth, flexible and allows the easy framing of the moon at low power before zooming in to better fit the field of view. Focusing at high magnification requires a gentle touch. The focus ring's resistance helps prevent accidental shifts, but fine adjustments demand patience. You'll also need to refocus slightly when changing magnification, which does somewhat interrupt the flow when observing.

Should you buy the Nocs Provisions Lite View spotting scope?

The Nocs Provisions Lite View Spotting Scope occupies an interesting niche. It's not a dedicated astronomical device, yet it performs impressively on the moon and bright objects. Its lightweight build, shoulder-ready pouch and integrated tripod mount make it ideal for travel, spontaneous observing sessions and lunar eclipses. Yes, there's some chromatic aberration. Yes, it softens slightly at 27x. However, when mounted steadily and aimed at Earth's natural satellite, it delivers detailed, rewarding views that exceed what its size suggests. For lunar lovers who value portability and simplicity, it's a compelling companion under the night sky.

How we tested the Nocs Provisions Lite View spotting scope

We tested the Lite View during multiple evening sessions under suburban skies and in darker rural conditions. Particular attention was given to lunar observing at various phases from crescent to gibbous and other bright objects in the night sky.

The scope was mounted on a stable tripod for all high-magnification observations. We evaluated sharpness, color fidelity, contrast and ease of focusing, as well as its ability to resolve Jupiter's Galilean moons and several bright deep-sky objects, largely bright open clusters of stars.

If the Nocs Provisions Lite View spotting scope isn't for you

If you're seeking significantly higher magnification and premium optical performance, consider the Celestron Regal M2 80 ED, which delivers outstanding clarity at a much higher price point. Astrophotographers may prefer a similarly priced entry-level smart telescope, such as the DwarfLab Dwarf Mini, which can capture excellent images of the moon and deep-sky objects. Another option is large stargazing binoculars like the Celestron SkyMaster 20x80 Pro, which offer greater light-gathering for fainter objects, though at the cost of added bulk.

The excitement of the new moon mission has potentially helped create a new generation of stargazers, just like the Apollo program did 60 years ago. These new observers will be looking for a beginner’s telescope that is easy to use and which can show them the craters on the moon in particular. The Celestron Moon Mission 100mm Tabletop Dobsonian could be the perfect entry point for them. It has a superb price-point for its aperture, and is capable of bringing not only the moon, but double stars, the brighter galaxies and nebulas and the moons of Jupiter to your backyard.

The Celestron Moon Mission 100mm Tabletop Dobsonian comes equipped with 8mm and 20mm eyepieces, one of which is intended specifically for the moon, as well as a red-dot finderscope, a moon filter, a moon-map poster and free access to download the Starry Night planetarium software and Celestron’s SkyPortal app, which is powered by SkySafari.

All in all, it will make an excellent package for someone to get started enjoying the night sky. Though the optics and accessories are not perfect, for the price their drawbacks can be overlooked, and as an entry-level telescope it paves the way for the user to graduate to increasingly more sophisticated telescopes at a later date.

Celestron Moon Mission 100mm Tabletop Dobsonian review

Celestron Moon Mission 100mm Tabletop Dobsonian: Design

• Quick and simple set-up
• Portable

The Celestron Moon Mission 100mm Tabletop Dobsonian comes out of its box complete, other than its eyepieces and red-dot finderscope in plastic bags. Set-up takes literally minutes — remove the plastic cap over the aperture and the cap on the focuser, insert your eyepiece of choice, screw on the finderscope and you are ready to go. No tools such as screwdrivers or Allen keys are needed— it is just a matter of unscrewing thumbscrews.

We found the finderscope went on easily — more about that later. However, the tiny thumbscrews that lock in the eyepiece were incredibly tight. Pliers didn’t help much and risked damaging the screw. In the end, we found elbow grease was just about enough to unscrew them, but if our review model is typical, then children will definitely need the help of an adult to unscrew these. Once they are unscrewed, they can be tightened to more forgiving tolerances.

Overall we can recommend the build quality of the Celestron Moon Mission 100mm Tabletop Dobsonian. Everything is sturdily made, from the Dobsonian base, the optical tube, the easily adjustable tilt and focuser knobs. The mount has a single arm and rotates on a ‘lazy Susan’ turntable.

Celestron Moon Mission 100mm Tabletop Dobsonian: Performance

• Three
• Bullet
• Points

This is where we thought that the Celestron Moon Mission 100mm Tabletop Dobsonian excelled. For such a small telescope, it was decently versatile.

For example, on the night of April 5, our first target was Jupiter, which was bright in Gemini, and unmistakable as it lay not far from the constellation’s twin stars Castor and Pollux. Jupiter appeared as a bright disk, with perhaps the merest hint of its banding — or was that our imagination? What certainly were real were the four Galilean moons: Io and Europa on one side, Ganymede and Callisto on the other. It was a sight sure to impress beginners and casual observers.

We moved the Celestron Moon Mission’s view towards the multiple star Castor, and the telescope capably split the main binary pair as two close, white stars using the 20mm eyepiece. Another popular multiple star is Mizar and Alcor in Ursa Major. Of course, Mizar and Alcor can be split with the naked eye, but the third visible star in the system is for telescopes only, and again the Celestron Moon Mission showed the three stars clearly.

Slewing east, Arcturus — the second brightest star visible from the U.K., and fourth brightest in the entire sky — appeared a glorious red, evoking its nature as a red giant.

While waiting for the moon to rise (and before taking some time out to watch the Artemis II coverage), we decided to track down some faint fuzzies. The box that the Celestron Moon Mission comes in highlights the Orion Nebula and the Andromeda Galaxy as two deep sky objects that the telescope can see. At the time of testing, the Orion Nebula was too low in the west, while the Andromeda Galaxy was not visible. Instead, we hunted down two other nearby galaxies, M81 and M82, in Ursa Major.

Searching for these two galaxies, which are located next to each other in the same field of view, is where the real challenge of using the finderscope, as we described in the Functionality section, really reared its head. In the end, we decided to star hop to the galaxies and struck out in roughly the right direction. Soon the telescope alighted on the two galaxies, visible as two fuzzy patches of light. Looking at them straight on, we found it difficult to discern their shape, but by using averted vision as we looked through the 20mm eyepiece of the Celestron Moon Mission, we could make out the broad disk-shape of the spiral M81, and the elongated cigar shape of M82, and even caught hints of mottling with brighter spots in the edge-on M82 that are better seen in images.

After we watched the live NASA feed of Artemis II going around the far side of the moon, the moon finally rose from our location after midnight. Its phase was a waning gibbous three days after full. As such, the moon appeared bright and reddish, being low to the horizon. Through the 20mm we could see the whole disk, though the phase meant that for most of the lunar surface there was no contrast, making it harder to distinguish craters except for at the terminator.

Adding the 1.25-inch moon filter — more properly known as a neutral density filter that dims the incoming light — helped to limit the contrast and make the details stand out more. Switching to the 8mm eyepiece, with a magnification of 50x, the view jumped closer to the moon and the lunar surface filled the field of view, with bright crater rays visible on dark lunar mares.

Celestron Moon Mission 100mm Tabletop Dobsonian: Functionality

• Finderscope is awkward to use when pointed at the zenith
• Focusing is adequate
• Simple to use

The tabletop nature of the telescope poses some challenges for adults using it. As its name suggests, the telescope is designed to go on the top of a table. Usually when we think of Dobsonian telescopes, we think of very large instruments with very large apertures, and eyepieces close to standing height. This Dobsonian, on the other hand, is very small, and without a very tall table we found that we spent a lot of our time bent double looking through the eyepiece. Of course, this also means it is the perfect height for a child.

We found it did pose a problem when using the finderscope. For objects at low elevations, such as Jupiter in Gemini during spring 2026, we found it wasn’t too bad. However, when we wanted to direct the telescope towards Ursa Major at the zenith, the only way we could look through the finderscope was by literally getting on the floor to look through it. This is a problem with all tabletop telescopes, not just the Celestron Moon Mission, and it would be unfair to suggest otherwise — but it is a problem nonetheless.

Once we addressed the tightness of the focuser thumbscrews, we could switch the eyepieces in and out with ease. We found the focuser to be perfunctory. It provides only coarse focusing, with no careful fine-tuning, and sometimes it was tricky to find the sweet spot. Additionally, Newtonian reflectors like this one require collimating for perfect pin-sharp images. Collimating refers to adjusting the secondary mirror (the primary mirror is fixed at the base of the optical tube) so that it aligns and focuses light reflected from the primary just so. It’s also a fact that astronomers hate collimating, as it is a finicky procedure.

Out of the box, the collimation wasn’t bad, and we felt it was also unreasonable to expect beginners and children, whom this telescope is undoubtedly aimed at, to collimate the instrument with no guidance or tools included. Therefore, we reviewed the telescope as it came out of the box, to replicate the experience that beginners and children would receive. Had we collimated the telescope, then it probably would have improved the image a tad.

We found that actually using the telescope, in terms of positioning and pointing, was very simple. It’s worth remembering that Newtonian reflectors reverse their image (up becomes down), and after using smart telescopes, GoTo telescopes and Celestron’s StarSense telescopes with directions provided by a smartphone for so long, that took a little getting used to again! It may confuse beginners and children, but before the days of smart telescopes and GoTo, everybody had to get used to navigating across the sky using a reversed image, so it’s no bad thing.

Should you buy the Celestron Moon Mission 100mm Tabletop Dobsonian

If you want to introduce your children to astronomy, then the Celestron Moon Mission 100mm Tabletop Dobsonian is the perfect instrument. It is safe to use, with no risk of knocking something heavy over, as it weighs about the same as a bag of sugar, which is amazing really. It is simple to use, in the sense that it is just a matter of pushing and turning, although children might need assistance in pinpointing the location of targets. It’s also a fair all-rounder, as all Dobsonians are – it excels at showing the moon, displays the planets very well, and shows deep-sky objects as best it can for a 100mm-aperture telescope

If you want to see fainter galaxies and nebulae, then you will need a telescope with a larger aperture. If you want to do imaging, then you will need a telescope with a motorized equatorial drive to enable you to track the objects while imaging.

And if you want assistance in finding celestial objects without having to star-hop, then a GoTo or smart telescope might be best for you.

If the Celestron Moon Mission 100mm Tabletop Dobsonian isn't for you

If you're looking to spend less, Celestron offers a smaller Dobsonian, the Celestron Firstscope 76. For a more flexible telescope, take a look at the Celestron Inspire 100Z. Or if neither fits the bill, we've rounded up the best telescopes and best beginner's telescopes.

How we tested the Celestron Moon Mission 100mm Tabletop Dobsonian

We used the Celestron Moon Mission 100mm Tabletop Dobsonian during the occasional clear nights in the first two weeks of April 2026 from our south-facing garden in the United Kingdom. The temperature was clement, about 50 degrees Fahrenheit (10 degrees Celsius), with some modest light pollution to the north and dark skies to the south looking towards a more rural area.

We began observing after 10 pm, with the skies completely dark. The moon was near full at the time of testing — in fact, quite fittingly, one of the nights was the same night that the Artemis II mission went around the moon. However, the moon remained low the entire night, meaning it could only be viewed near moonrise after midnight, close to the horizon, before it became hidden behind a nearby bank of trees for the rest of the night.

If you've not seen the Milky Way this year from the Northern Hemisphere, it's time to make a plan. August's dark sky window opens around Aug. 6, when the moon begins to rise late at night as a waning crescent, meaning dark moonless skies for about 10 nights. That's when to see the Milky Way (and if you can time it for Aug. 12/13's Perseid meteor shower peak, all the better).

Five things are required to successfully see the Milky Way:

• the correct time of year (The brightest part is visible March-October)
• the correct moon phase (last-quarter moon through slim crescent moon)
• a dark sky away from light pollution
• dark-adapted eyes (stand in total darkness for 25 minutes)
• an idea of what you're going to see

The best way to dark-adapt your eyes is to start stargazing. Look south and begin picking out stars you know, paying special attention to the Summer Triangle. These three stars — Vega, Deneb and Altair — are your major signpost for finding the dense arc of starlight that will gradually emerge. Specifically, focus on the sky from Deneb through Altair — the left-hand side of the Summer Triangle — and you'll slowly see not only the Milky Way, but something else in front of it that few stargazers properly appreciate.

Sure, you can see the bright halo of gas and stars that indicate the center of the Milky Way galaxy, which is particularly bright below the Summer Triangle in the Sagittarius constellation. The closer you are to the equator, the higher in the sky, and the brighter, this region — known as the Galactic Center — will be.

Now look again. See those dark patches within the arc winding from Deneb to Altair? That's the Great Rift, so named because it appears to tear the Milky Way in half. It's an interstellar cloud of gas and dust (dark nebulas) between the solar system and the bright center of the Milky Way, which blocks and scatters visible light, essentially covering up bright stars and nebulas from our point of view. It looks like someone has spilled black ink across the Milky Way.

There are two ways of seeing the Great Rift. The most modern way is to observe it in infrared and radio light, which passes through the dust without being absorbed. This is exactly what some observatories are built to do, from radio dishes to the James Webb Space Telescope, which can probe the inner Milky Way — including the billions of stars in the center of our galaxy — which are on the other side of the Great Rift. Meanwhile, the new Vera C. Rubin Observatory has begun observing the entire visible southern sky every few nights over the course of a decade, mapping the Milky Way (including the Great Rift) to answer questions about its structure and formation.

The second way to see the Great Rift is to see it for what it is. Astronomers call the section we're looking at the Cygnus Rift, also called the Northern Coalsack, 1,000-3,000 light-years away in the constellation Cygnus. It's just below Deneb (which is 1,500 light-years distant), slightly outside of the Summer Triangle over an otherwise bright, dense region of stars called the Cygnus Star Cloud (around 2,600 light-years away). About six degrees in diameter, the Northern Coalsack blocks the light of background stars. However, it's just the northern tip of the Great Rift, which stargazers also call The Dark River or Dark Cloud.

Beyond the Northern Coalsack, however, the Great Rift is something to travel to see more of. It stretches across about 120 degrees of the night sky from Cygnus and Sagittarius in the Northern Hemisphere to Centaurus in the Southern Hemisphere. The latter is home to the famous Southern Cross and, besides its star Acrux, the original Coalsack Nebula. Another reason to travel to see more of the Milky Way is to appreciate how Southern Hemisphere cultures view the Great Rift. While modern astronomers see it as a dark cloud that needs to be peered through, indigenous cultures see its shapes. The Wiradjuri in Australia see the silhouette of an emu (its head is the Coalsack Nebula) and use its position in the night sky as a seasonal calendar. Meanwhile, the Inca in South America saw a llama (and, beside it, a baby llama).

The Great Rift is one of my favorite things to see, because it reveals what we're doing when we see that arc of light stretch across a summer night sky — we're looking at a galaxy from the inside, with all of its depth and complexity.

How and when I'm watching it

You do need perfect darkness and excellent timing. With that in mind, I'm trying out a new app called Milky Way Tonight, which is built around a useful question: is tonight actually worth the effort? It checks when the Milky Way core is above the horizon, then weighs that against moon phase, moonrise and moonset times, the local cloud forecast and the Bortle rating for your location. That last part matters. A technically clear night in a bright suburb is still a bad Milky Way night. The app also has a dark-sky finder, which is the feature I suspect I will use most.

Although the Milky Way has to be enjoyed as a naked-eye sight, it's also worth bringing along some binoculars to let you sweep across the dense star fields right up to the edges of the Great Rift.

Stargazer's corner: July 31-August 7, 2026

This is a good week to plan a trip to see the Milky Way and the Great Rift, but not to actually take that trip. Since the moon was recently full, our galaxy will be badly washed out for much of the night. That will make it difficult to see much of the Southern Delta Aquariids peak around July 30-31, as well as the now-active Perseids building toward their August peak. Saturn is worth a pre-dawn look, and Venus remains bright low in the evening sky if the horizon is clear, but if you're an astrophotographer or you have a smart telescope, you can use light-pollution filters to take advantage of nebula season — with key deep-sky sights being the Lagoon and Trifid Nebula (M8 and M20), the Little Sagittarius Star Cloud (M24) and the Wild Duck star cluster (M11).

Asterism of the week: The Coathanger/Brocchi's Cluster

The Coathanger looks exactly like its name. Also known as Brocchi's Cluster, it's a pattern of 10 stars in the small constellation Vulpecula, with six forming a straight bar and four making a curved hook. First find the Summer Triangle — Vega, Altair and Deneb — then scan roughly halfway between Vega and Altair. The small constellation Sagitta, the Arrow, points nearby, with the Coathanger just to its north. Dark skies may reveal it to keen naked eyes, but binoculars are the best way because they show the whole shape at once. One last thing: it's not a real coathanger! Once thought to be a cluster of stars born together, the shape is now known to be a chance alignment of unrelated stars at different distances — yet another cosmic illusion.

Looking forward to the 2026 solar eclipse, happening on Aug. 12? I know I am and even though it's not a total solar eclipse here in the UK (the path of totality crosses Greenland, Iceland and northern Spain), we'll still get to watch the moon obscure around 90% of the Sun, a sight that terrified our ancient ancestors.

However, you'll need proper eye protection, such as solar eclipse glasses, to watch the eclipse safely. Sunglasses are not sufficient for a solar eclipse; instead, you need eclipse glasses that follow ISO 12312-2:2015, the standard for solar viewers. If that number's not somewhere on the glasses, you're at risk of damaging your eyesight, maybe even permanently.

So, read on as we round up the best solar eclipse glasses to buy in the UK. Want a slightly better view? Here are the best places in the UK to see the partial solar eclipse.

• We've got you covered with reviews and rankings of the best telescopes, binoculars, star projectors, cameras, drones, Lego, streaming and more.

Venus dominates the evening sky throughout August, but early risers have a special treat too, as Mercury and Jupiter draw together in a beautiful dawn conjunction around mid-month.

From our vantage point on Earth, Venus reaches the end of its tether to the sun on the evening of Aug. 15, when it is at greatest elongation 46 degrees to the east of the sun. And yet, paradoxically, instead of appearing high up in the west, Venus is getting noticeably lower to the west-southwest horizon as the month progresses. This is because its declination in the sky is taking it well to the south of the sun. In fact, Venus's greatest elongation coincides with the time that it sets right at the end of evening twilight.

During the second half of August, into September, Venus will no longer be setting in a dark sky, but rather in a progressively brighter twilight sky. This is all due to its increasing southerly declination and the fact that the ecliptic — the apparent path of the sun, moon and planets through the zodiacal constellations — appears to slope closer to the western horizon at sunset during late summer and early fall.

The planet best positioned for telescopic observation this month is the "Lord of the Rings," Saturn, which comes up during late evening and is in a commanding position, well up in the south-southeast at the break of dawn.

Mars becomes evident a few hours before sunrise. During August, Earth approaches it at an average daily rate of 425,800 miles (685,100 kilometers). Still, even at month's end, Mars will be 172.2 million miles (277.1 million km) away, so while it continues to brighten, that process will still be quite slow.

Mercury and Jupiter are morning objects. Mercury will be evident during the first half of August, low in the east-northeast within about an hour of sunrise. It will be joined at midmonth by Jupiter as that big world emerges into view out of the glare of the rising sun.

In our schedule, remember that when measuring the angular separation between two celestial objects, your clenched fist held at arm's length measures roughly 10 degrees. Here, we present a schedule below which provides some of the best planet viewing times while directing you as to where to look to see them

Mercury

Mercury reaches greatest elongation from the Sun (19 degrees) on the morning of Aug. 2; it should be an obvious, +0.2-magnitude point low in the east-northeast if you look 50 minutes before sunrise. About a week later, look for Mercury very low in the east-northeast about an hour before sunrise. This small fleet world gets lower each dawn in early August, but it also rapidly brightens, from magnitude -0.7 on Aug. 9 to -1.3 (a trifle fainter than the brightest star, Sirius) by Aug. 16.

Also on Aug. 9, Castor and Pollux, the "Twin Stars" of Gemini, point directly toward Mercury. Just extend an imaginary line twice the distance between these two stars, down toward the east-northeast horizon and you'll come to Mercury. Early on the morning of Aug. 11, an exceedingly thin crescent moon — just 2% illuminated and about 32 hours from new (and a solar eclipse) — will lie about 2 degrees to the upper left of Mercury. From Aug. 13 through Aug. 17, Mercury will engage in a close interaction with Jupiter. Mercury arrives at superior conjunction with the sun on Aug. 27 and transitions into the evening sky.

Venus

Venus continues to outshine August's other evening stars and planets by a huge margin, brightening from magnitude -4.2 to -4.5 over the course of the month. It reaches its greatest elongation from the sun (46 degrees) on the evening of Aug. 15 and now resembles a roughly half-moon phase (48% illuminated) through a telescope. On the same evening, a three and a quarter day old crescent moon is poised to the lower right of Venus.

Mars

Mars rises around 2 a.m. local daylight time. When dawn breaks just over two hours later, it will stand 20 degrees above the east-northeast horizon. On the morning of Aug. 9, it can be found about 4.5 degrees to the right of a waning crescent moon.

Jupiter

Jupiter was in conjunction with the sun on July 29 and on Aug. 5, it is still too close to the sun to be visible without optical aid. But Jupiter appears two-thirds of a degree higher each morning and by Aug. 12, it should be visible about 5 degrees to Mercury's lower left shortly before sunrise, appearing dim in the bright twilight even though it shines at magnitude -1.8. Jupiter and Mercury shine less than 4 degrees from each other from Aug. 13 through Aug. 17.

Early on the morning of Aug. 15, the smallest and largest planets will meet in a close conjunction, with Jupiter shining about twice as bright as Mercury and separated by less than 0.6 degrees. However, seeing this tight pairing will be a challenge, as the duo lies just 12 degrees west of the sun and are up just 65 minutes before sunrise as seen from mid-northern latitudes. This majestic pair is about 10 degrees above the east-northeastern horizon at sunrise. You probably are going to need binoculars to fish them out against the brightening twilight sky. Still, it's worth the effort. After that, Jupiter moves rapidly off to Mercury's upper right, climbing into better morning view as its year-long apparition gets underway.

Saturn

Saturn rises a few hours after sunset, brightening in a lonely spot near the Cetus-Pisces border. In a telescope, its rings are tilted enough for good viewing; they narrow somewhat in the months ahead. Late on the evening of August 3rd, you'll find Saturn shining to the lower right of a gibbous moon.

If you're looking for a telescope or binoculars to observe the night sky, our guides for the best binocular deals and the best telescope deals are here to help. Interested in capturing the night sky? Check out our best cameras for astrophotography and best lenses for astrophotography.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

The full Buck Moon rose to delight and dazzle stargazers with a spectacular display of moonlight on July 29 and we've got the photos to prove it!

July's moon is also known as the full "Buck Moon" — a traditional name used by Native American tribes to reflect the time of year when young deer grow out their antlers. Sadly, the name didn't herald any dramatic transformation in the appearance of the moon, but it still made for a spectacular sight — and photo opportunities — as it climbed above the eastern horizon at sunset on July 29.

Here's a selection of spectacular photos of the July Buck Moon 2026 captured alongside gorgeous natural landscapes, terrifying wildfires and stunning cityscapes from around the world.

Best photos of the July 2026 full Buck Moon

Our first photo of the full Buck Moon comes courtesy of Mesut Karaduman, who captured a gorgeously framed view of a ballerina performing in front of the yellow-orange lunar disk on a hillside close to the city of Tekirdağ in northwestern Türkiye on July 29.

Sadly, the rising of the full Buck Moon was not a tranquil occasion for some in Europe, where its color was stained a deep crimson by the smoke from wildfires, which continue to ravage vulnerable areas in the wake of a prolonged heatwave.

Photographer Sergen Sezgin captured one such scene firsthand, as the moon rose over a smouldering hillside close to the Turkish city of Balıkesir, a few hundred miles south of Tekirdağ.

Kevin McCarthy captured this photo of the full Buck Moon as it glowed in the skies over North Carolina, with the dark profiles of lunar seas and bright pockmarks of craters scarring the lunar surface.

"I stepped out onto my driveway in Charlotte, North Carolina, at 11:15 p.m. to capture tonight's full Buck Moon," McCarthy told Space.com in an email. "The moon has a definite warm tint likely caused by its low position in the sky, causing the light to pass through thicker layers of the atmosphere. "

That same moon appeared warped by atmospheric disturbances when it rose above the city of San Francisco's Golden Gate Bridge on that same night, as a flock of birds flitted across its ancient surface in this photo from Tayfun Coskun.

Coskun captured another gorgeous scene of the moon rising over San Francisco on July 28, as the last of the day's sunlight kissed the tops of the surrounding hills, along with the tallest of the city's skyscrapers.

Mert Alper captured another image of moonrise being watched by a couple from Woodbine Beach in Toronto, Canada, as the lunar disk emerged from behind a dense cloud bank to brighten the evening sky.

Gary Hershorn, meanwhile, captured this magnificently timed view of the full Buck Moon as it shone at the pinnacle of Manhattan's One World Trade Center in New York on July 29 while looking over the Hudson River from New Jersey.

Our next atmospheric shot was taken with the aid of a telephoto lens by Ismail Kaplan during moonrise, as the lunar disk shimmered alongside Ankara Castle in the capital city of Türkiye.

This beautiful photo of the moon shining in the wheel of a young boy's bicycle was taken as the moon rose over the Zemplen Hills close to the Hunfarian town of Telkibánya that same night.

Finally, Izhar Khan was able to capture this impressive view of a bat's silhouette darkening the Sea of Tranquility and the Sea of Serenity as it flew through the night sky over Sydney, Australia.

The July 29 full moon is just the opening act for a spectacular month of skywatching events, kicking off with a jaw-dropping total solar eclipse on Aug. 12 that will be seen from Spain, Iceland and Greenland, which coincides with the peak of the Perseid meteor shower.

That's followed just two weeks later with a spectacular lunar eclipse that sees the moon fall deep into our planet's shadow, painting it a rusty-orange hue, weather permitting.

Be sure to check out our roundup of the best cameras and lenses for astrophotography to ensure that you're ready to capture next month's action-packed calendar of skywatching events, along with our guide to the best solar viewing gear available in 2026.

Editor's Note: If you would like to share your astrophotography with Space.com's readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.

The best smart telescopes have transformed astrophotography over the past few years, combining small telescope optics and automated mounts with dashcam-style camera sensors and image-processing software. The result? Compact devices that can be controlled entirely from a smartphone. Impressively, the DwarfLab Dwarf Mini pushes that concept even further.

Roughly the size of a thick paperback book, it’s one of the smallest smart telescopes yet produced — tiny enough to fit in a jacket pocket while still capable of imaging nebulae, star clusters, the moon and even sunspots. It's also one of the best telescopes for beginners.

Positioned below the larger Dwarf 3 in DwarfLab’s lineup, the Mini sacrifices aperture and resolution for portability. It uses a 30mm refractor paired with Sony’s IMX662 sensor and relies on automated stacking to gradually reveal deep-sky objects. The telescope connects to a phone via Wi-Fi or Bluetooth and handles alignment, tracking and imaging automatically through the DwarfLab app.

With built-in filters, optional equatorial tracking, and advanced software features such as Mega Stack and Stellar Studio processing, the Dwarf Mini is aimed at beginners and traveling astrophotographers who want a compact, automated imaging system that doesn’t require lots of extra kit — and works well even in light-polluted cities.

DwarfLab Dwarf Mini smart telescope review

DwarfLab Dwarf Mini: Design

• Ultra-compact 30mm refractor telescope
• Internal motorized filter wheel
• Magnetic solar filter
• Lightweight design
• Ideal for travel and eclipse chasing

The defining characteristic of the Dwarf Mini is its size. The body includes a 360-degree rotating base and an articulating lens arm that moves through 225 degrees, allowing the telescope to cover most of the sky. It's significantly smaller than its competitors, including the larger Dwarf 3, making it easy to pack for travel. In fact, it’s easily small enough to slip into a camera bag or carry-on luggage, making it an appealing option for traveling astrophotographers — perhaps including eclipse chasers preparing for the upcoming trio of total solar eclipses beginning in 2026, since a magnetic solar filter is included in the box. Nice touch!

The telescope itself is a 30mm f/5 refractor with a focal length of 150mm. This produces a field of view of about 2.4 degrees, roughly five times the apparent diameter of the full moon. That optical system is paired with a Sony IMX662 sensor, a 1/2.8-inch sensor capable of 2.1MP resolution (1080p). This sensor is all about low noise and sensitivity, making it well-suited to short astrophotography exposures, but not to high-resolution images. Compared with the Dwarf 3’s Sony IMX678 Starvis 2 sensor, which delivers 8.3MP and 4K resolution, the Mini is a step down in terms of detail. However, in practice, the difference is smaller than expected, particularly after image stacking and processing.

The device also features a motorized internal filter wheel, allowing users to switch between broadband and dual-narrowband filters directly in the app to mitigate light pollution and better image nebulae. This avoids the need to install external filters, which are an add-on accessory with some smart telescopes.

The box includes a magnetic solar filter, a USB-C charging cable and a lens cloth. However, a small tripod is not included in the box, which feels like an omission given the Mini’s travel-friendly design. That's not a deal-breaker since any small tabletop (or full-size) tripod can be used, but the all-in-one feel is sacrificed.

DwarfLab Dwarf Mini: Performance

• Reveals deep-sky objects even under light pollution
• Plate-solves stars and stacks short exposures
• Mega Stack combines data from multiple sessions

The Dwarf Mini performs surprisingly well considering its small optics. During testing, it proved capable of capturing bright deep-sky targets such as the Orion Nebula (M42) and the Pleiades (M45), as well as open clusters like M44, even from suburban skies.

Smart telescopes compensate for small apertures by stacking many short exposures over time, gradually building up a deeper image. In standard alt-az mode, exposures are typically limited to around 10-15 seconds to prevent field rotation (which can cause blur). This technique allows the telescope to perform well even under heavy light pollution and/or strong moonlight, making it particularly useful for urban astronomers, where the chance of seeing faint nebulae is virtually zero.

One particularly useful feature is Mega Stack, which combines multiple imaging sessions of the same targets. Instead of capturing everything in a single session, data from several shorter sessions can be added later — even months or years later — to produce deeper images. That's handy when windows of clear skies are few, or if you plan occasional trips to dark skies where better data might be possible.

For more advanced imaging, the telescope also supports an equatorial (EQ) tracking mode, something professional astrophotographers insist upon. EQ mode may not be essential on a travel-friendly smart telescope like this, but its inclusion is impressive. It requires the purchase of an equatorial wedge, such as Dwarf Mini’s Mini Tripod accessory, which we were not able to test during this review. After a simple alignment with Polaris, the mount tracks the sky’s rotation, allowing exposures of up to 90 seconds. It can make a marked difference with very faint targets — though it’s not an essential feature on a smart telescope aimed at beginners.

Daytime performance is also strong. With the included solar filter, the Mini easily captured sunspots and solar activity, while lunar images also showed impressive crater detail.

The main limitation is resolution. The 2MP sensor produces images that look excellent on smartphones and social media, but they lack the detail needed for large prints or serious astrophotography. But for a telescope this small, the results are genuinely impressive.

DwarfLab Dwarf Mini: Functionality

• Smartphone control via Wi-Fi or Bluetooth
• Sky Atlas feature for automatic target selection
• Manual pointing and mosaic imaging modes

The Dwarf Mini is designed to be controlled entirely through the DwarfLab smartphone app, which connects via Wi-Fi or Bluetooth.

Once connected, users can browse a built-in sky atlas, which displays objects currently visible from their location. Selecting an object prompts the telescope to plate-solve the surrounding stars, automatically align itself, slew to the target and begin stacking exposures. Imaging sessions can be stopped at any point if you’re happy with the result so far. The app also displays session details such as exposure count and total integration time.

For users who want more control, the telescope can also be manually aimed at any patch of sky, which is particularly useful when imaging newly discovered comets or objects not yet included in the atlas database. For objects larger than its field of view, such as the Andromeda Galaxy (M31), Mini has a mosaic mode, which allows the telescope to capture multiple adjacent frames and stitch them together.

Captured images can then be processed using Stellar Studio, DwarfLab’s built-in image processing software, which is very good at removing noise and adding contrast. Images can be saved in JPG, TIFF or FITS formats, giving beginners a set of sharing-friendly options and more advanced users the chance to download files into desktop processing software.

It’s all remarkably easy to operate once you’re comfortable with how the app works. Beginners can capture solar, lunar and deep-sky images within minutes of set-up, while more experienced astrophotographers can still access advanced features such as EQ tracking and mosaic imaging.

Firmware updates are frequent and install easily through the app, so it’s worth connecting the telescope to your home Wi-Fi before heading to a dark-sky site — you never know when new features will appear!

Should you buy the DwarfLab Dwarf Mini smart telescope?

The DwarfLab Dwarf Mini offers a tempting combination of portability, automation and surprisingly capable astrophotography performance. It won’t replace a full astrophotography setup, but for beginners, urban astronomers, travelers and eclipse chasers, it provides an easy way to capture the night sky — and the sun — without bulky and expensive equipment.

If the DwarfLab Dwarf Mini smart telescope isn't for you

If you're after something with a little higher resolution, the DwarfLab Dwarf 3 is a larger, more powerful version with a 4K sensor and a slightly larger aperture.

ZWO Seestar S30 is a similar smart telescope with automated tracking and an included tabletop tripod, though it's recently been surpassed by the slightly pricier ZWO Seestar S30 Pro, a higher-resolution alternative that boasts superior optics and imaging.

For an overview of the top telescopes in this category, read our 2026 guide to the best smart telescopes.

User reviews

Online reviews of the Dwarf Mini often highlight its portability, simplicity and image quality. One reviewer described it as a “great piece of kit for deep space astrophotography.”

Another wrote: “I had no trouble getting it imaging within a few minutes out of the box,” praising the image quality, autofocus, GoTo accuracy, tracking, and the app. “It's a brilliant piece of kit,” said another user.

However, several users also reported poor quality in planetary images — and that’s certainly true (though it can find the moons of Jupiter).

How we tested the DwarfLab Dwarf Mini smart telescope

Our observations took place on a few clear nights during February and March 2026, in temperatures down to lows of 43 degrees Fahrenheit (6 degrees Celsius) and highs of about 54 F (12 C). Light pollution was between 5 and 6 on the Bortle scale — urban conditions with bright city lighting. Battery life averaged around 4 hours, though longer imaging sessions were supported using an external USB power bank connected to the telescope's USB-C slot.

Editor's Note: The full "Buck Moon" charged into the summer sky on July 29 to to dazzle stargazers with a gorgeous display of natural moonlight and we have the photos to prove it! Check out our wrap article to see jaw dropping photos of the July 2026 full moon captured from around the world.

The July full "Buck Moon" rises tonight to lead Saturn, Mars and Mercury in a spectacular mini planetary parade through the summer sky. Here's what you need to know.

July's full moon phase occurs at 10:36 a.m. EDT on July 29 (1436 GMT), when the lunar disk will appear fully illuminated. It's often called the Buck Moon, to reflect the time when young male deer grow out their antlers. It has also been named the Berry Moon by the indigenous Anishinaabe people and as the Thunder Moon by the Western Abenaki people, according to the Old Farmer's Almanac.

Look to the southeastern horizon at sunset to catch the full Buck Moon as it creeps slowly into the summer sky. The moon may appear particularly large at moonrise thanks to a phenomenon known as the "Moon Illusion", where our brains trick us into perceiving it as larger than it actually is while close to the horizon. You might also see it adopt a yellow-orange hue as Earth's atmosphere scatters the bluer wavelengths of its light as it travels low in the sky.

Sunlight strikes the moon head on during July's full moon phase, leaving no shadows to emphasize the presence of the countless craters that litter the lunar surface. It's a perfect time to explore the dark lunar seas that scar the moon's surface, where ancient lava flows once flooded networks of impact basins, then hardened billions of years ago, repaving vast swathes of Earth's natural satellite.

Grab a pair of binoculars or a telescope and look a little closer. You'll find a network of bright streaks intersecting as they travel outward from youthful impact craters. These features are known as ejecta rays, and were created when material cast out in violent impacts fell back onto the lunar surface. Every crater on the moon once had its own set of ejecta rays. However, all but the most recent have since faded into obscurity due to space weathering.

Venus will appear as a bright evening star to the west after sunset, serving as the opening act for a magnificent planetary procession in the hours that follow. Saturn, Mars and Mercury will rise in the east to trail the moon in a majestic arc as it treads a ponderous path from east to west through the summer sky.

Want to capture the incredible predawn lineup for yourself? Then be sure to check out our guide to photographing the planets, along with our expert tips on photographing the moon. You can also read our roundup of the best cameras and lenses for astrophotography to ensure that you're ready for the next big skywatching event.

Editor's Note: If you would like to share your astrophotography with Space.com's readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.

Correction 7/29: Look to the southeastern horizon at sunset to catch the full Buck Moon, not the southwestern horizon.

An astrophotographer captured a breathtaking scene as the International Space Station zoomed by Venus in the daytime sky.

What is it?

Photographer AJ Smadi set up the scene on July 18 in a park near Seattle, Washington. Smadi used a 9.25" (23.5 cm) Celestron Schmidt-Cassegrain Telescope and a ZWO ASI662MC camera equipped with an ultraviolet and infrared filter to capture the incredible image.

But this isn't the first time Smadi has pulled off such a feat. Just over a year ago, the photographer captured the ISS beside Venus in a photo that was selected by NASA as one of its Astronomy Photos of the Day.

"The thing that inspired me to capture Venus with the ISS is the fact that nobody has done it before," Smadi told Space.com by email. "After having realized this in April 2025 following my first time capturing the pair together, I was determined to best my own achievement," Smadi said.

Smadi regularly photographs the ISS but says the clarity differs greatly depending on the stability of the air and its distance.

Why is it incredible?

Capturing Venus, the ISS, or any other object in space (other than the moon) during the daylight hours takes careful planning and a deep understanding of astrophotography techniques and filters.

The ISS travels at a mind-boggling 4.6 miles per second (7.5 km per second) and is 84 million miles (135 million kilometers) away from Venus, so lining up a photograph of the two seemingly side-by-side is no easy feat and takes painstaking planning.

For more of AJ Smadi's work, including photos of the ISS transiting the sun, the moon, and passing by Saturn, visit his Instagram.

ZWO is well known for its Seestar smart telescopes but they also make dedicated astronomy cameras for use with telescopes to get highly detailed astrophotography. We have reviewed three of these ZWO astrocams and they have delivered beautiful images of the different objects.

The color cameras like the ZWO ASI183MC Pro and ZWO ASI533MC Pro have delivered beautiful colored detail in galaxies and nebulas, whereas the monochrome ZWO ASI175 mono delivered exceptional solar photography.

Explore the ZWO range on sale at B&H Photo and Video, with the ZWO ASI183MC Pro, ASI153MC Pro and ASI175 mono astronomy cameras 10% off.

An astronomy camera has only one job: To be good at astrophotography, nothing else. They are essentially just camera sensors but full of features that only benefit astro. It has active cooling for reducing image noise, no infrared (IR) cut filter to allow nebula colors in Hydrogen-alpha to be captured and a range of different things that sharpen every aspect of image capture during astrophotography. If you want to start using an astrocam, you will need optics to use with your astrocam, so grabbing a telescope or a special astrophotography telescope is essential.

• We've got you covered with reviews and rankings of the best telescopes, binoculars, star projectors, cameras, drones, Lego, streaming and more.

Professional astrophotographer Damian Peach gave strong ratings to these astrocams for their performance in capturing deep-sky targets such as the Orion Nebula (M42), the galaxy NGC 6946 and the planet Jupiter.

He said both the ZWO ASI183MC Pro and ASI533MC Pro are suitable for those looking to get a dedicated multi-use camera for astrophotography, including deep sky objects and short exposure lunar and planetary photography. The ASI533 is the pro choice, as it features newer sensor technology with zero amp glow circuitry, decreasing the need for dark frame captures like with the older ASI183MC.

Astronomy expert Jamie Carter tested out the ZWO ASI174mm mono camera to photograph the solar surface, along with a Sky-Watcher Heliostar 76mm and Solar Quest mount. He was able to capture some incredibly detailed images of the solar surface, showing features like sunspots, filaments and prominences.

You should grab a monochrome camera like this if you are interested primarily in getting solar, lunar and planetary photography. They can capture more detail in these objects than color astronomy cameras and then color can be corrected in post-processing.

Check out our other guides to the best telescopes, binoculars, cameras, star projectors, drones, lego and much more.

One month from today, skywatchers across the Americas, Europe and Africa will have the chance to witness the best lunar eclipse until New Year's Eve 2028.

On Aug. 28, Earth's shadow will cover up to 96% of the moon's disk in an exceptionally deep partial lunar eclipse. At maximum eclipse, only a thin sliver of the moon will remain outside Earth's darkest shadow, creating an "almost blood moon" with nearly the entire lunar surface glowing a deep reddish-orange.

Unlike a solar eclipse, a lunar eclipse is completely safe to observe with the naked eye and requires no special equipment. All you need is clear skies and a view of the moon.

Where can I see the lunar eclipse?

The eclipse will be visible across Europe, Africa, the Americas and parts of western Asia, though exactly what you'll see depends on your location.

The Americas are particularly well-placed to catch the eclipse's most dramatic stages, as many locations will see the moon rise already deep within Earth's shadow. Across eastern North America, observers will see the "almost blood moon" climb above the horizon shortly before or during maximum eclipse.

Across Europe and Africa, the eclipse occurs before dawn on Aug. 28. Observers in the U.K. and western Europe will see the moon low in the western sky during the final stages of the eclipse, before it sets shortly after maximum. Farther east, progressively less of the eclipse will be visible before moonset.

• North & South America: Best overall views
• Europe & Africa: Excellent predawn moonset eclipse
• Western Asia: Limited views before moonset
• Eastern Asia: Little or no visibility.

What will it look like?

Because 96% of the moon will pass through Earth's central dark shadow, known as the umbra, this eclipse is expected to look remarkably similar to a total lunar eclipse or a "blood moon" lunar eclipse. The moon will likely take on a deep coppery-red hue with only a narrow bright silver lining remaining.

Follow along with Space.com

Over the coming month, Space.com will bring you everything you need to prepare for eclipse night. From viewing guides and photographing the event to a live blog bringing you the latest news and action from the best lunar eclipse until NYE 2028. We'll also be releasing details on how you can watch the eclipse online if you're unable to catch it in person.

Smart telescopes like the Seestar S30 Pro have changed astrophotography and, arguably, urban astronomy. The Seestar S30 Pro takes that concept further than most. Small enough to fit inside a camera backpack, it combines a refractor telescope, motorized mount, dual cameras and image-processing software into a compact unit controlled entirely from a smartphone. Within minutes of powering on, it can align itself to the night sky, slew to a specified target and begin stacking exposures to reveal galaxies, nebulas and star clusters — even from light-polluted locations.

It makes astrophotography — once a complex and expensive hobby — possible with a single, automated device, though what makes the Seestar S30 Pro particularly interesting is not just its simplicity, but how it changes the experience of observing. Instead of actively operating a telescope, users watch a digital image build in real time. Sure, your eyes don’t see the photons coming from distant galaxies, but that misses the point — urban astronomers can’t see much of those galaxies anyway when using an optical telescope.

Positioned as an upgrade to the original Seestar S30, it introduces higher-resolution 8.3MP imaging, equatorial tracking support and expanded imaging modes aimed at more advanced users.

Designed for beginners, urban astronomers and astrophotographers of any level who are looking for a portable rig, the Seestar S30 Pro is about convenience, capability and a different way to explore the night sky.

ZWO Seestar S30 Pro smart telescope review

ZWO Seestar S30 Pro: Design

• Lightweight design
• Dual-camera system
• Full smartphone control

At first glance, the Seestar S30 Pro barely resembles a telescope, being closer in size to a telephoto lens than a traditional optical instrument. That portability is one of its defining strengths — this is a telescope you can realistically take anywhere, whether into a backyard, onto a balcony or on a dark-sky trip. You could even take it as hand luggage on a trip to see a total solar eclipse in a distant land.

The design is deliberately minimal. Aside from a power button and USB-C slot, there are no physical controls. Everything — from slewing and focusing to image capture and processing — is handled through the Seestar app. Once connected to a phone via its own WiFi network, the system operates entirely offline, connecting directly to your phone without requiring an internet connection in the field.

A key feature of this new, improved model is its dual-camera system. The primary telephoto camera is dedicated to deep-sky imaging, using a Sony IMX585 sensor that’s capable of 8.3MP (4K) images, while the secondary wide-angle uses an equally capable Sony IMX586 sensor for sky alignment and wide-field imaging modes.

The included tabletop tripod is solid, if small, so users with backyards surrounded by buildings or trees will benefit from mounting the device on a full-size photographic tripod. It also comes with a handy, high-quality padded shoulder bag to store the telescope and all its accessories.

ZWO Seestar S30 Pro: Performance

• Automatic stacking with intelligent frame rejection
• EQ mode enables longer exposures
• Strong results under urban/suburban skies

Using the Seestar S30 Pro is less about operating equipment and more about using an app. After powering on and connecting via WiFi, the telescope automatically plate-solves the stars overhead, determines its position and slews to a selected target. Within minutes, it begins capturing short exposures — typically around 10 seconds — which are stacked in real time to reduce noise and improve detail. Crucially, the system automatically discards poor-quality frames caused by tracking errors, wind shake or star trailing.

The effect of the image stacking is gradual. As more data is collected, a faint patch of light slowly resolves into a nebula or distant galaxy. The longer the telescope runs, the clearer and more detailed the final image becomes, with nebulosity and spiral arms becoming visible. Stars remain sharp across the field of view — the Seestar S30 Pro’s optics may be small, but they are excellent quality. During our test, we produced some superb images of the Orion Nebula (M42), as well as Bode’s Galaxy (M81) and the Cigar Galaxy (M82), the Whirlpool Galaxy (M51) and the Great Globular Cluster in Hercules (M13).

Stacking images is a hugely effective way to do observational astronomy under light-polluted urban skies. By stacking multiple exposures and applying built-in filters (there are three), the Seestar S30 Pro can reveal objects that would otherwise be invisible through the eyepiece of a traditional optical telescope.

The all-new equatorial (EQ) mode extends performance further, though aligning the telescope with Earth’s rotation requires purchasing the add-on Seestar TH10 Fluid Tripod Head. This is easy to set up, thanks to an in-app setup process that perfectly positions the tripod and ball head. With Expert Mode engaged, exposures of up to 60 seconds are possible. We tried it on two faint targets — the Whirlpool Galaxy (M51) and the Great Globular Cluster in Hercules (M13) — and got much greater detail.

Planetary imaging is less impressive, with planets appearing small and lacking fine detail. That said, we did manage to image Jupiter and its moons. The telescope is clearly optimized for deep-sky imaging rather than solar system work — the exception being the moon, which looked fabulous through the Seestar S30 Pro.

ZWO Seestar S30 Pro: Functionality

• Intuitive smartphone app
• Automated imaging and Plan mode
• Built-in processing and FITS export

The Seestar app is central to the entire experience. It acts as both controller and processing platform, offering a planetarium-style sky atlas that displays objects visible from the user’s location. Selecting a target triggers automatic alignment, slewing and image capture. Once imaging begins, the app displays real-time progress, including exposure count and total integration time. Users can stop a session at any time or continue it for deeper results. The telescope can operate largely unattended, making it easy to leave running and check later.

If all of this is beginning to sound like the Seestar S30 Pro is ideal for lazy astronomers, it doesn’t end there. Cue the app’s Plan mode, which allows users to schedule multiple targets for imaging overnight. Orion Nebula not rising until 3 a.m.? No problem. Pre-sunrise comet? Stay in bed. Assuming you’ve checked for clear skies beforehand, the Seestar S30 Pro can observe while you sleep. However, Plan mode does come with limits: exposure time and gain cannot be fine-tuned per target, so users must rely on default settings. For most, that won’t deter.

For those interested in post-processing, the Seestar S30 Pro supports FITS file export, enabling images to be refined in external software such as Siril, PixInsight, DeepSkyStacker or Photoshop (though advanced users dealing in FITS files may find that the system’s 128GB internal storage needs frequent attention). Alternatively, the built-in Deep Sky Stack provides quick results with minimal effort, allowing frames to be discarded and the effective AI Denoise pipeline to be engaged — something that takes a little patience, but delivers excellent results.

How we tested the ZWO Seestar S30 Pro

Testing took place over multiple nights during late winter and early spring, under suburban Bortle 6 skies in cold but not freezing temperatures. It was also used in Bortle 2 skies in sub-zero temperatures, with no ill effects on the 6-hour battery life. The telescope was used to image a variety of deep-sky objects, with sessions ranging from short captures to integrations lasting several hours. Both standard alt-az mode and EQ mode were tested.

Should you buy the ZWO Seestar S30 Pro?

The Seestar S30 Pro is best understood not as a traditional telescope, but as an automated imaging system designed to make astrophotography accessible. It’s also an upgrade on the Seestar S30 that may or may not be worth the money, depending on your needs.

For beginners, it provides a clear pathway into astrophotography without the usual financial or technical barriers. For more advanced users, it’s an efficient grab-and-go system for casual or supplementary imaging.

If the ZWO Seestar S30 Pro isn't for you

If you’re looking for a more affordable entry point, the ZWO Seestar S30 offers similar ease of use, but with lower (2MP) resolution and fewer advanced features. For those who simply want basic, shareable images, it remains a strong alternative.

The DwarfLab Dwarf Mini is even smaller and more portable but it is limited to 2MP imaging. At the other end of the market, the Unistellar Odyssey is a premium smart telescope offering much larger apertures and access to citizen science campaigns, albeit at significantly higher prices.

For an overview of the top telescopes in this category, read our guide to the best smart telescopes.

There is a particular moment every July when the night sky makes perfect sense to me. Every time I step outside at night, I instinctively look overhead for the Summer Triangle. Not because it's the most spectacular sight in the sky. In fact, the vast asterism is almost suspiciously simple: three bright stars, large enough to cut through twilight and light pollution without much effort.

Experienced stargazers quietly depend on the Summer Triangle more than we admit. People imagine astronomy involves memorizing the entire sky at once, knowing exactly where each star is and what it's called. Everyone navigates differently, but we all rely on familiar anchor points because the night sky changes quickly with the seasons.

The Summer Triangle is one of the best anchors because it appears exactly when the northern sky can otherwise feel vague and washed out during late twilight. Once those three stars appear, I immediately know where everything else is. The Milky Way becomes easier to trace. The darker regions of the sky reveal themselves. Constellations stop looking random. Suddenly, I know where the Perseids will emerge from later in the night and where to point binoculars to find summer's dense star fields without even thinking about it.

The Summer Triangle also teaches you how to see the night sky. To the untrained eye, the night sky appears as a flat backdrop of stars — hence the "blanket of stars" saying. Every time I hear that cliche, I wince. There is no blanket! The night sky has incredible depth, and there's nowhere better to learn how to appreciate that than when gazing at the Summer Triangle.

Take Altair, the lowest star. It's relatively nearby at about 17 light-years away. It shines brightly largely because it is close to us. Vega lies slightly farther away at roughly 25 light-years, but it is intrinsically far more luminous. It once served as Earth's North Star thousands of years ago and, thanks to our planet's slow axial wobble, will become the North Star again many millennia from now. So far, so local — we're in the sun's backyard with these two stars. The light from both of them began its journey to us this century.

Then there's Deneb. Deneb is so distant — roughly 2,600 light-years away — that the fact it appears this bright at all becomes genuinely difficult to process. Its light began traveling toward Earth while the Roman Empire was still in existence. The only reason it remains prominent in our sky is that Deneb is an enormously luminous supergiant radiating tens of thousands of times more energy than the sun.

Knowing this about Deneb transforms the Summer Triangle into a three-dimensional shape. Here are three stars that appear neatly connected overhead, but in reality, one is separated by an incomprehensible distance. So next time you look at the Summer Triangle, keep Altair and Vega at the front and push Deneb way, way back. It's not a triangle anymore — it's an arrow pointing far into the distance, thousands of light-years away into the starfields of the distant Milky Way.

What's happening and when to look

This week is the perfect time to reacquaint yourself with the Summer Triangle using just your naked eyes. Around 11 p.m. local time at mid-latitudes of the Northern Hemisphere, look high in the southeast. Vega is usually the first to appear, high and brilliant with a slightly blue-white color. To its lower left sits Deneb. Farther south is Altair. By midnight, the entire Summer Triangle stands high overhead and remains one of the defining features of the northern summer sky through October.

Stretching directly through it is our view into the Orion Arm of the Milky Way — the spiral arm of the galaxy containing the solar system itself — while farther south, the glowing river of starlight continues toward the galactic core near the constellations Sagittarius and Scorpius, low on the horizon. Under dark skies, the Milky Way visibly streams behind Deneb and through Altair like a river of stars.

How and when I'm watching it

Once I start slowly sweeping binoculars through the Summer Triangle, I usually lose all sense of structure and planning. Dense star clouds spill into view everywhere. Dark lanes slice through the Milky Way. Tiny clusters appear almost accidentally. The region between Deneb and Altair may be my favorite casual binocular territory in the entire sky.

Inside the Summer Triangle itself lies the Cygnus Star Cloud, one of the richest naked-eye sections of the Milky Way visible from northern latitudes. Nearby are the Ring Nebula and the Dumbbell Nebula. The beautiful double star Albireo — one bright yellow and the other a fainter blue — sits at the beak of Cygnus, the Swan.

I'll also look for a couple of smaller constellations within and around the Summer Triangle — Delphinus, the Dolphin, hovers to the left of Altair, while tiny Sagitta, the Arrow, hangs above Altair, looking improbably compact.

That's another thing the Summer Triangle taught me — astronomy improves dramatically once you stop hunting objects individually and start exploring regions instead. It's armchair travel of the grandest kind.

If you're looking for a telescope or binoculars to observe the night sky, our guides for the best binocular deals and the best telescope deals can help. Our best cameras for astrophotography and best lenses for astrophotography can help you get ready to capture the next stunning skywatching event.

Stargazer's corner: July 24-31, 2026

The moon will move beneath the Summer Triangle this week, appearing as an 81%-illuminated waxing gibbous moon as it shines close to supergiant star Antares in the constellation Scorpius, on Friday, July 24. By now, the moon is dominating the night sky, albeit low on the horizon, and on Wednesday, July 29 — the night before the full Buck Moon — the Summer Triangle will appear to point straight at it. Late July also marks the gradual strengthening of the Perseid meteor shower, with occasional early meteors now appearing after midnight. The Southern Delta Aquariids and Alpha Capricornids peak around Thursday-Friday, July 30-31, though the full moon will reduce visibility of fainter meteors considerably.

Constellation of the week: Sagitta

Sagitta, the Arrow, is one of the smallest constellations, but also one of the easiest to recognize once you've found it. It appears as a short line of five stars — all between 450-650 light-years distant — with an arrowhead, shaft and two stars as the fletchings. It's between Cygnus and Aquila.

It's not bright, but it's well-defined, and once you spot it, it becomes a reliable reference point. Learning these smaller constellations helps fill in the gaps between the more obvious patterns.

In a rare first for me, I actually used autofocus for this entire astrophotography shoot. If I'm being honest? I prefer it when shooting astro with a mirrorless camera. Why? Because it is quicker and that means more time capturing the stars and less time setting up. I can get a star in sharp focus using autofocus in half the time that it would take me to do it manually and it's way easier to focus with the shutter or back button than play about with the focus ring, especially with cold fingers.

I only managed to get out under one clear sky to test the new R6 III but it was a wonderful session at my usual dark hill spot surrounded by a sea of stars and celestial shapes. After setting up my tripod, I was ready to start shooting, armed with the Canon 14mm f/1.4 and 45mm f/1.2 lenses.

If you are a seasoned astrophotographer, you will undoubtedly have started your craft by learning how to manually focus on stars to get them crisp and sharp in the frame. Everyone does. Whilst the manual focus (MF) versus autofocus (AF) debate continues within the community, the technology for low-light autofocusing capability has come a long way since mirrorless cameras were first introduced and the R6 III is physical proof of that.

The astrophotography

You only get the luxury of being able to do this if your camera is actually good at autofocusing in low light and for starry nightscapes. All three versions of the Canon EOS R6 feature a low-light autofocus range of -6.5 exposure value (EV), so they already have a strong baseline for shooting under dark skies. The Canon EOS R6 III features a higher resolution and advanced autofocus algorithms, so the AF system actually has more data to use and is better at using it.

I was able to capture bright objects easily and start shooting without having to spend ages using manual focus for each new shot. The autofocus was powerful enough to capture at least one star in each of my frames. I simply used autofocus on the brighter points of light in my composition, waited for the green box and then switched to manual to avoid any refocusing if I decided to recompose the shot.

Bright objects were the easiest to capture, with Jupiter, Pollux and Castor easily captured in the western sky. Light pollution washed out the contrast in this shot but it was the quickest autofocus because of the brightness of the objects.

The autofocus helped me capture a range of other constellations too. With the R6 III focusing on the bright star Arcturus, along with the rest of Boötes and Coma Berenices next to the Coma Star Cluster (Melotte 111).

The shape of Leo is recognisable and the autofocus captured the brightest star, Regulus, to bring the rest of the stars in the constellation into focus. You can even spot the Beehive Cluster (M44) in Cancer, to the right of the frame and it is fairly sharp in focus. Barring some minor star trailing from my lack of a star tracker, the stars are nicely in focus, including on minor objects like star clusters.

Using the 45mm lens, I got some close-ups of some quadrilateral shapes in the sky. Hercules' prominent trapezoidal keystone is visible and one of the corners, Zeta Herculis, was picked up by the autofocus. It is not exactly a bright star, with a magnitude of 2.88, but the R6 III picked it up easily and brought the rest of the corners into focus. Whilst barely a smudge along one of the sides of Hercules, I even managed to capture the Hercules globular cluster (M13) with the R6 III and the Canon RF 45mm wide open at f/1.2.

The polygonal head of the dragon in Draco was easily captured in the centre of the frame, with bright stars Eltanin (2.23), Rastaban (2.79) and even Iota Herculis (3.8) showing prominently. The autofocus capabilities of the EOS R6 III are maximised when used alongside a lens with a very fast aperture like f/1.4 and f/1.2. Without these types of lenses, you would be much less likely to be able to autofocus on such dim stars.

The upgrades

The big question when looking at the third iteration of a camera model is to figure out if the upgrades are actually worth it. First, you have to think about your budget and also what you are using the camera for. For astrophotography, there are a few upgrades in the EOS R6 III that can be considered to see whether they are worth it.

The most noticeable upgrade on the R6 III is the resolution, which has been upgraded from the R6 II's 24.2MP sensor to a 32.5 MP sensor. On top of improved resolution for general and astrophotography, the boosted number of pixels allows the Dual Pixel CMOS AF II to collect even more data points because there are more pixels. Dual Pixel architecture splits each pixel into two separate photodiodes and allows each photodiode to read the light from the star at two different positions and allows the lens motor to bring those points together into perfect focus.

The upgraded sensor resolution combined with upgraded tracking algorithms from the flagship Canon EOS R5 II make the R6 III better at locking onto low-light points and make autofocus for astrophotography much more reliable than in previous models.

I initially expected the higher resolution to translate into more image noise on photographs but this was not the case. The R6 III utilizes dual-gate gain architecture, which means that every pixel has a switchable path at the hardware level depending on the ISO level used and allows images with higher ISOs to have a heavily reduced base amount of noise and thus makes them less grainy.

Photos at lower ISOs on the R6 III have an incredibly high dynamic range (HDR) thanks to the low conversion gate (LCG) circuit. This allows the natural color of the stars to be preserved instead of coming across as indeterminate white blobs, as well as the subtle hues of the dark surrounding sky in the photograph.

Aside from the technical aspects of how the resolution improves the autofocus, the detail in images from the R6 III is noticeable and is great for picking up finer stellar structures such as star clusters and smaller stars. When paired with a distorted lens like the Canon RF 7-14mm f/2.8-3.5 fisheye lens, extra resolution really helps details pop. I didn't get to use the fisheye lens for astro but general daytime shooting delivered some high-quality photographs.

The final important upgrade on the R6 III is the inclusion of a CFexpress card slot, which allows faster writing and reading speeds both in camera and during media downloads. A UHS-II SD card has an average read speed of 300MB/s and an average write speed of 260MB/s.

This may seem fast but the most advanced CFexpress cards have a read and write speed of over 3000MB/s, which makes huge workloads so much easier to process. This may only be of benefit to professional photographers who shoot a lot of video or need to do a huge amount of burst photography in RAW format, but it does vastly improve the performance of this camera. Bear in mind that CFexpress cards are much more expensive than SD cards and require an additional CFexpress reader to transfer data to a computer.

Is it worth it?

The price difference between the R6 Mark II and the Mark III is just under $1000 and for that amount of money, justifying the move up to the latest model comes down to a few factors that you will have to consider. The power of the low-light autofocus is tempting but you should think about the camera as a whole to see whether it is worth making the investment.

If you are looking to boost resolution in your night-time scenes and have been shooting astrophotography for a long time, the R6 III could be worth the extra investment thanks to the 32.5MP sensor, which retains the powerful dual-gain architecture for getting high dynamic range images at lower ISOs and delivering high ISO images with significantly less grain.

If you have a heavy workflow, you are likely to be frustrated with the lack of a CFexpress card slot on the earlier R6 models and would benefit from the advanced functionality the new slot will give you, especially if you shoot a lot of RAW imagery and video.

Stick with an earlier model or a different mirrorless camera if you are a very casual astrophotographer who does most of your shooting in the daytime. I just can't justify the massive jump in price for basic shooting, where a beginner or intermediate photographer's money might be better spent on getting a fast f/1.4 lens for superior astro. I used the Canon RF 14mm f/1.4 lens for astrophotography testing and I don't think the images would have looked half as good if I had used a lens with a smaller aperture. If you already own the R6 II, the only reason you might upgrade is if you need to do more heavy cropping into your images or need better hybrid video functionality from a camera.

Picture it: A slash of vivid green light splits the starry sky. There for a moment and then gone, leaving nothing but a short-lived glowing trail and a moment of pure joy. You've finally caught it, your first Perseid shooting star of the season.

What you saw was the final moment of a story billions of miles and thousands of years in the making. A story that began with that same shooting star locked inside the icy body of the wandering comet 109P/Swift-Tuttle.

The 16-mile-wide (26 kilometer) giant of a comet spends its life journeying back and forth between the outer and inner solar system, where its frigid body is heated by the sun, triggering dramatic outbursts of activity. While in close proximity to our star, ice near to the surface of the comet is transformed into gas, skipping the water stage entirely as it escapes out into the vastness of interplanetary space.

Embedded within that ice was once a micrometeoroid no larger than a grain of sand, destined to become the Perseid shooting star you saw.

The violence of the newborn micrometeoroid's exile was followed by an epoch of utter silence, as its orbit was subtly influenced by the unseen forces of the solar system. It would be easy to think of this as a lonely existence, but we'd be wrong.

Our cosmic pebble was joined by millions of others, all shed in the wake of Swift-Tuttle. A great stream of primordial material that threads through the inner solar system, crossing the path of Earth before extending in a great swarm that messily traces the elliptical orbit of their comet progenitor, below the plane of the solar system. Beyond the orbit of Pluto.

Each follows its own unique path. Trajectories are shaped by the force of a micrometeoroid's expulsion from the comet's nucleus, along with the gentle push of radiation from the sun and the gravitational tug of the planets.

It's impossible to know how long our shooting star drifted through the cold expanse of interplanetary space. Was it hundreds or many thousands of years? How many times might it have journeyed around the sun before its fateful rendezvous with our Blue Marble?

We can never know. What we do know is how its journey ended.

Civilizations could have risen to their zenith and crumbled in the time our micrometeoroid spent traversing the unfeeling expanse of interplanetary space, but its demise lasted but a fraction of a second. It collided with our planet's gaseous shell at 132,000 miles per hour (212,433 kmph), cutting a brilliant green trail through the summer sky as atmospheric friction vaporized the cometary shard.

It's that fiery demise that you spotted tonight — an experience that will repeat hundreds of times each and every hour at the height of the Perseid meteor shower, as Earth passes through the densest part of the debris stream cast off by comet Swift-Tuttle.

The Perseid meteor shower is active from now until Aug. 24, with the best viewing window occurring in the early hours of Aug. 13, as the shower's radiant rises to its highest point on the night of the shower's peak.

This year's peak will be particularly spectacular, unfolding as it does in the pristinely dark skies surrounding the Aug. 12 new moon, which will also cause a spectacular total solar eclipse to be visible across parts of Spain, Iceland and Greenland. If you find yourself in the path of totality and have luck on your side, then you might just spot a Perseid fireball brightening the false twilight that falls as the moon hides the face of the sun at the crescendo of the eclipse!

Want to capture a shooting star that will stay with you forever? Then be sure to read our guide to photographing fast-moving meteors, along with our roundups of the best cameras and lenses for astrophotography if you're looking to upgrade your gear.

Editor's Note: Did you catch a photo of a Perseid shooting star and want to share it with Space.com's readers? Then please go ahead and send your photos along with your comments, name and location to spacephotos@space.com.

The Canon 18x50 IS binoculars are ideal for stargazing and are able to deliver clarity on night sky objects, thanks to their image stabilization. The 50mm objective lenses are the benchmark for stargazing binoculars and are able to deliver bright views of the night sky. They are currently 30% off their retail price.

You can get the Canon 18x50 IS all-weather binoculars on sale for $1195 from Amazon.

When it comes to stargazing, image-stabilized binoculars are a cut above the rest. Even at high magnifications, you get detailed views of night sky objects like star clusters and nebulas, instead of shaky worms of light. Our expert reviewer gave the Canon 18x50 IS binoculars four stars and called them 'stargazing ready' thanks to their high 18x magnification and image-stabilization.

• We've got you covered with reviews and rankings of the best telescopes, binoculars, star projectors, cameras, drones, Lego, streaming and more.

Stargazing with regular binoculars or image stabilized binoculars is the same difference as night and day. Especially at higher magnifications, image stabilization becomes a necessity when using the binoculars without a tripod and you can struggle to get a shake-free view without it.

The Canon 18x50 IS binoculars offer a powerful 18x magnification and 50mm objective lenses for great astronomy performance. You don't need to worry sacrificing low-light capability for image-stabilization. The star clusters, galaxies and nebulas are bright without becoming lines of squiggly light. They are brilliant for bird watching and general use, too, with the image stabilization adding to the quality of all views.

The optical technology stands out with ultra-low dispersion (UD) glass elements for virtually no chromatic aberration (color fringing) and doublet field flatteners for sharp stars from edge-to-edge. Optics expert, Jase Parnell-Brookes, gave them four stars in their full Canon 18x50 binoculars review for enabling a relaxing and impressive session of stargazing. They highlighted the strong grip for sturdiness in challenging conditions but even though they are advertised as all-weather, they are not fully waterproof. At 27% off asking price, this is a huge saving on a pair of binoculars we think are among the best for stargazing.

Key features: 18x magnification, 50mm objective lens diameter, 3.7-degree field of view, 15mm eye relief, 41.6 oz (1.2 kg).

Price history: The Canon 18x50 IS binoculars have a retail price of $1,648 but are often discounted from Amazon for $1,549. This deal from an Amazon seller brings the price down to $1,195, with the official Amazon listing on sale for $1,199.

Price comparison: Amazon: $1,195 | BHPhotoVideo: $1,449 | Adorama: $1,149

Reviews consensus: In our Canon 18x50 IS binoculars review, we praised their the premium features that made it perfect for stargazing: 18x magnification, 50mm objective lenses and superb image stabilization.

Space: ★★★★

✅ Buy it if: You want high powered views of the universe from handheld binoculars without the need for a tripod.

❌ Don't buy it if: If you don't need high magnification or image-stabilization, a lower magnification pair might be more suited to you, like the Nikon Action 7x50 binoculars.

Check out our other guides to the best telescopes, binoculars, cameras, star projectors, drones, lego and much more.

Aug. 12, 2026, offers a rare double-header for skywatchers across northeastern North America: a partial solar eclipse during the afternoon followed, hours later, by the peak of the Perseid meteor shower beneath dark summer skies. The eclipse is part of a total solar eclipse happening in eastern Greenland, western Iceland and northern Spain.

"The neat thing about seeing a partial eclipse, especially one that is total somewhere else, is that you get to join in with the whole event that's going on," Tyler Nordgren, astronomer and eclipse artist at Space Art Travel Bureau, told Space.com. "It is a worldwide event, and you can get a sense of the three‑dimensional nature of the universe."

Together, the two events make a perfect excuse for an overnight astronomy road trip — whether that means heading into the mountains, camping beside a lake or escaping to a remote coastline. Pack a reclining camp chair, warm layers and plenty of bug spray, but before you do anything else, book a campsite because peak Perseids night can be one of the busiest camping nights of the year.

Do take precautions with the solar eclipse. "It will not be safe to look at with the naked eye, and it will not be safe to photograph with a camera that doesn't have a solar filter on it," Nordgren explained. "If you've got eclipse glasses left over from 2024, take them out, point them at a bright light bulb, and make sure there is no light coming through any pin pricks or scratches."

Eclipse timings and sightlines are from Xavier Jubier's Interactive Google Maps; cloud cover is from Time and Date, and Bortle and sky quality meter (SQM) data come from the Light Pollution map. Bortle and SQM ratings indicate darker skies and better stargazing conditions.

REMEMBER: During a partial solar eclipse, it is never safe to look directly at the sun without proper solar viewing protection, such as certified eclipse glasses or approved solar filters. Read our guide on how to observe the sun safely.

1. Gros Morne National Park, Newfoundland

Gros Morne National Park combines relatively dark skies with the deepest eclipse in eastern North America, with nearly half of the sun obscured at maximum. Coastal viewpoints, lakeshores and elevated trails offer wide southwest-facing horizons for the afternoon eclipse, while the park's low levels of artificial light make it well suited for Perseid viewing after midnight. The main drawback is Newfoundland's often variable weather and relatively high average cloud cover.

2. Mount Carleton Dark-Sky Preserve, New Brunswick

Mount Carleton Provincial Park has some of the darkest skies in Atlantic Canada, with Bortle 2 conditions across much of the preserve. Open areas around Mount Carleton and nearby lakes provide unobstructed southwest views for the eclipse, while the remote setting is perfect for Perseid observing later that night. Campgrounds inside the park make it practical for an overnight trip.

3. Fundy Dark-Sky Preserve, New Brunswick

Fundy National Park offers reasonably dark skies and accessible observing locations along the Bay of Fundy coast. Open areas around Wolfe Lake and Chignecto Campground provide good visibility toward the southwest during the eclipse, while the surrounding dark-sky corridor supports decent Perseid observing conditions after dark. Coastal "Fundy fog" and changing maritime weather can occasionally affect visibility.

4. Kejimkujik National Park, Nova Scotia

Kejimkujik National Park remains one of the darkest accessible observing sites in Atlantic Canada, with low light pollution and broad lake horizons that are well-suited to meteor observing. The partial eclipse here approaches 30%, and the park's lakeside campgrounds provide convenient overnight access for Perseid watching later that evening. Compared with many coastal locations in the region, Kejimkujik also has somewhat lower average cloud cover.

5. Acadia National Park, Maine

Acadia National Park combines relatively accessible dark skies with open coastal horizons facing the eclipse. Elevated viewpoints around Cadillac Mountain and the Schoodic Peninsula offer clear sightlines toward the southwestern sky, while overnight observers can expect reasonably dark conditions for Perseid viewing by northeastern U.S. standards. Summer crowds and vehicle access restrictions around Cadillac Summit mean you should make a plan well in advance.

6. Mont Mégantic Dark Sky Reserve, Quebec

Mont-Mégantic is one of the best-established astronomy sites in eastern North America, with protected dark skies and extensive observing infrastructure around the observatory and national park. Although the eclipse magnitude is moderate, the reserve's dark nighttime conditions and elevated observing areas make it a strong location for Perseid observing after dark. Cloud statistics are less favorable than farther south in New England.

7. Adirondack Mountains, New York

The Adirondacks offer some of the darkest skies in the northeastern U.S., particularly around remote lakes and higher-elevation observing sites. While the partial eclipse will be modest, the region's low artificial light levels and broad rural horizons make it a strong overnight option for the Perseids. Public campgrounds and astronomy events at local observatories may fill quickly around peak Perseid night. Check the Adirondack Sky Center & Observatory for events.

8. Catskill Mountains, New York

The Catskills provide relatively accessible dark skies within a few hours of major northeastern cities, making them a practical option for short-notice observing trips. The partial eclipse will be small, but reservoirs, ridgelines and open viewpoints offer decent southwest sightlines during the afternoon event. Overnight conditions are darker than much of the surrounding northeast region, particularly away from populated valleys.

9. Cherry Springs Dark Sky Park, Pennsylvania

Cherry Springs State Park is one of the best-known observing locations in the eastern US, with very dark skies and unusually open horizons in all directions. Although the eclipse itself will be very shallow, the park is among the best suited for the Perseids later that night, when low light pollution and established observing fields provide excellent meteor-viewing conditions. Expect heavy attendance around the shower peak.

10. Assateague Island National Seashore, Maryland

Assateague Island offers unobstructed coastal horizons and relatively low light pollution for the mid-Atlantic region. The partial eclipse here will be a technical affair, but the island's open beaches provide excellent naked-eye conditions for Perseid observing after dark, especially looking away from nearby coastal development. However, humidity, sea haze and mosquitoes can be significant factors during August observing sessions.

The Perseids may be the summer meteor shower everyone marks on the calendar, but they are not the only reason to look up this season.

From mid-July through late August, Earth plows through several other streams of comet and asteroid debris, triggering a series of lesser-known meteor showers across Northern Hemisphere skies.

Most will not deliver the dazzling hourly rates of the Perseids, and moonlight will spoil some peak nights in 2026. But for patient skywatchers under dark skies, these lesser-known showers can still serve up bright fireballs, faint streaks and a preview of the main event to come.

The duration in days of a shower we provide here is somewhat arbitrary, since the beginning and ending are gradual and indefinite. While the hourly rates from these other meteor streams provide but a fraction of the numbers produced by the Perseids, combined, overall, they provide a wide variety of meteors of differing colors, speeds and trajectories.

Capricornids

First to appear are the Capricornids, starting around July 10, with their maximum on July 25 and end on Aug. 15. Under the best conditions only a few bright meteors per hour come from this stream, so you'll hardly know it is in progress unless you plot meteor trails on a star map and trace them back to their common intersection point; most of the meteors you'll see will be sporadics or members of another shower.

The radiant reaches its highest point at about 30 degrees high in the south, about 2:00 a.m. local daylight time. The waxing gibbous moon will have set at around 1:40 a.m. on the night of the peak, leaving the rest of the night dark for prospective meteor watchers.

Delta Aquarids

Next come the Delta Aquarids, July's most prolific shower, with maximum on July 29, and as many as two or three dozen meteors per hour under ideal conditions. The shower lasts from July 12 to Aug. 23. It has a double radiant, indicating that we are seeing two distinct streams of celestial debris burning up in the Earth's atmosphere.

The meteors are mostly faint; a few bright, 5-10% leave persistent trains; they move at medium-slow speeds because they are coming in sideways across Earth's orbit. On peak night this year, the double radiant will be highest — roughly 40 degrees above the southern horizon — at 3:30 a.m. Unfortunately, in 2026, peak activity will coincide with full moon, so most of these streaks will likely be squelched by bright moonlight.

Piscis Australids

Another weak shower is the Piscis Australids, on July 30, with normal limits July 10 to Aug. 10. This is a lesser stream; only about eight members per hour are seen under best conditions to observers in the Southern Hemisphere, where the radiant — near the bright star Fomalhaut — climbs high in the sky.

As is the case with the Delta Aquarids, the moon, only one day past full, unfortunately, wrecks any chances of getting any decent views this year.

Alpha Capricornids

The final shower peaking in July is the Alpha Capricornids, which begin about July 7, peak on July 31, and end on Aug. 15. The radiant reaches its highest point, about 30 degrees high in the south at about 1:00 a.m. local daylight time. Though sparse (5 per hour) in number, the Alpha Capricornids are photogenic, frequently producing bright yellow fireballs that can be quite spectacular. Sadly, the bright moon, 93% illuminated, is in eastern Capricornus and will seriously impact the peak of this year's display.

Iota Aquarids

The last minor shower before the Perseids is the Iota Aquarids, a two-radiant shower having detectable members from July 15 to Aug. 25. At peak activity on Aug. 6, only about six members per hour are seen under good conditions; the radiants are at their highest point, about 40 degrees in the south at 2:30 a.m. A last quarter moon will be about one-third up in the eastern sky at that hour, which will interfere to an extent with viewing these meteors.

Perseids

The Perseids are predicted to reach their peak in 2026 on the morning of Aug. 13. Meteors whose paths extended backward intersect at a spot near the Perseid-Cassiopeia border not far from the famous Double Cluster in Perseus.

It rises at dusk and is highest in the sky — nearly overhead — at 5:40 a.m. When maximum occurs in a dark sky, as will be the case this year, this rich stream offers a crescendo in hourly rates averaging more than 50 members per hour, though double this rate has been seen on occasion. Many flaring meteors with trains are seen. This shower normally extends from July 17 through Aug. 24.

Kappa Cygnids

The last summer shower is the Kappa Cygnids. The limits of this shower run from Aug. 3 to Aug. 25, with the peak on Aug. 17. Though the maximum rate is only about four per hour, the stream does provide slow-moving flaring fireballs, and a careful observer may be nicely rewarded for the time spent.

The radiant is just north of the star Kappa Cygni and is nearly overhead — some 80 degrees high — at around 10:00 p.m. local time. At about that same time, a waxing crescent moon is low in the southwest and is about to set and will offer little viewing interference.

Where to look

The radiant is the place in the sky where the paths of shower members, if extended backward, would intersect when plotted on a star chart. Many people are misled into thinking that this is the best place to look for these meteors, but only stationary meteors — ones coming nearly straight at you — can be seen here.

The greatest numbers will be seen perhaps 30 degrees away from the radiant, in the general direction of the zenith. Remember that your clenched fist held at arm's length is roughly equal to 10 degrees.

In addition to shower meteors, there are always sporadic ones, apparently unrelated to one another, that occur at an average rate of about 7 per hour. The duration in days of a particular shower is somewhat arbitrary, since the beginning and ending are gradual and indefinite.

Skywatching tips

The only equipment you'll need is your eyes and a modest amount of patience.

The number of meteors an observer can see in an hour depends strongly on sky conditions. The rates quoted here are based on a limiting star magnitude of +6.5 (an exceptionally good, dark sky), an experienced observer, and the assumption that the radiant is directly overhead.

The lower the radiant in the sky, the fewer the numbers that will be seen. At an altitude of about 30 degrees, the hourly rate is halved, at 15 degrees it is one-third. No two observers prepare for a meteor vigil the same way.

Expect the overnight low temperature to be well below what the weather forecast suggests. When you sit quite still, close to the rapidly cooling ground, and if the air is even just slightly damp, you can become very chilled. It helps to take a late afternoon nap, followed by a shower, and to wear fresh clothing. Heavy blankets, sleeping bags, a ground cloth, an auto cushion, and a pillow are all necessary equipment. Some food and non-alcoholic beverages will help keep you comfortable.

Don't forget the moon

Another factor is the phase of the moon, which this year will be full on July 29 and new on Aug. 12. This makes it a very favorable year for viewing the Perseids, but not so favorable for those displays peaking at the end of July into early August. However, most are also active for a good number of days before and after maximum activity, so you can also watch for them when moonlight is not a hindrance.

Are these meteor showers worth watching?

In short, minor summer meteor showers are worth watching if you enjoy patient, low-key skywatching, but they are not ideal if you expect a dramatic display.

They offer a long observing season, require no equipment, and can produce a variety of meteors with different colors, speeds, paths, and occasionally bright fireballs. They also give observers more chances to watch when skies are clear and moonlight is less intrusive.

However, most are weak when compared to the Perseids, with low hourly rates and many faint meteors. Moonlight, low radiant positions, overlapping showers, and sporadic meteors can make them harder to see and identify, so observers need dark skies and patience.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

People keep asking me about the total solar eclipse on August 12. That's understandable. For anyone in the Northern Hemisphere, it is shaping up to be a joyous day of astronomy. Totality will cross eastern Greenland, western Iceland and northern Spain, but much of Europe will see a very deep partial eclipse, and even parts of North America will see a small bite taken from the sun. Then, just hours later, the Perseid meteor shower will peak beneath perfectly moonless skies. What a double-act!

The problem with promoting days and nights like that is that they make us think skywatching is only worth doing at very specific times. Everything becomes about moments, peaks and countdowns. That rings true for an eclipse, of course, but for the Perseids, it's less so.

The Perseid meteor shower actually begins right now. It's active from July 17 through August 24. Yes, it reaches a strong maximum overnight on August 12-13, where observers under ideal dark skies could see 50 or more "shooting stars" per hour. That's absolutely the night to aim for if you only go stargazing once a month. But for stargazers with a little more time, the hunt can begin right now.

The best Perseid is the first one you see. In these weeks before the peak, there's less expectation, less focus on the weather. An unexpected streak while you are outside feels accidental.

For me, it often happens when I've stopped observing properly for the night. Last summer, I was moving my telescope indoors late at night after a fairly unremarkable session looking at a few globular clusters. As I went back inside, I did my usual pause and look at the stars one last time. As I did, my peripheral vision caught a bright meteor whizzing across rooftops in the northeast. Summer's meteor season had begun with a bang when I least expected it to.

The Perseids officially build gradually over several weeks as Earth slowly enters the broad debris stream left behind by Comet Swift-Tuttle. It was last in the inner solar system in 1992 and will return in 2126. The peak around August 12—13 marks the densest part of the stream, but in mid-July, only a handful of meteors will appear each hour. That's exactly why early Perseids feel so special — you stumble across a meteor when you least expect it. Its gradual beginning also explains why some of the earliest Perseids can be surprisingly dramatic. The shower is famous for bright fireballs — large, vivid meteors that sometimes leave glowing trails lingering for several seconds. Even when overall meteor rates remain low in July, a single bright Perseid can add some magic to a night's observing.

What's happening and when to look

If you want to begin watching for Perseids this week, the best time is after midnight through the small hours before dawn, when the radiant constellation, Perseus, climbs higher in the northeastern sky. "Shooting stars" can appear anywhere in the night sky, but if their paths backward point roughly toward Perseus, it's a Perseid. That's what gives the shower its name.

There's more to look at than Perseids because July is quietly crowded with other meteor showers. The Southern Delta Aquariids begin strengthening through the second half of the month. From southern latitudes, they can produce roughly 25 meteors per hour under dark skies, though observers farther north tend to see fewer because the radiant stays low in the southern sky. These meteors are usually softer and subtler than Perseids — medium-speed streaks without many dramatic fireballs or glowing trails.

Running alongside them are the Alpha Capricornids, active from early July into mid-August. Technically, this is a weak shower, often producing only a handful of meteors per hour, but it compensates with unusually bright, slow-moving fireballs.

Unfortunately, both showers peak this year beneath an almost full Buck Moon on July 30-31, which will wash out many fainter meteors. But bright meteors and fireballs should still occasionally punch through the moonlight.

How and when I'm watching it

I will probably begin meteor season the same way I always do: accidentally. I'll increase the odds by lingering outdoors slightly longer than necessary on warm nights, staying up later than I should and using my smart telescope to collect data on deep-sky objects while I search the skies for the first Perseid. It's best done now, before the moon waxes to full, and certainly before early August, when it wanes — the worst moon phase for observing meteors because it's in the sky just as meteor activity peaks.

Stargazer's corner: July 17-24, 2026

With a new moon on July 14, this weekend is perfect for watching the return of a waxing crescent moon to the night sky. Look low in the west during dusk on Friday, July 17, to see a 16%-illuminated waxing crescent moon to the left of Venus. Watch it climb higher into the evening sky night after night, leaving genuinely dark late-night skies once it sets. It's good timing for the first serious Perseid-watching session of the season, particularly after midnight when meteor activity naturally increases as Earth rotates into the direction of travel around the sun.

Meanwhile, the Summer Triangle — formed by Vega, Deneb and Altair — hangs almost overhead during the darkest hours, making this one of the easiest seasonal star patterns for beginners to learn. Saturn now rises comfortably before midnight and dominates the southeastern sky by dawn, when it's joined by Mars and the stunning Pleiades open cluster.

Constellation of the week: Perseus

Perseus, "The Hero," never quite looks how beginners expect. Rising into the northeastern night sky around midnight this week between bright star Capella and Saturn in the east, its name suggests something dramatic, but the constellation itself appears more like a loose chain of stars stretching below Cassiopeia in the northeastern sky. At this time of year, Perseus rises late, which is why the best Perseid activity happens after midnight once the radiant climbs higher. Beginners often assume meteors appear only near the radiant itself, but the longest and most impressive Perseids usually streak much farther away across the sky. Perseus matters less as a viewing target than as a reminder that meteor showers are fundamentally about perspective. The meteors are not actually emerging from the constellation at all — Earth is simply driving through comet debris head-on.

Look up! The Perseid meteor shower is finally active, bringing the potential for gorgeous shooting stars and fireballs as Earth plunges into the trail of debris shed by the icy comet Swift-Tuttle. Here's what you need to know.

The Perseid meteor shower 2026 is set to be a truly magnificent affair and a stark contrast to last year, when moonlight drowned out all but the brightest shooting stars. The shower will reach peak activity overnight on Aug. 12-13 under the dark skies of the new moon. During the peak, up to 100 shooting stars may be seen each hour as they cut fiery paths through the summer sky, according to the American Meteor Society.

You could even spot a Perseid brightening the false twilight triggered at the climax of the Aug. 12. eclipse, as the moon perfectly hides the surface of our parent star. But for that to happen you'd have to find yourself in the path of totality just as a large fireball-producing meteoroid struck Earth's atmosphere. It's certainly possible, but let's just say that the odds aren't stacked in your favor.

If you're not in the path of totality then there's no need to despair, you stand a much better chance of spotting Perseids the old fashioned way anyway!

How to spot Perseid shooting stars

Perseid meteors can be spotted anytime after dark from tonight onwards, streaking away from a patch of sky, or radiant, located close to the red supergiant star Eta Persei in the constellation Perseus.

To find the best meteors, you'll first want to locate Perseus glistening above the northwestern horizon after dark. Next, find a patch of sky 40 degrees above it, and settle in for one of the year's premier natural light shows. This is where the shooting star trails will be at their longest.

The Perseids are also famed for producing vivid green fireballs capable of briefly turning night to day as larger chunks of debris collide with Earth's atmosphere at speeds of up to 37 miles per second (59 kilometers per second).

When to look for Perseid meteors

Perseid meteors may be spotted anytime from 10 p.m. onward for viewers in the U.S., though the number of visible shooting stars will be higher in the hours before dawn, when the radiant rises to its highest point in the summer night sky. Try to head away from city lights and allow at least 20 minutes for your eyes to adapt to the darkness.

Relatively few shooting stars will be visible in the days following the shower's awakening compared to the peak. However, if you do catch one, you'll have seen the demise of a meteoroid that's likely been flying through space for thousands of years before reaching Earth.

"The meteors we see early and late during the activity are most likely the oldest as they have obviously been perturbed from the main orbit of the comet, which we encounter in mid-August," said Robsert Lunsford of the American Meteor Society in an email to Space.com.

The greatest number of meteors can be seen in the predawn hours of Aug. 13 as the shower reaches peak activity, when Earth passes through the densest section of the debris stream left behind by comet Swift-Tuttle.

Want to capture your own photos of the Perseid meteor shower? Then be sure to read our guide detailing how to image shooting stars, along with our roundups of the best cameras and lenses for astrophotography.

Editor's Note: Did you capture a photo of a Perseid and want to share it with Space.com's readers? Then please send your photos and comments, along with your name and location to spacephotos@space.com.

On Aug. 12, I get to fulfil a lifelong ambition. I'll take a flight to Madrid and travel northwest to the city of Valladolid by rail, before striking out for Valoria la Buena — a charming town in central Spain with a population of less than 1,000.

There, I'll bear witness to one of the most spectacular naked eye shows that the solar system has to offer: a total solar eclipse. My first total solar eclipse.

Don't get me wrong. I've been obsessed with eclipses my entire life. I just haven't found myself in the right place at the right time to experience totality until now. 10-year-old me came pretty close during a deep partial eclipse in 1999, when I caught a fleeting glimpse of the moon's silhouette taking a bite out of the sun in the cloud-ridden skies over the United Kingdom.

Smash cut 20-something years later and I'm inexplicably the Skywatching Writer for Space.com, where one of the major perks of the job is being sent to report on eclipses. Things aligned quite nicely.

For the 2026 eclipse, I'll be joining a volunteer team from NASA's Dynamic Eclipse Broadcast (DEB) Initiative led by citizen scientist Charles Greenwald.

The DEB is a network of enthusiastic solar observers led by professional astronomers who use standardized telescopes and software to share inspiring eclipse imagery to the public, while also capturing valuable scientific data on the sun's disk and golden atmosphere.

It was Greenwald who scouted Valoria la Buena as a prime location to observe the eclipse. He's since been hard at work liaising with DEB initiative leadership to test software updates and troubleshoot other issues, while also travelling to Mexico to help train student members of the team ahead of their expedition to Spain. Two more eclipse enthusiasts are due to join the group once it arrives in Madrid, making it a wonderfully international affair.

Less than a month out, things are pretty settled, and a kind of nervous anticipation has taken hold. Flights and trains are booked, and I have a pair of Celestron EclipSmart 10x42 binoculars and the EclipSmart 3-Piece Solar Eclipse Observing and Imaging Kit, courtesy of Celestron. Also hats and an ungodly amount of suntan lotion. I'm bald after all, so the sun is my greatest natural predator.

Of course, preparations can only get you so far. Once we get to Valoria la Buena on Aug. 10 there'll still be important work to do. The first order of business for Charles and his DEB team will be to stake out a location with a clear line of sight to the west for their equipment. Totality will occur with the sun less than 10 degrees above the horizon — roughly the width of your clenched fist held at arm's length — so line of sight will be everything.

We'll also be at the mercy of the weather. Clouds could easily arrive to hide the cosmic show from view — especially with the eclipse so low on the horizon. The DEB team also has to find a spot with good connectivity, which will allow them to broadcast near-live images of our parent star for the public to enjoy and scientists to pore over.

All being well, myself, the DEB team and over 15 million others in the path of totality will bear witness to a heartstopping display of orbital mechanics that crescendos with the fleeting artificial night of totality, as the moon blocks the last sliver of the sun from view. Space.com's Skywatching Editor Daisy Dobrijevic will also be on hand to report on the total solar eclipse as it unfolds in the skies over Greenland.

We can't wait to share our experiences with you. Be sure to stick with Space.com to discover everything there is to know about the Aug. 12 total solar eclipse, along with details on how to watch it online, which will be published closer to the event!

You should also read our guide to safely observing the sun, to ensure that you're ready to enjoy the eclipse, and our roundup of the best solar viewing equipment available in 2026 if you're looking for safe, quality gear.

Editor's Note: Want to share your eclipse photography with Space.com's readers? Then please send your photos and comments, along with your name and location to spacephotos@space.com.

On Aug. 12, 2026, skywatchers across the U.K. will experience a rare astronomical double-header: a deep partial solar eclipse before sunset followed, hours later, by the peak of the annual Perseid meteor shower. Although the path of totality will sweep from Greenland and Iceland to Spain, it will miss Britain entirely. However, the solar eclipse will still be dramatic, with up to 96% of the sun obscured for viewers in the far southwest.

This will be the U.K.'s deepest partial solar eclipse since 2015, and timing will be everything. The eclipse reaches its peak around 7:00-7:16 p.m. BST, with the sun hanging low above the west-northwest horizon as a narrowing crescent shortly before sunset. Because the sun will be relatively low, choosing the right location will matter far more than traveling huge distances. Coastal viewpoints, hilltops and open landscapes with unobstructed western horizons will offer guaranteed views — if the sky is clear.

The locations below prioritize another crucial factor: dark skies. While the eclipse will be visible almost everywhere in the U.K. and most will be happy to see it from close to where they live, the real reward comes after darkness falls, when the Perseids begin flashing across the sky. Find somewhere remote, stay overnight — ideally camp — and this could become one of the most memorable observing sessions of the year.

Eclipse timings and sightlines are from Xavier Jubier's Interactive Google Maps; cloud cover is from Time and Date, the figures reflect long-term climatological averages for mid-August, not weather forecasts. Bortle and sky quality meter (SQM) data come from the Light Pollution map.

During a partial solar eclipse, it is NEVER safe to look directly at the sun without solar eclipse glasses designed for solar viewing. Read our guide on how to observe the sun safely.

1. Hugh Town

The Isles of Scilly combine Britain's deepest partial eclipse with some of southern England's darkest skies. From Hugh Town and nearby west-facing beaches on St Mary's, the eclipsed sun will hang low above the Atlantic Ocean late in the day. Later that night, with minimal light pollution and broad sea horizons, the islands are an exceptional place to watch the Perseid meteor shower beneath pristine late-summer skies.

2. Land's End

Land's End is one of the best places on mainland Britain to watch the eclipse because of its vast Atlantic horizon and minimal obstruction toward the west-northwest. The sun will appear heavily eclipsed as it descends toward the ocean before sunset. After dark, the remote far-western location and low levels of artificial light make this region an outstanding destination for viewing the Perseid meteor shower.

3. Boscastle

Boscastle's narrow harbor and dramatic valley may create a natural frame for the eclipsed sun as it sinks toward the Atlantic. The village's northwest-facing coastline offers clear views toward the low evening eclipse, while the surrounding Cornish countryside remains relatively dark after sunset. Once twilight fades, the cliffs and headlands nearby become excellent places to watch for bright Perseid meteors.

4. Exmoor Dark Sky Reserve

Exmoor combines elevated moorland, dramatic coastline and protected dark skies, making it ideal for both the eclipse and the Perseids. Coastal viewpoints such as Valley of Rocks and Heddon's Mouth offer clear west-facing horizons for the low-eclipsed sun before sunset. Later that night, Exmoor's status as a Dark Sky Reserve makes it perfect for seeing bright Perseid meteors — and the Milky Way.

5. Rhossili Bay

Rhossili Bay's enormous west-facing beach and elevated clifftops make it ideal for watching a low eclipse unfold above the sea. Located on the Gower Peninsula, the area is a Dark Sky Community that retains relatively dark skies despite its popularity during the day. As darkness falls later that evening, the open coastal landscape provides excellent visibility for Perseid meteors.

6. Strumble Head

Strumble Head offers one of the clearest west-facing horizons in Wales, with the eclipsed sun appearing above the Irish Sea beside its iconic lighthouse. The remote Pembrokeshire coastline experiences very little artificial light, helping preserve dark skies after sunset. Once the eclipse ends, this rugged headland becomes an excellent place to watch the Perseids, with broad ocean views and little interference from nearby towns.

7. Llŷn Peninsula

The remote Llŷn Peninsula projects deep into the Irish Sea, offering expansive views toward the west-northwest horizon, where the eclipsed sun will appear before sunset. It is also one of the darkest regions in Wales, lying close to the protected skies of Ynys Enlli (Bardsey Island) Dark Sky Sanctuary. With minimal light pollution and wide rural vistas, the peninsula becomes a superb location for watching Perseid meteors later that same night.

8. Galloway Forest Dark Sky Park

Galloway Forest Park was Britain's first Dark Sky Park and remains one of the country's premier stargazing destinations. Open western views around Clatteringshaws Loch, along with other viewpoints away from the forests, make it well-suited to the low evening eclipse. After twilight fades, exceptionally dark skies reveal the Milky Way in striking detail, creating near-perfect conditions for viewing the Perseid meteor shower in the early hours — if the sky is clear.

9. Northumberland Dark Sky Park

Northumberland's Dark Sky Park combines remote landscapes with some of England's darkest skies. Locations around Kielder Water and Northumberland National Park provide broad views toward the low west-northwest eclipse shortly before sunset. Later that night, the region becomes one of the finest places in Europe to watch the Perseids, with frequent views of the Milky Way and bright meteors overhead. Check for any events at Kielder Observatory.

10. Giant's Causeway

The Giant's Causeway in Northern Ireland offers a spectacular foreground for the eclipse, with the sun appearing low above the Atlantic beyond the famous basalt columns. Although the skies here are not as dark as in some rural parks, the north Antrim coastline still experiences relatively modest light pollution. Nearby coastal viewpoints and beaches provide good conditions for watching Perseid meteors later that night beneath expansive northern skies.

Sometimes weeks go by without anything notable happening in the sky. Then along comes something spectacular, like a total solar eclipse, the peak of a major meteor shower or a bright planet reaching a landmark moment in the evening sky. On Wednesday, Aug. 12, 2026, all three occur almost simultaneously. As a bonus, if you are under a dark sky for the Perseids, the Milky Way's bright central regions will stretch across the southern sky by around midnight.

Exactly what you'll see of the eclipse depends on where you are on Earth. From within a narrow 180-mile-wide path of totality across eastern Greenland, western Iceland and northern Spain, a total solar eclipse will briefly turn day into night for lucky locals and intrepid eclipse chasers. Across the U.K., millions will see a partial eclipse of the sun, ranging from 90% to 95%. Across Europe and northwest Africa, an equally deeply eclipsed sun will peak at sunset, creating a truly strange sight. Minutes later, brilliant Venus reaches dichotomy — appearing exactly half-lit in telescopes, while to the naked eye it blazes at magnitude -4.4 in the western twilight. A few hours later, the annual Perseid meteor shower reaches its peak.

Wherever you are, there will be something worth looking at. Here's exactly what will happen, where and when, depending on where you are (times are from Time and Date).

Iceland or Greenland: a total solar eclipse … and aurora?

If you've traveled to (or live in) western Iceland, or you're booked on an expedition cruise ship on Aug. 12, you're in for a treat. The point of maximum eclipse — 2 minutes 18 seconds — is off the coast of Iceland, accessible by ship, but likely not by many. It's possible that expedition ships in the lower reaches of Scoresby Sund, Greenland, will experience the most totality, with 2 minutes 17 seconds possible at 4:36 p.m. WGST, with the eclipse 25 degrees above the west-southwest. Here, the sun will set at 10:15 p.m., with the darkest time about 12:50 a.m. — there is no truly dark night, just all-night civil twilight. That makes the Perseids and aurora unlikely to be seen even if they're present. Ditto Venus — Greenland is too far north.

In Iceland, totality will begin between 5:43 and 5:50 p.m. GMT, depending on the exact location. It will last longest in regions farthest west, with 2 minutes 13 seconds at Látrabjarg in the remote Westfjords (5:44 p.m.) and 2 minutes 10 seconds at the westernmost coast of Snæfellsnes Peninsula (5:45 p.m.). The eclipse will be 25.5 degrees above the west-southwest. The sun will set at 9:53 p.m. in Reykjavík, with the darkest window from 11:00 p.m. to 4:00 a.m. (and the darkest time 1:30 a.m.). That makes Perseids and aurora possible — though summer twilight often limits visibility. However, Venus will not be visible after sunset.

Spain: Totality, Venus and the Perseids

For anyone within Spain's path of totality, Aug. 12 promises to be one of the greatest days of skywatching imaginable. The main event comes late in the day as the moon completely covers the sun. In parts of northern and eastern Spain, totality will occur with the sun hanging low above the western horizon, creating one of the most photogenic eclipse scenarios of the century.

In Spain, totality will begin between 8:26 and 8:33 p.m. CEST, depending on the exact location. Its maximum duration in Spain will last longest in regions farthest northwest, with 1 minute 50 seconds at Playa de la Escaladina in Galicia (8:26 p.m.), where the eclipse will be 11 degrees above the west-northwest. It will be at its shortest, at 1 minute 36 seconds, at Bellavista, Mallorca, one of the Balearic Islands (8:31 p.m.). The eclipse will be just a couple of degrees above the west-northwest. The sun will set at 9:16 p.m. in Madrid, with a dark night from around midnight through 4:40 a.m. CEST. The darkest part of the night — and the point when the radiant point Perseus will be high above the horizon — will be around 02:00 a.m. CEST.

Unless there's a whopping solar storm (unlikely), concentrate on the Perseid meteor shower, rather than hoping for aurora. Light pollution is irrelevant for a total solar eclipse, but if you've cross-referenced your eclipse-viewing sight with a Light Pollution Map, you'll be in Bortle 4 skies in rural Spain, ready for a potentially unforgettable Perseids (the solar eclipse means by definition that it's taking place at new moon, after all). Under rural Spanish skies, particularly in dark-sky regions away from towns and cities, observers could see 30 to 50 meteors per hour, with occasional bursts producing even more.

It might be wise to have an afternoon nap before the eclipse — it could be a long, exciting night if skies are clear.

U.K: Deep eclipse, Venus and the Perseids

The path of totality misses Britain entirely, but Aug. 12 will still be a remarkable day. Across most of the U.K., more than 90% of the sun will be covered by the moon, with maximum eclipse shortly after 7 p.m. BST. The sun will hang low above the west-northwest horizon as a narrowing crescent, so the best locations will be coastal viewpoints, hilltops and open landscapes with clear western horizons. London, Manchester and Glasgow all experience about 91% coverage, while Cardiff reaches 93%. The deepest eclipse will be seen in the far southwest, with 96% coverage in the Isles of Scilly and almost 96% at Land's End in Cornwall.

Although it will not become as dark as during totality, observers may notice a subtle drop in temperature and a strange dimming of the landscape. Shadows will soften, colors will become muted, and daylight will take on an unusual quality that many first-time eclipse watchers find surprising.

Once the eclipse ends, Venus becomes the next target. Look west after sunset for the dazzling Evening Star. Venus is only days from its greatest elongation and near its best evening appearance of 2026, making it hard to miss. Even a small telescope will reveal its half-lit phase. The Perseids will then peak during the early hours of Aug. 13.

Western Europe: Eclipsed sunset, Venus and the Perseids

For millions of people across Western Europe, Aug. 12 offers a slightly different spectacle. Instead of totality or a partial eclipse in late afternoon, many locations will witness a deeply eclipsed sun setting below the horizon. An eclipsed sunset is surprisingly rare, and particularly one this deep. In some places, more than 90% of the sun will be obscured as it approaches the horizon, creating a dramatic crescent-shaped sunset. In places such as Corsica, the Ligurian coast, Venice, the Alps and parts of central Europe, photographers will have the chance to capture one of the most dramatic sunset eclipses visible anywhere this decade.

With Venus visible across Europe after sunset, as well as the Milky Way and the Perseids peak, Aug. 12 will effectively become an all-night astronomy festival across Europe.

North America: Partial eclipse, Venus and the Perseids

The total solar eclipse — and a deep partial eclipse — may belong to Europe, but North America gets its own small version of the event. A partial solar eclipse will be visible from Alaska to New England, touching 26 U.S. states and every Canadian province. While the eclipse is modest compared with North America's recent total eclipses, millions of people will still be able to participate in the global event.

The deepest U.S. eclipse occurs in Alaska, where Fairbanks will see about 37% of the sun covered and Anchorage almost 28% (8:21 a.m. AKDT). In the Northeast, Maine gets the best view, with about 28% obscuration (1:50 p.m. EDT), while Boston sees 16% (1:55 p.m. EDT) and New York City about 10% (1:54 p.m. EDT). In Canada, the eclipse becomes considerably more impressive. Iqaluit, Nunavut, will see 61% of the sun covered (1:24 p.m. EDT), while St. John's, Newfoundland, will experience more than half of the sun obscured (3:35 p.m. NDT). Every Canadian province will see at least some part of the eclipse. Remember that eclipse glasses are still essential, even for small partial eclipses.

If you're looking for a telescope or binoculars to make the most of these incredible skywatching events, our guides for the best binocular deals and the best telescope deals are here to help. Interested in capturing the night sky? Check out our best cameras for astrophotography and best lenses for astrophotography.

One month from today, millions will turn their eyes to the skies for one of the most anticipated skywatching events of the year: the total solar eclipse on Aug. 12, 2026.

The eclipse will sweep across parts of Greenland, Iceland and Spain, briefly turning day into night for those lucky enough to be within the narrow path of totality.

It's been a long time coming for European skywatchers, as the event marks Europe's first total solar eclipse since 1999.

Where can I see the total solar eclipse?

If you're hoping to experience totality, now is the time to finalize your plans. The path of totality crosses Greenland, Iceland and northern Spain, with maximum eclipse lasting up to 2 minutes and 18 seconds.

Spain is expected to be one of the most popular destinations thanks to its favorable weather prospects, though it's not without a catch! Viewers will need to secure a clear view of the western horizon because the eclipsed sun will sit very low in the sky during totality.

Will I see the eclipse from where I live?

Not inside the path of totality? Don't worry. A spectacular partial solar eclipse will be visible across much of Europe, with more than 90% of the sun covered from locations including London, Paris and Dublin.

If you're still deciding where to watch, we have several guides on the best viewing locations close to popular Spanish holiday destinations, the best Spanish beaches, and the best places to view the eclipse overall.

How we will be covering the eclipse

Over the coming weeks, Space.com will bring you everything you need to prepare for eclipse day. We'll publish viewing guides, safety advice and information on how to watch the eclipse online.

Closer to the event, we'll launch a dedicated live blog covering the latest eclipse news and insights from our reporters in the field.

Skywatching Editor Daisy Dobrijevic will join an eclipse expedition to Greenland with HX, while Skywatching Writer Anthony Wood will travel to northern Spain with the DEB initiative and citizen scientists to report firsthand from the path of totality.

Should stargazers also be cloudspotters? Everyone knows clouds are the first thing you see as soon as you get under a dark sky or buy a new telescope — it's almost guaranteed! However, by early July, I usually start actively looking for a special kind of noctilucent or "night shining" cloud — and they can be a magnificent sight to rival anything celestial.

At its core, the search for these so-called "space clouds" is the flip side of the seemingly never-ending twilight in July in mid-northern latitudes of the Northern Hemisphere. You wait all winter for tolerable temperatures, then summer arrives and the night sky never properly commits to darkness. At my latitude, the northern horizon glows all evening in early-to-mid July like somebody forgot to turn the sun off completely. Serious stargazing gets harder as even bright constellations seem washed out by lingering light.

Cue noctilucent clouds. Peer at the northern sky during twilight between late May and August, and you may see strange silver-blue ripples. Delicate yet bright, they can look artificial — thin electric-blue strands stretched across twilight, with a texture like smoke. They seem entirely detached from the normal atmosphere.

Noctilucent clouds are an accident. They are caused by sunlight striking ice crystals roughly 50 miles above Earth, near the edge of space, where ice crystals can only form under extremely cold conditions. They exist so high in the mesosphere — a layer of Earth's atmosphere above the stratosphere and below the thermosphere — that they continue to glow long after sunset, because the sun is still shining on them even though it has set as seen from beneath.

Water vapor should not exist in the mesosphere, a dry layer on the edge of space. Yet under the right conditions, trace amounts of water vapor can freeze onto tiny particles, creating the ice crystals that make noctilucent clouds possible.

While greenhouse gases warm the Earth's surface, they cool the mesosphere, allowing the increased moisture to freeze. There is growing evidence that changing upper-atmosphere conditions and increasing atmospheric moisture may be affecting how often noctilucent clouds appear and how far south they are seen.

Perversely, noctilucent clouds arrive exactly during the brightest weeks of the year, when many stargazers are complaining that there is nothing worth observing. Cloudspotting on summer nights was probably not on your stargazing wishlist when you started, but for some of us, the chance of noctilucent clouds is all we have for a few weeks. See them once, and they'll fast become a seasonal delight you'll wait all year for.

What's happening and when to look

If you want to search for noctilucent clouds this week, look north about an hour to two hours after sunset, or before sunrise, during deep twilight when the sky is dark except in the extreme north. July is prime season across northern latitudes, including much of the U.K., northern Europe, Canada and the northern U.S. You do not need total darkness.

The key is a clear northern horizon. Noctilucent clouds usually appear low in the sky as pale blue, silver or sometimes faintly gold ripples and filaments. Beginners often mistake them for illuminated cirrus clouds at first, but ordinary clouds darken after sunset. Noctilucent clouds keep glowing with an oddly cold brightness.

How and when I'm watching it

You wouldn't typically go out on a special trip to see noctilucent clouds — it's too much of a long shot (though if they're sighted one night, going out the following night is a good idea). Instead, I have developed a habit of checking the northern horizon obsessively every clear July evening before bed. If I'm lucky, I'll pause if the twilight looks suspiciously textured. Noctilucent clouds don't hang around for long — they reward attentiveness more than planning. You don't need telescopes or even dark-adapted eyes, just a willingness to keep looking north during a season when many astronomy enthusiasts assume nothing interesting is happening.

Stargazer's corner: July 10-17, 2026

The real challenge in July is not moonlight but the simple fact that darkness never fully settles at northern latitudes. This week, the moon wanes toward new, creating some fabulous opportunities for anyone crazy enough to get up very early. The prime moment is about 80 minutes before sunrise on July 11, when you can glimpse a 15%-illuminated waning crescent moon curled up to the Pleiades open cluster (M45), with Mars and red supergiant star Aldebaran below. For something more leisurely, look west after sunset on July 17 to see the exact opposite sight — a 15%-illuminated waxing crescent moon close to Venus. Put a telescope on Venus itself, and you'll see that it's now a 60%-lit gibbous shape as it gets closer to Earth.

Constellation of the week: Cassiopeia

Cassiopeia becomes especially useful during the noctilucent cloud season because it remains visible above the northern horizon throughout summer twilight. It's a familiar W-shape that cuts through even bright skies surprisingly well. It's a circumpolar constellation, so it always sits opposite the Big Dipper, forming two distinctive shapes permanently wheeling around Polaris, the North Star.

My latest stargazing obsession

I'm always on the lookout for puddles. The dark skies coming this week will be a fabulous time to photograph nightscapes, including the Milky Way, but composition is everything. The night sky reflected in still water can look more dramatic than the sky itself because reflections compress and simplify structure. If I'm under a dark sky (or even in twilight) with a camera, I actively search for reflective surfaces — parked car roofs, wet pavements, ponds and puddles. Stargazing teaches you that observing is not always about pointing higher into the sky. It's often just as much about noticing how Earth participates in the view.

Before dawn on July 11, early risers will be treated to a striking celestial scene low in the east-northeast sky.

A slender waning crescent moon, softly glowing with earthshine, will appear to align with the orange light of Mars, the orange-red star Aldebaran, with the sparkling Pleiades and Hyades star clusters close by. Together, they will form a beautiful morning tableau in Taurus — one well worth setting an alarm to see.

First: the moon

Most obvious is, of course, the moon, appearing as a lovely waning crescent, 14% illuminated. It rises around 2:00 a.m. local daylight time and will likely appear as a thin arc of light enclosing a ghostly ball. Here is one of nature's beautiful sights and fits the old saying, "the old moon in the new moon's arms." Leonardo da Vinci (1452-1519) was the first to recognize it as earthshine. That faint bluish-gray light is light from Earth reflected toward the moon. Earth's light, of course, reflects sunlight, so earthshine is really sunlight that is reflected off Earth to the moon and reflected toward Earth.

Next: Mars

The second object is a planet: Mars. It will appear as an orange-yellow star roughly five degrees below and slightly to the right of the moon. Your clenched fist held at arm's length measures roughly 10 degrees in width, so Mars will hover roughly 'half a fist-width" below the lunar disk.

Mars rises around 2:40 a.m. local time and is about 15 degrees above the east-northeast horizon by dawn. So as the eastern sky begins to lighten up, Mars will be about "one and a half fist-widths" above the horizon.

It currently resides within the boundaries of the zodiacal constellation of Taurus the Bull. Mars remains rather inconspicuous, but its luminosity continues to increase as we gain on it in our smaller, faster orbit, though it is a very slow process. The planet moves from 17.5 light minutes away on July 1 to 15.4 light minutes by Sept. 1, brightening ever-so-slightly from magnitude +1.3 to +1.2. At its closest approach this coming February, Mars will be only 5.6 light minutes from Earth and will appear to shine fully 10 times brighter than it does now.

Finally: Aldebaran

Shining about 5.5 degrees below and slightly to the right of Mars will be a similarly hued, orange-red star, appearing to shine nearly twice as bright as the planet. That will be Aldebaran, marking the angry right eye of Taurus. Aldebaran is the fourteenth brightest star in the sky and lies 67 light-years from Earth. This is a red giant star, 45 times larger than our sun, 1.6 times more massive and over 400 times as luminous. Aldebaran is older and redder than the sun and is preparing to fuse its lightweight core into heavier elements, which are common among stars of its type. Aldebaran has a surface temperature of about 6,760 degrees F (3,738 degrees C). And Aldebaran is really a double star; its companion is much smaller and far dimmer, with an overall mass less than half that of the sun and only about one-third as large.

Incidentally, although it appears among them, Aldebaran is not actually a member of the V-shaped Hyades cluster. But it's much closer to us in space than the other Hyades stars, so it's simply an "innocent bystander," but nicely completes the V-shaped face of the Bull in our sky. Henry M. Neely (1879-1963), a long-time lecturer at New York's Hayden Planetarium, wrote in his book: A Primer for Stargazers:

"When Taurus is in the night sky, it is well worth the while of any stargazer to beg, borrow or steal a pair of binoculars. . . because the most dazzling of the stars are not visible to the naked eye. This is particularly true of the area inside the V of the Bull's face. Someday I hope an imaginative designer of jewelry will duplicate this superb setting of celestial gems, matching them in color, sparkle and design."

And completing this lovely early morning tableau, is the beautiful Pleiades star cluster. They'll glitter, as Tennyson imagined, "like a swarm of fireflies tangled in a silver braid." They'll sparkle about six degrees to the moon's upper right. Good binoculars will reveal a score of stars in this little group, while long-exposure observatory photographs show about 1000 in the area — all suffused in great clouds and streamers of nebulous light.

What a great way to start the second weekend of July!

So, rise before the first blush of dawn, seek out a clear east-northeast horizon, and let the morning sky reward your early vigil. With binoculars in hand, linger a little longer among the Pleiades and the nearby celestial jewels—an ancient sparkle waiting quietly above the waking world.

If you're looking for a telescope or binoculars to observe the night sky, our guides for the best binocular deals and the best telescope deals can help. Our best cameras for astrophotography and best lenses for astrophotography can help you get ready to capture the next stunning skywatching event.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

Between July 7 and July 17, Venus will put on two evening-sky shows: first passing close to Regulus, the brightest star in Leo the Lion, and then appearing near a waxing crescent moon.

Both events are easy to see with the naked eye and offer excellent opportunities for casual skywatchers and photographers alike.

Look low in the western sky after sunset for both events. Viewing times and positions are best suited for observers at mid-northern latitudes; check a local skywatching app for exact timing in your area.

When to look: Around 9:45 p.m. local daylight time in mid-twilight.

Where to look: Low in the western sky for Venus and Regulus; west-northwest for Venus and the crescent moon.

Best tools: Both events are visible to the unaided eye, but binoculars will improve the view.

Venus meets Regulus

The first celestial meeting will be when Venus aligns with the blue-white star Regulus, the brightest star of Leo, the Lion. Six stars in Leo form a large backward question-mark shape, popularly known as the Sickle. Regulus is at the end of the handle. It was one of the four "royal stars" which were supposed long ago to rule over the four quarters of the heavens. On the list of the 21 brightest stars, Regulus is number 21, but at least it's on the list.

Key dates

Silvery white Venus and blue-white Regulus will be 3 degrees or less apart from July 7 through 12th and will be closest — just one degree apart — on July 9.

July 7: We see them side by side, Venus on the right, Regulus on the left.

July 9: They're somewhat closer, with Venus to the upper right of Regulus.

July 11: The gap between them will be noticeably wider with Venus sitting to the upper left of Regulus. Look low toward the west around 9:45 p.m. In late twilight, both planet and star will be readily visible to the unaided eye. The difference between the two is considerable: Venus will outshine Regulus some 158 times; binoculars will enhance the view.

Venus pairs with the moon

Then, on July 17 comes the second meeting, this time with the moon. The moon will be 3.5 days past new phase, a slender crescent 17% illuminated, sitting to the left of Venus. They will not be particularly close together, being separated by about 6 degrees by mid-twilight. Regardless, both will attract attention, calling even casual observers to look at them as they descend toward the west-northwest sky, finally setting at around 10:30 p.m. As was the case with Regulus, binoculars will enhance the view of Venus with the moon. You'll no doubt notice earthshine — sunlight reflected from off the Earth toward the moon, which will faintly illuminate its dark part with a greyish-blue glow, seemingly imparting a three-dimensional effect.

What's next for Venus?

Near the start of this year, Venus was situated behind the sun at superior conjunction (on Jan. 6) and entered the evening sky, yet it was hidden from our view for many weeks due to its proximity to the sun. But Venus rapidly climbed out of the bright evening twilight during March, becoming by far the most brilliant of all the "stars," and by mid-June it stood nearly 30 degrees above the sunset horizon and was setting 2.5 hours after the sun.

Since then, Venus has taken a track placing it increasingly to the south of the sun's path across the sky. The result of this is that although its angular distance from the sun continues to increase, this is balanced out by its southerly track, which in the coming days and weeks will cause it to become progressively lower and set gradually earlier relative to the sun.

As such, compared to now, Venus will be noticeably lower in the western evening sky at its greatest elongation (46 degrees) on Aug. 15. Come the end of September, it rapidly sinks, appearing as an increasingly large, thinning crescent through telescopes and steadily held binoculars. At mid-northern latitudes, we'll have to struggle to catch it very low in the west-northwest soon after sunset during the final nights of September. It falls past the sun on October 24th — well south of it (6 degrees) at this inferior conjunction, so any chance of trying to get a glimpse of it on those evenings and mornings of adjacent days will be solely for those who reside south of the equator, in the Southern Hemisphere.

But during November, it will dramatically sprout up into the morning sky, ultimately grabbing the attention of early risers and providing us with a perfect "Star in the East" adorning the predawn sky during the Christmas season.

If you're looking for a telescope or binoculars to observe the night sky, our guides for the best binocular deals and the best telescope deals can help. Our best cameras for astrophotography and best lenses for astrophotography can help you get ready to capture the next stunning skywatching event.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

For the Aug. 12, 2026, total solar eclipse, Spain's great cities will be pulling in eclipse-chasers from across Europe, but not every famous destination is equally well placed. In Barcelona and Madrid, the eclipse is a near miss — dramatic on paper, yet ultimately disappointing. Madrid gets a 99.96% partial eclipse, which means no totality, so no corona, no twilight sky and no plunge in temperature. Cue a mass exodus from Spain's two biggest cities in search of totality.

To experience a total solar eclipse, you need to be inside the narrow path of totality stretching across northern Spain, from the northwest coast to the east coast. Timing and geography matter because this is a very low-sun eclipse, with totality arriving close to sunset. Coastal beaches, riverbanks, hilltop miradors and elevated parks with unobstructed west-northwest horizons will become prime real estate for one of Europe's most anticipated astronomical events. Here are 10 cities for the eclipse, with recommended viewpoints.

Essential resources for checking and re-checking intended destinations for totality include Xavier Jubier's Interactive Google Map, which has timings and built-in sight lines from Peak Finder, as well as The Eclipse App, Eclipse Horizon Checker and the Instituto Geográfico Nacional. However, nothing beats being in place the night before to check for trees and other obstructions at the time of the eclipse. All times and cloud statistics come from Time and Date and are for totality only.

1. Valladolid

Surrounded by flat land and with an excellent chance of clear skies, Valladolid is one of the top spots for the eclipse. There will be some clear sight lines from the east bank of the Pisuerga River, specifically its Playa de las Moreras river beach, though buildings will complicate things, so play it safe and head to the Parque Urbano de las Contiendas on the west side.

2. Palencia

One of the destinations most likely to have clear skies, Palencia is surrounded by flat, open landscapes perfect for viewing a low-altitude eclipse. Key locations include the scenic Mirador de Palencia, overlooking the city from the southwest, and the elevated Cristo del Otero, overlooking the city from the north.

3. León

This historic city south of the Cantabrian Mountains is bound to be one of the hotspots for the eclipse. Considered one of the best spots to watch the sunset because of its panoramic views of the city, Mirador de las Lomas (specifically Mirador de Las Lomas Tres), overlooks León from the east and offers panoramic sunset views across the city.

4. Zaragoza

On the Ebro River between Madrid and Barcelona, Zaragoza is best known for its spectacular Basilica of Nuestra Señora del Pilar (Basilica of Our Lady of the Pillar). It just so happens that, from the historic Puente de Piedra bridge, photographers may be able to capture the totally eclipsed sun just above the silhouette of its spires. Expect crowds here, and also on the San Lázaro riverfront behind. For a quieter spot, follow the Ebro River northwest away from the city center.

5. Burgos

Famed for its medieval architecture, this provincial capital will be busy for the eclipse, but pay close attention to sight lines. Many will be close to the historic Arco de Santa María, but it's poorly placed, so instead get yourself on the northwest bank of the elevated Parque del Castillo for a low panoramic view of the city — and the eclipse.

6. Logroño

A stop on the pilgrimage route to Santiago de Compostela, Logroño — 92 miles (148 km) south of Bilbao — is famed for the twin towers of its Cathedral of Santa María de la Redonda. Its Parque de Ebro, on the banks of the River Ebro, is ideal for eclipse-viewing, with the Puente de Piedra bridge also offering a clear view.

7. A Coruña

The first major city on mainland Europe to experience totality will be A Coruña in northwestern Spain, where its crescent-shaped Riazor and Orzan beaches will doubtless be crowded for the occasion. They're close to the city center, home to exquisite Galician seafood restaurants.

8. Gijón

There are lots of places to watch the eclipse from this large coastal city in northern Spain. The clifftop park on Santa Catalina hill is bound to be busy, but there's plenty of space on the beaches on either side — the crescent-shaped Playa de San Lorenzo on the east and artificial Playa de Poniente on the west.

9. Bilbao

Bilbao, on the Bay of Biscay at the northern edge of the path, gets a short totality, but has a spectacular elevated spot to watch the eclipse close to the center. Artxanda Viewpoint is a three-minute journey via funicular railway and gives panoramic views of the city. It's a popular sunset spot in August, so it's bound to be busy.

10. Madrid (San Sebastián de los Reyes)

Frustratingly for madrileñas, madrileños, and eclipse planners, Puerta del Sol (Gate of the Sun), at the heart of Madrid, gets a 99.96% partial solar eclipse. Only its northern suburbs see totality, including San Sebastián de los Reyes, 12 miles (20km) north. El Mirador de Pichón has a clear sight line to a short, dramatic totality. San Sebastián de los Reyes is one of 11 observation points curated by the Community of Madrid.

What did the evening sky look like for Benjamin Franklin, Thomas Jefferson, and their contemporaries on July 4, 1776?

As the United States marks its 250th birthday, many astronomy enthusiasts may be asking exactly that. If you stepped outside around 9 p.m. local time on July 5, 1776, the sky would look much as it does today. Only careful measurements would show that the stars were not in quite the same positions they occupy in 2026.

To understand the sky more fully, it helps to look at how people in 1776 tracked celestial events and what they would have expected to see overhead.

But first, how did people in 1776 keep track of astronomical phenomena? People studied astronomy for practical reasons both in and out of the classroom. It was essential for navigation, surveying, timekeeping, and charting unfamiliar lands. In an age before light pollution, ordinary people were also likely far more familiar with the stars and constellations than most people are today.

Almanacs: timetables of the heavens

In the American colonies of the 17th and 18th centuries, an almanac ranked just behind the Bible in everyday importance. It listed sunrise and sunset, moonrise and moonset, the times when bright stars reached their highest points in the sky, lunar phases, planetary positions, some astrological lore, and practical information such as road conditions, husbandry tips, and weather forecasts.

By the early 18th century, numerous almanacs were in print. Many survived only a few years, but a bestseller could support its printer well into the following year. Among the most successful was Benjamin Franklin's "Poor Richard's Almanack", published in Philadelphia under the pseudonym Richard Saunders from 1732 to 1758. It became immensely popular, selling more than 10,000 copies annually. Franklin has often been called America's first true Renaissance man — an author, printer, politician, diplomat, inventor, and scientist who counted astronomy among his interests.

Later, yearly "prospectuses of the sundry celestial events" could be derived from the extensive calculations appearing in "The Nautical Almanac", established in 1766 by Dr. Nevil Maskelyne, the fifth Astronomer Royal of England.

The planets visible over the U.S. in 1776

For anyone consulting an almanac for the year 1776, they would find that only one planet could be readily viewed after sundown. Saturn, in the constellation Virgo, passed opposition to the sun on April 7 and during July would be evident in the southwest sky at dusk, shining with a yellowish-white glow and appearing slightly brighter than the bluish first magnitude star Spica, about 7 degrees to its lower left. On the evening of July 22, a waxing crescent moon would appear to form a broad triangle with Saturn and Spica. Of course, Saturn's most notable telescopic feature is its ring system, which at that time was tilted 10 degrees from edge-on with its north face in view.

Toward the end of the month, three other planets would be available about 90 minutes before sunrise, low in the east-northeast amidst the stars of Gemini: Mercury, Jupiter and Mars. Dazzling Venus would be invisible due to its proximity to the sun.

The great lunar eclipse of July 1776

The month's most anticipated astronomical event was the total lunar eclipse of July 30. By the standards of most eclipses, it was exceptional: totality would last an unusually long 1 hour 35 minutes. Unfortunately for observers in Philadelphia, New York, Boston, and many other locations, much of the spectacle unfolded before moonrise. Mid-totality was predicted for "7:01 o'clock in the evening," before the moon rose, and the moon would begin emerging from Earth's shadow at 7:49 p.m., when it was positioned just above the east-southeast horizon. It would "quit the shadow completely" at 8:48 p.m.

The eclipse came just 26 days after the Declaration of Independence was unanimously adopted by the Second Continental Congress in Philadelphia. It was widely observed and discussed in journals of the era and later became part of Revolutionary War Lore. In a time of profound uncertainty, early Americans watched it closely despite poor viewing conditions. Diarists and observers, including hymn writer John Newton and militia officers, often treated the event as an omen reflecting the gravity of the Revolution. The Declaration of Independence was engrossed on parchment, and delegates began signing it on Aug. 2, 1776, only three days after the eclipse.

Beyond the month's most dramatic event lies a subtler question: whether the background stars themselves would have looked meaningfully different from the way they appear today.

Did the stars look different 250 years ago?

Besides rotating and revolving, Earth has an oscillating motion like that of a spinning top due chiefly to the pull of the moon on Earth's equatorial bulge. Each oscillation takes about 26,000 years. Thus, the North Pole traces a circle in the sky, pointing to different stars as it moves in its circuit.

Consequently, Polaris wasn't as good a pole star in 1776, being 1.88 degrees from the celestial pole compared to 0.63 degrees today. Put another way: the gap between the celestial pole and Polaris measured nearly four moon-widths in 1776 compared to just over one-width today.

What about proper motion? Have any stars shifted noticeably in 250 years? The only one would be the brilliant orange star Arcturus in Boötes, which has the largest proper motion of any 1st-magnitude star, but since 1776 has drifted only about 0.13 degrees (equal to about one-quarter of a moon diameter) with respect to its fainter neighbors.

The weather on America's first Independence Day

One final detail adds historical texture: the weather in Philadelphia on July 4, 1776, was pleasant and mild, with clear morning skies giving way to increasing clouds by afternoon. Weather journals kept by Thomas Jefferson and local observer Phineas Pemberton record a high of 76° F. Those later clouds, however, might have obscured much of the sky on that first night of Independence.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

I used to think Uranus was the sort of planet you graduated into. Saturn and its rings first, obviously. Jupiter and its cloud bands soon after that. Venus, if it's shrinking to a crescent (which it soon will be), and, of course, Mars and its ice caps. But Uranus? The seventh planet feels like something reserved for people with huge telescopes, expensive eyepieces and incredibly lucky atmospheric seeing. It may be considered an ice giant planet, but it's almost four times farther from the sun than Jupiter and twice as far as Saturn — and it's a lot smaller than both. Uranus didn't figure in my plans.

And yet on a frosty evening in September, a few years ago, I finally got to see it as a blue-green dot nearly 1.8 billion miles away. It was through a large Dobsonian telescope belonging to one very generous member of the Salt Lake Astronomical Society, outside the visitor center at Bryce Canyon National Park, which hosts popular astronomy and night-sky programs. Uranus shone dimly, but I could easily make out its color by averting my eyes (looking slightly to the side of the planet rather than directly at it). That way, the human eye's light-sensitive peripheral cells can catch brightness — it's a technique that's worth learning for all kinds of telescopic astronomy. Even then, Uranus looked like a faint, motionless star rather than a glowing planet. It was no Saturn.

What surprised me wasn't finally seeing Uranus — that was down to a massive telescope. It was how suddenly my perception changed once my eye locked onto it. After seeing it up close (ish), I wanted to know exactly where Uranus was in the night sky. Uranus is technically visible to the naked eye, but it is very challenging to see. It shines at 5.7 magnitude — right at the absolute limit of human visibility, but in Bryce Canyon's dark moonless skies, it was definitely there. Was it a satisfying sight? Not especially — but I could not unsee it. That transition — from looking casually to carefully observing, first with powerful optics and then navigating with the naked eye — is what observational astronomy is all about. Uranus now always figures in my plans, but typically only when I have access to a very large telescope.

Finally seeing Uranus is a milestone. Most people remember their first view of Saturn because its rings impress immediately. But many people remember Uranus because they had to work for it. It's a planet you can discover for yourself — and you can do it this week.

What's happening and when to look

I tend to forget all about Uranus unless it's involved in a conjunction — and that's exactly what's happening. Conjunctions involving Uranus tend to occur a couple of times each year, typically as one of the fast-moving, closer planets — such as Venus and Mars — appear next to it. Venus was close to Uranus back in April, and on July 4, it's the turn of Mars. A conjunction between Mars and Uranus happens about every two years as the red planet surges past on its far quicker journey around the sun (687 Earth days versus the 84 years it takes Uranus).

This won't be the most convenient conjunction to observe, but they'll get to within about 11 arc minutes of each other — extremely close! From the northern hemisphere, the planets will be low on the eastern horizon in the early morning hours before astronomical dawn. The best time to be up and looking east will be about 3:45 a.m. local time. The observing window is only about 45 minutes before dawn, making it harder to find with every passing minute.

How and when I'm watching it

Find Mars, find Uranus. That's the entire point of using a close conjunction to see the seventh planet. Mars will serve as a guidepost and be easy to see. It will shine at 1.3 magnitude below the sparkling Pleiades open cluster. You won't be able to miss it in a clear sky. All you have to do is look slightly above Mars for Uranus — first with the naked eye, then with any pair of binoculars (I'll be using 10x50 binoculars). The conjunction will be close enough to fit comfortably in binoculars and to look beautiful in a small telescope, if you have one.

Normally, locating Uranus involves hopping through fairly anonymous star fields while constantly second-guessing whether you are looking at a star or the planet itself. Here, Mars does the navigation for you. Your reward will be the sight of a tiny pale point with a subtle blue-green tint. The satisfaction comes less from appearance and more from seeing something so distant directly with your own eyes.

There's also something fitting about this conjunction falling on July 4 during the 250th anniversary year in the U.S. Uranus takes 84 years to orbit the sun, meaning it has completed almost exactly three orbits since the Declaration of Independence was signed in 1776. The planet itself was not discovered until 1781, when William Herschel identified it while searching the sky systematically rather than casually. It's a reminder that back in 1776, only six planets were known about. Now we're on a hunt for a ninth planet (sorry, Pluto).

Stargazer's corner: July 3-9, 2026

July opens with a slowly darkening sky after the long twilight of late June. Earth reaches aphelion on July 6, its farthest point from the sun (the seasons are driven by Earth's tilted axis, not its distance from the sun). So the sun's disk will be at its smallest in the sky, one factor contributing to the total solar eclipse on Aug. 12. Meanwhile, the very early hours of July 7 and 8 will see a close conjunction of a last quarter moon and Saturn in the east, kicking off relatively moonless conditions for the following 10 nights or so.

Asterism of the week: Summer Triangle

By early July, the Summer Triangle dominates the sky after dark. Formed by Vega, high overhead, Deneb to the northeast and Altair lower in the south, it creates a vast, unmistakable pattern that defines the season. It's actually not a constellation, but an asterism — a popular shape in the sky, like the Big Dipper — and its scale is what makes it so useful. Once you've got it nailed, it becomes a framework for the entire sky, helping you orient yourself instantly all season long. It also traces the path of the Milky Way, which runs straight through it, adding an extra sight if you're somewhere not blighted by light pollution.

Aside from fireworks, what better way to celebrate 250 years of independence than by launching your own model rocket into the sky? The limited edition Estes Liberty Star rocket is the perfect model for the job, decked out with a blue and red styling and featuring beginner friendly assembly for an easy setup.

You can get the Estes Liberty Star America 250th Celebration model rocket for $38.84 on Amazon

Estes features a lot in our model rocket guide, with six of their models included. They are the biggest name in model rockets and have the reptuation to back it up. This special edition rocket was designed for the once-in-a-lifetime milestone of 250 years of American independence. For something that is a bit different from a fireworks show, launch this proud rocket and watch it return to solid ground this Independence Day.

• We've got you covered with reviews and rankings of the best telescopes, binoculars, star projectors, cameras, drones, Lego, streaming and more.

It's an extra-special Independence Day this year, celebrating 250 years of America, and I'm sure that celebrations will be lasting longer than July 4. The Estes Liberty Star is a limited edition model rocket styled in red, white and blue with a projected altitude of 920 feet. It makes a great commemorative decoration of this special anniversary or it might make an exciting first flight for a loved one and kick off a lifelong hobby of model rocketry. If you don't have a launch setup already, we would recommending grabbing an Estes Porta-Pad II and an Estes 3/16-inch Maxi launch rod, along with a C11-5 or D12-5 model rocket engine from a hobby store. Asides from the extra purchases, this is an extremely beginner friendly model rocket, with a setup time under 10 minutes.

Estes is a household name in model rocket enthusiast circles and they helped revolutionise the entire industry in the 1950s with the National Association of Rocketry (NAR). Before Estes and the NAR, teenagers were making their own fuel for model rockets and the lack of regulation often led to severe injuries. Independence Day is synonymous with pyrotechnics but all kinds of explosive material can be life-threatening, so rest assured you are getting a patriotic rocket from a safety pioneer. That being said, extreme caution should always be followed when operating a model rocket with an engine and launch pad, as apart from self-injury, there is also a high risk of fire, so make sure you launch in a wide open area and check local fire laws.

Key features: Red, white and blue styling, beginner skill level, pre-molded plastic fins for easy setup, 15-inch (38 cm) recovery parachute, maximum altitude of 920 feet (280 m), 3.5 oz (99.2 g) weight.

Product launched: June 2026

Price history: This product was launched at $38.84 and has not seen any price fluctuations.

Price comparison: Amazon: $38.84 | Walmart: $38.84

Reviews consensus: We haven't reviewed any Estes rockets but they have a great reputation in the model rocket community and our editor-in-chief Tariq Malik has used a few models and loves them.

✅ Buy it if: You want to celebrate or commemorate the 250th anniversary of Independence Day with a limited edition red, white and blue rocket.

❌ Don't buy it if: You don't have access to a large open area or you live in a restricted area. Local laws and fire codes may totally ban model rocketry in your area.

Check out our other guides to the best telescopes, binoculars, cameras, star projectors, drones, lego and much more.

Want to see Uranus for yourself? Independence Day morning offers one of the best opportunities in decades, as the distant ice giant passes extraordinarily close to Mars in the predawn sky.

Although we often hear that only five planets are visible to the unaided eye, Uranus can also be seen from Earth under the right conditions. As the seventh planet from the sun, it is very faint — near the threshold of naked-eye visibility at roughly sixth magnitude — so viewing it requires a very dark sky with little to no significant light pollution.

The second challenge is knowing exactly where to look. Uranus is faint enough to blend into a background of similarly dim stars, but early on Saturday, July 4, at around 4 a.m. local daylight time, Mars provides a useful guide. On that Independence Day morning, Mars and Uranus will appear unusually close together in the sky.

Finding Mars first

Mars currently rises about half an hour before the first light of dawn. It is still relatively faint at about magnitude +1.3, and through a telescope it appears tiny, measuring less than 4.5 arc seconds across. Look for it low in the east-northeast, about 5.5 degrees directly below the Pleiades star cluster.

• Find Mars low in the east-northeast before dawn.
• Point binoculars or a small telescope at Mars.
• Look almost directly above Mars for a much fainter, star-like point of light. That will be Uranus.

What Uranus will look like

Uranus should resemble a tiny greenish star and will appear only about 1/63 as bright as Mars. Although Uranus is nearly 7.5 times larger than Mars, it is more than 9.5 times farther away as seen from Earth. At about 1.88 billion miles (3.02 billion km), it appears only slightly smaller than Mars in apparent size, measuring about 3.5 arc seconds across.

How close will they be?

According to Belgian celestial calculator Jean Meeus, Mars and Uranus will be closest at 5 a.m. Universal Time (UTC) on July 4, when only 6 arc minutes will separate them. For comparison, Mizar — the middle star in the Big Dipper's handle — and its fainter companion Alcor are separated by about 12 arc minutes. In other words, Mars and Uranus will appear only half as far apart as Mizar and Alcor.

Observers with exceptionally sharp vision and very dark skies may want to try spotting Uranus near Mars without optical aid, though binoculars or a small telescope will make the view much easier.

Mars and Uranus are in conjunction on average once every 2.38 years. But meetings as close as this one are quite rare, occurring on average once about every 40 years. The next similarly close approach between these two worlds that is readily visible in a dark sky is not due until Dec. 8, 2147!

A Bonus Target: HIP 19146

If you are using a small telescope, look for an even fainter object about 2 arc minutes below Uranus. This is not a Uranian satellite, but a background star cataloged as HIP 19146. The "HIP" designation comes from Hipparcos; a European Space Agency satellite launched in 1989 and operated until 1993. Hipparcos was the first space mission devoted to precision astrometry, the accurate measurement of celestial positions and distances.

On the morning of the upcoming Mars-Uranus conjunction, try to spot this eighth-magnitude star as well. It is about 11 times dimmer than Uranus and lies roughly 882 light-years from Earth.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

The United States' 250th birthday is almost here, so why not take a break from the fireworks and explore four America-themed wonders hiding in the summer night sky?

Our celestial sightseeing targets run the gamut from lone stars and constellations to historic lunar landmarks and an uncannily shaped nebula — some of which will require a small telescope or a camera to truly appreciate.

If you're new to the night sky, then you may want to check out our roundup of the best stargazing smartphone apps, which will help you navigate to specific targets using augmented reality technology.

Apollo 11 landing site

One of America's finest moments came on July 20, 1969, as Apollo 11 astronauts Neil A. Armstrong and Edwin E. "Buzz" Aldrin Jr. took humanity's first steps on the surface of Earth's moon. Here's how to spot the region of the moon that contains the Apollo 11 "Tranquility Base" landing site with the naked eye on the weeks surrounding a full moon.

First, find the dark expanse of Mare Tranquilitatis darkening a swathe of the moon's eastern limb close to the equator, where ancient lava flows once filled networks of impact basins before solidifying to create vast basaltic plains.

The Apollo 11 landing site is located on the southwestern shore of the Sea of Tranquility, between the Sabine and Moltke impact craters, which can be spotted with the aid of a small telescope. You can also search for the Apollo 11 backup landing sites using our handy guide, or even attempt to find where each Apollo-era mission touched down on the lunar surface.

Spica

The United States' relationship with the night sky dates back to its founding. After all, the stars depicted on the nation's earliest flags were intended to symbolize the birth of a new constellation, with each representing one of the 13 original colonies that formed the early union, according to the Smithsonian Institution.

You can honor that spirit on the nation's semiquincentennial anniversary by finding a star whose light left its surface around the same time that the United States declared its independence!

The blue-white double star system Alpha Virginis — known better as Spica — is located roughly 250 light-years from Earth in the constellation Virgo. As such, the light cast out from its surface some 250 years ago is only now reaching Earth, having traveled for centuries through the near vacuum of space at the speed of light — a blistering 186,282 miles per second (299,791 kilometers per second).

To find Spica, you first need to locate the seven bright stars of the Big Dipper asterism above the northwestern horizon after sunset, and trace an imaginary line along the curve of the Big Dipper's handle. Do that, and you'll come across the bright orange star Arcturus, the 4th brightest star in the night sky. Continue that arc beyond Arcturus and the next bright blue-white star you find will be Spica!

The constellation Aquila

Next up, we have the constellation Aquila, the "Eagle", which shines along the glowing ribbon of the Milky Way in early summer. The constellation evokes the shape of a great Bald Eagle, which was adopted as a national emblem of the United States in 1782. Aquila itself has been associated with an eagle for thousands of years and was catalogued by the ancient Greek astronomer Claudius Ptolemy in the second century AD.

A good way to find Aquila is to search for the bright star Altair, which can be seen glowing halfway up the southern sky to the left of the Milky Way for viewers in the U.S. around midnight in early summer. Altair, along with the nearby stars Alshain and Tarazed, represent the head of the great eagle, while the body and raised wings of the celestial bird are depicted in a cross formation of stars beneath.

North America Nebula

Our final stop is the North American Nebula — a gorgeous emission nebula whose vast glowing clouds of interstellar hydrogen resemble the outline of North America.

The North America Nebula is too faint to see with the naked eye. However, a pair of 10x50 binoculars or a small telescope should reveal the star-forming region as a gentle brightening in the band of the Milky Way from a dark sky location, less than five degrees from the bright star Deneb, which shines above the eastern horizon after sunset.

Its structure is best seen through long exposure photography, which will help reveal the dusty filaments and chaotic cosmic clouds that form the nebula. Read our beginner's guide to photographing the Milky Way for more!

Want to get a closer look at the night sky? Then be sure to check out our roundups of the best telescopes and binoculars for stargazing, along with our expert tips for beginning your amateur astronomy journey.

Editor's Note: If you would like to share your astrophotography with Space.com's readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.

The July full moon occurs at 10:36 a.m. EDT (1436 GMT) on July 29, when the lunar disk appears fully lit as it shines opposite the sun in Earth's sky.

The July full moon is often called the "Buck Moon", to reflect the time of the year when young male deer grow out their antlers in the northern hemisphere and is the first full moon of summer, occurring soon after the 2026 summer solstice.

When to see the July full moon

Look to the east at sunset on July 29 to catch the full Buck Moon as it climbs silently into the early summer sky, veiling the nearby stars of the constellation Capricornus behind the glare of its moonlight.

You may notice the lunar disk appear particularly large in the hour following moonrise. This phenomenon is known as the "Moon Illusion", wherein our brains trick us into thinking an object in the sky is bigger than it really is as it rests low on the horizon, with objects nearby to provide context.

Earth's moon could also take on an eye-catching yellow-orange color while close to the horizon, as an effect called Rayleigh scattering deflects the blue wavelengths of its light, while allowing the longer red wavelengths to travel through the atmosphere more easily.

The table below displays local full moon timings for when the moon is 100% illuminated for a selection of cities spread across the globe (note local moonrise and moonset times will vary depending on your location):

Why it's called the Buck Moon

July's full moon is also called the Buck Moon by some Native American tribes in reference to the furry antlers that grow from the heads of young deer around the time it rises. The Algonquin people also called it the Raspberry moon, evoking the fruit that ripens around that time in North America, while the Cree knew it as the Feather Moulting Moon, according to the Old Farmer's Almanac.

It is also known as the Thunder Moon, to reflect the intense storms that can arise in the hot summer months. European peoples, like the Anglo-Saxons, had their own traditional names for the occasion, linking it to the harvest time by referring to it as the Hay Moon, or Corn Moon, according to the Royal Museums Greenwich.

Cultural traditions and festivals

The July full moon marks the celebration of Guru Purnima for followers of the Hindu and Buddhist faiths, when worshippers take time to honor their teachers and spiritual guides — known as Gurus — by fasting, attending a temple and via acts of gratitude and service, per Time and Date.

July 29 also coincides with the holy day of Asalha Puja for the Theravada Buddhist community, which commemorates Buddha's first sermon, which occurred in Sarnath, India, where the spiritual leader imparted the "Four Noble Truths", according to the University of Birmingham.

What else to see in the sky around the full moon

The glare of the Buck Moon will hide many of the fainter wonders of the night sky when it rises above the southeastern horizon at sunset on July 29, making it an ideal time to spot some of the brighter asterisms and solar system planets that glisten in the summer sky.

First, look out for the dazzling trio of stars that form the famous Summer Triangle asterism. Altair can be found shining a little over 30 degrees above the silver glow of the lunar disk, with Vega and Deneb to its upper left, marking the brightest points in the constellations of Lyra and Cygnus, respectively.

The glowing ribbon of the Milky Way tumbles directly through this cosmic triangle before arcing towards the southern horizon, though its diffuse light will be hidden behind a veil of moonlight on the night of the full moon.

Next, look to the right of the Buck Moon to spot the red light of the supergiant star Antares glowing at the heart of the constellation Scorpius, with the stars Acrab, Dschubba and Pi Scorpii glowing above, representing the claws of the celestial beast.

Be on the lookout for bright shooting stars belonging to the southern delta aquarid meteor shower, which comes to a peak overnight on Jul. 30-31. Sadly, the light of the full moon will hide all but the brightest shooting stars around the peak, but there's always a chance that a dramatic fireball could appear to outshine even Venus in the night sky.

Venus will also be visible shining as a bright evening star shining low on the western horizon on the evening of July 29, but will set less than two hours after the sun, along with the stars of the nearby Leo, the lion.

The predawn sky will more than make up for the evening's scant planetary offering, as Saturn, Mercury and Mars form a majestic arc to the left of the full moon, just before it sets below the western horizon. Together, the planets sketch out the path of the ecliptic — the imaginary line that the worlds of our solar system traverse as they glide silently through the night sky.

Observing tips

July 2026 will see the 57th anniversary of the Apollo 11 moon landing. Why not celebrate by finding each of the Apollo-era landing sites using our handy observer's guide?

While you're at it, read our expert's guide to photographing the moon, along with our roundups of the best cameras and lenses for astrophotography, and track Earth's natural satellite as the shadows change its aspect over the course of the month.

Top tips to photograph the moon

• Use a tripod to keep your camera as steady as possible.
• Use a remote shutter/timer to prevent camera wobble.
• A smartphone stargazing app can help you find the exact point of moonrise on your local horizon.
• A lens with a focal length of 12-50 mm is useful for landscape photography, while a focal length of at least 400 mm is advised for capturing more detailed views of the lunar surface.
• The moon can be made to appear particularly large while close to the horizon next to foreground objects, where it may take on an orange-yellow appearance thanks to Rayleigh scattering. A cleaner, more "classic" view can be captured as it soars high overhead.

These times mark the exact instant of full illumination. Your specific moonrise or moonset may be hours earlier or later, depending on your location. For the best viewing plan, use an app such as Stellarium or Sky Safari 7 Pro to find your local moonrise time.

Editor's Note: Did you capture a beautiful picture of the moon and want to share it with Space.com's readers? Then please send your photo(s), comments, and your name and location to spacephotos@space.com.

Heads up aurora chasers! The sun has been very busy.

After unleashing an X1.1 solar flare on June 30, the sun continued its outburst by firing off 10 M-class solar flares in 24 hours! Several of these eruptions were accompanied by coronal mass ejections (CMEs) that appear to be at least partially Earth-directed.

Exactly how many of these solar storms will reach Earth (and how effective they will be) is still being calculated, but space weather forecasters say the coming days could bring heightened geomagnetic activity and increased chances of seeing the northern lights.

Solar physicist Tamitha Skov described the recent activity as a "Machine-gun sun" in a recent post on X, writing that more than five solar storms are on their way to Earth, with at least three offering "good chances" for aurora displays.

"NOAA and NASA model predictions do not show all the storms yet," Skov wrote, explaining that the rapid succession of eruptions has made them difficult to model. Skov added that the first storm could arrive before 8 a.m. EDT (1200 GMT) on July 3, with G2 or stronger geomagnetic storm conditions possible if the incoming CMEs carry a favorable magnetic orientation, allowing them to connect more efficiently with Earth's magnetic field.

According to NOAA's Space Weather Prediction Center, at least one CME from July 1 appears to have an Earth-directed component, although further analysis is still underway. The agency continues to forecast moderate (G2) geomagnetic storm conditions beginning tonight, driven primarily by the CME launched during the June 30 X-class flare, while noting that additional CMEs from the barrage of July 1 eruptions are still being analyzed.

Will the northern lights be visible?

The forecasts are looking increasingly promising for aurora chasers.

NOAA's latest forecast calls for moderate (G2) geomagnetic storm conditions around 8-11 p.m. EDT tonight (0000-0300 GMT July 3), with minor (G1) storm conditions for much of July 3. That could push the northern lights farther south than usual, potentially making them visible across parts of the northern U.S., including New York and Idaho, provided skies are dark and clear.

Exactly how impressive any display becomes will depend on how the incoming CMEs interact with one another and, crucially, the orientation of their magnetic fields when they arrive. When a magnetic field within a solar storm aligns the right way, it can more effectively transfer energy into Earth's magnetic field, producing stronger geomagnetic storms and brighter auroras.

However, nights remain short for observers in the northern hemisphere and lingering twilight could make auroras harder to spot.

That being said, it's worth making sure your cameras are charged and your aurora alerts are switched on. With multiple CMEs heading our way, there could be some natural fireworks lighting up the skies this July 4 weekend.

Northern Hemisphere aurora forecast courtesy of the U.K. Met Office

The three-planet evening show that graced June's twilight sky has now dwindled to one lone survivor.

Mercury and Jupiter are now swinging behind the sun and are lost in the bright solar glare. Only Venus remains evident after sunset, and even here the dazzling evening star itself is showing subtle signs of slowly dropping down into the sunset fires; it is getting noticeably lower in the western sky with each passing week. It will pass close to the brightest star in Leo the Lion, Regulus, during the second week of July.

Saturn is in a fine position to be viewed just before the break of dawn in the east-southeast. The famous rings are now tilted some 9 degrees toward Earth, once again making this planet a showpiece for telescopic observation.

Mars rises about 2.5 hours before sunrise but is ever-so-slowly becoming more conspicuous as it brightens while climbing a bit higher in the eastern sky. It will also serve as a benchmark to locate the much fainter planet Uranus early on the morning of July 4; this distant greenish world will then be positioned only about 7 arcminutes (less than one-quarter of the apparent width of the moon) above Mars. Certainly, if you have never seen Uranus before, this will be an excellent opportunity to sight it, either with a small telescope or binoculars, or even possibly with your unaided eyes.

In our schedule, remember that when measuring the angular separation between two celestial objects, your clenched fist held at arm's length measures roughly 10 degrees. Here's where and when to look for each planet during July.

Mercury

Mercury passes inferior conjunction and enters the morning sky on July 12. It's too low and dim to detect until about July 26 or maybe later. By Aug. 2, Mercury will reach a greatest western elongation of 19 degrees from the sun.

Venus

Venus is conspicuous as July's long evening twilights fade. If you live at mid-northern latitudes and look to the west about 45 minutes after sunset, you'll find Venus shining brightly about 15 degrees high this month. This is noticeably lower than it was in June.

The planet starts July by setting more than two hours after the sun and follows the sun down to the horizon somewhat sooner by month's end. Venus is still rather small in a telescope this month, but there's no doubt that it has a gibbous phase. It will be larger in apparent diameter but smaller in phase, down to about half lit, when it reaches greatest elongation from the sun in mid-August.

On July 9, you will notice a much dimmer but still reasonably prominent point of light near Venus: the bluish 1st magnitude star Regulus. Venus burns only 1 degree to the upper right of Regulus, which is 150 times fainter. They're less than 3 degrees apart from July 7 through July 12. On July 17, the 3.5-day-old crescent moon will sit 5.5 degrees to the left of Venus.

Earth

Earth reaches aphelion, its farthest point from the sun in its orbit, on July 6 at 1:30 p.m. EDT (1730 GMT). Our planet is then 94,502,962 miles (152,087,775 km) from the sun (measured center to center), which is 3.28% farther from the sun than we were at perihelion last Jan. 3; a change of only one part in 30.

Mars

Mars rises around 2:50 a.m. local daylight time and is positioned between the Hyades and Pleiades star clusters, low in the east-northeast sky by dawn. At magnitude +1.3, it remains rather inconspicuous, but its luminosity continues to increase as we gain on it in our smaller, faster orbit.

On Independence Day morning (July 4), Mars points the way to Uranus, which is only 1/63 as bright. But with good binoculars or a small telescope, this distant world should appear like a tiny greenish star, hovering just 0.1 degree above Mars. Uranus is 168 light-minutes from Earth and more than 9½ times farther than Mars.

On the morning of July 11, about 90 minutes before sunrise, look low toward the east-northeast horizon to see a waning crescent moon. About 5 degrees below it, you'll find Mars and about the same distance below the Red Planet, you'll find a similarly hued and somewhat brighter star, orange Aldebaran in Taurus the Bull.

Jupiter

Jupiter comes to conjunction with the sun on July 29; it's on the far side of the sun during July and can't be seen.

Saturn

Saturn comes up in the east around 1 a.m. local time at the beginning of July and 11 p.m. at month's end. It's located near the border separating the constellations Pisces and Cetus. By month's end, the rings are tilted 9.1 degrees from horizontal — their greatest tilt of the year. Early on the morning of July 7, you'll find Saturn mimicking a bright star shining with a sedate yellow-white hue, sitting well to the lower left of the moon.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

A restless Earth-facing sunspot unleashed a powerful X-class solar flare on June 30, triggering radio blackouts across parts of North America.

The X1.1 solar flare erupted from sunspot region AR4479, peaking at 4:50 p.m. EDT (2050 GMT) according to NOAA's Space Weather Prediction Center.

The intense burst of X-rays released during the eruption reached Earth in just over 8 minutes, triggering strong (R3) radio blackouts across the daylight side of Earth. This mainly affected high-frequency radio users across parts of North America who may have experienced temporary signal degradation or brief communication outages while the flare was at its strongest.

The eruption also launched a coronal mass ejection (CME) — a huge cloud of magnetized solar plasma hurled into space. Initial observations suggested most of the material was traveling northward, limiting the chances of a significant Earth impact.

However, after further analysis, NOAA's Space Weather Prediction Center issued a Moderate (G2) geomagnetic storm watch for July 3, indicating that at least part of the CME could land Earth with a significant blow.

Will we see the northern lights?

When Earth-directed, CMEs can interact with our planet's magnetic field and spark geomagnetic storms, which can produce dazzling northern lights displays.

A G2-level storm is capable of pushing the northern lights farther south than normal. According to NOAA, auroras could become visible across some northern and upper Midwestern U.S. states, from New York to Idaho, provided skies are dark and clear.

Exactly how impressive the display becomes will depend on the strength of the CME and, crucially, the orientation of its embedded magnetic field when it arrives. If conditions are favorable, the natural light show could provide an extra helping of "fireworks" just in time for the July 4 weekend.

What are solar flares?

Solar flares are sudden bursts of energy released when magnetic fields around sunspots become twisted and reconnect. They are ranked using five classes — A, B, C, M and X — with X-class flares representing the most powerful eruptions.

What are CMEs?

CMEs behave a little differently. Unlike the radiation from a solar flare, which reaches Earth at the speed of light, these clouds of charged particles typically take one to three days to reach us. If they arrive in the right magnetic orientation, they can disturb Earth's magnetic field and trigger geomagnetic storm conditions.

Editor's note: This story was updated at 9:30 a.m. EDT on July 1 to reflect NOAA's latest forecast, including the issuance of a G2 (Moderate) geomagnetic storm watch for July 3 following further analysis of the accompanying coronal mass ejection.

The first full moon of summer, June's Strawberry Moon, wowed skywatchers worldwide with a spectacular display.

June's full moon was the lowest-hanging full moon of the year for observers in the Northern Hemisphere. That's because a full moon always sits opposite the sun in the sky. During the summer solstice that just passed on June 21, the sun was following its highest path of the year; that means this full moon took the opposite route, skimming low across the southern sky.

It rose in the southeast, remained low above the horizon throughout the night and set in the southwest, delighting photographers around the world. Here are some of the best photos.

Photographer Davide Pischettola captured the Strawberry Moon behind the sailing ship Nave Italia in the Port of Molfetta, Italy, on June 29, 2026.

The June Full moon rises behind the skyline of midtown Manhattan and the Empire State Building in New York City in this vibrant image captured by photographer Gary Hershorn.

Hershorn was also in the right place at the right time to capture this well-positioned photograph of the Strawberry Moon atop the Empire State Building.

Even Lady Liberty appeared to embrace the Strawberry Moon in another striking image by Hershorn, with the full moon seemingly cradled in the Statue of Liberty's hand.

Meanwhile, in California, photographer Tayfun Coskun captured the Strawberry Moon emerging above San Francisco Bay in dramatic fashion.

The Strawberry Moon peeked through a thin layer of cloud as it rose above an ornate rooftop in Meishan, China.

The rich orange Strawberry Moon looks particularly striking in this image captured in Qingzhou, China, on June 29, 2026.

Photographer Robert Nemeti captured this dark and moody image of the Strawberry Moon rising above a Reformed Church in Abaújvár, Hungary, from a vantage point just across the border near Kechnec, Slovakia.

A glowing Strawberry Moon rises behind the ancient Temple of Poseidon at Cape Sounion in this remarkable image captured by photographer Ayhan Mehmet.

Photographer Veysel Altun captured the June full moon rising above a dolphin sculpture on the waterfront in Samsun, Turkiye.

A curious feline stole the spotlight as photographer Osmancan Gurdogan captured the Strawberry Moon rising over the skyline of Istanbul, Turkiye.

If you're looking for a telescope or binoculars to observe the moon, our guides for the best binocular deals and the best telescope deals are here to help. Interested in capturing the night sky? Check out our best cameras for astrophotography and best lenses for astrophotography.

Fancy taking a more in-depth moonlit tour of our rocky companion? Our ultimate guide to observing the moon will help you plan your next skywatching venture, whether it be exploring the lunar seas, mountainous terrain, or the many craters that blanket the landscape. You can also see where astronauts, rovers and landers have ventured with our Apollo landing sites observing guide.

The United States' 250th birthday is right around the corner and what better way to celebrate than by looking for a star whose light began its journey to Earth around the time the Declaration of Independence was signed?

Starlight travels through the near-perfect vacuum of space at a staggering 186,282 miles (299,791 kilometers) per second — or the speed of light. Even at this pace, it can take hundreds, thousands, or even millions of years for starlight to reach its destination, rendering each point of light in the night sky a twinkling time capsule, which represents a snapshot in the life of a star encoded at the moment the radiation left its source.

The blue-white double star system Alpha Virginis — known colloquially as Spica — happens to shine roughly 250 light-years from Earth. In other words, the light we see today left the star's surface 250 years ago, around the time that America's founding fathers signed the Declaration of Independence in 1776.

How to find Spica in the night sky

Finding Spica is easy. First, locate the Big Dipper, shining above the northwestern horizon in the hours following sunset in June for viewers in the U.S., with the three stars representing its "handle" pointing up and away from the horizon.

Next, draw an imaginary line following the arc of the handle out into space, until you find the red light of Arcturus, the 4th brightest star in the night sky. Continue the arc beyond Arcturus and the next dazzling bright blue-white star that you spot will be Spica, which twinkles above the southwestern horizon at sunset in early summer.

The single point of light that we call Spica is actually a pair of massive stars that orbit each other once every four days, while shining with the combined light of over 12,000 suns.

Another star at a similar distance from Earth is Bellatrix, which shines at the left shoulder of the celestial hunter depicted in the constellation Orion. This variable star is also located 250 light-years from Earth, but is sadly lost from view in the glare of the sun during the summer months.

Want to get a closer look at the night sky? Then be sure to read our roundup of the best telescopes and binoculars for exploring the post sunset realm, along with our beginner's guide to amateur astronomy.

Editor's Note: If you would like to share your astrophotography with Space.com's readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.

Editor's note: Wow, the Strawberry Moon 2026 certainly served up quite the treat! We've rounded up some of our favorite photos captured by skywatchers worldwide. If you didn't catch it last night, don't worry; it will still appear full for another night or two.

Get ready to see the first full moon of summer as the stunning Strawberry Moon rises tonight (June 29).

The moon officially reaches its full phase at 7:57 p.m. EDT (2357 GMT) on June 29 when it sits opposite the sun in Earth's sky and appears fully illuminated. While that will mark the exact moment of the full moon, our lunar neighbor will appear bright and round for a night or two before and after.

June's full moon will be the lowest-hanging full moon of the year. That's because it occurs close to the summer solstice, when the sun reaches its highest point in the daytime sky. As a full moon always appears opposite the sun, it follows the opposite path across the sky, tracing the year's lowest arc.

Look east shortly after sunset to watch the Strawberry Moon climb into the evening sky among the stars of the constellation Sagittarius.

June's full moon is known as the Strawberry Moon, a name linked to the short strawberry harvesting season traditionally observed by Native American tribes. Other names for June's full moon include the Rose Moon, Hot Moon and Mead Moon, according to Time and Date.

Despite its name, the Strawberry Moon won't appear pink. However, it may take on a golden or orange hue as it rises. This happens because moonlight must pass through a thicker layer of Earth's atmosphere when the moon is low on the horizon, scattering shorter wavelengths of light and allowing warmer colors to dominate.

You may also notice the moon appearing unusually large near the horizon. This is due to a phenomenon known as the moon illusion, a trick of perception that makes the moon seem bigger when viewed alongside distant landscape features.

If you're looking for a telescope or binoculars to observe the night sky, our guides for the best binocular deals and the best telescope deals can help. Our best cameras for astrophotography and best lenses for astrophotography can help you get ready to capture the next stunning skywatching event.

Editor's Note: If you snap a photo of the full moon and would like to share it with Space.com's readers, send your photo(s), comments, and your name and location to spacephotos@space.com.

Astrophotographer Efrain Morales captured spectacular footage of China's Tiangong space station as its silhouette buzzed Tycho Crater during a lunar transit on May 29, one night before May's Blue Moon.

Morales recorded the outlines of Tiangong's vast solar panels and habitable modules using a 12-inch telescope and astronomy camera as it passed silently across the lunar surface in the skies above Puerto Rico at 11:33 p.m. EDT on May 29 (0333 GMT on May 30).

"It is a challenge in less then a second to capture this event," Morales said in an email to Space.com. "Using a program the ISS Transit Finder helps in giving information to capture the space station. Adjusting the FOV and at times calculating last minute deviations in time and positions in which makes it more challenging."

The orbital outpost appeared to dive directly toward Tycho Crater, whose 53-mile-wide (85 kilometer) impact site and bright ejecta dominate the southern region of the lunar disk on the nights surrounding the full moon phase.

The dark expanses of Mare Nubium (the Sea of Clouds) and Mare Nectaris (the Sea of Nectar) can also be seen scarring the lunar disk to the left and upper right of the footage, respectively, where ancient lava flows hardened to form basaltic plains billions of years ago.

What is the Tiangong space station?

The Tiangong space station, which translates to "Heavenly Palace" from Mandarin, is made up of the core module Tianhe and theMengtian and Wentian laboratory modules, which orbit Earth at an altitude ranging between 217 and 280 miles (340 to 450 km).

Tiangong is currently crewed by the three taikonauts of the Shenzhou 23 mission — commander Zhu Yangzhu, pilot Zhang Zhiyuan and payload specialist Lai Ka-ying — who launched to the orbital station atop a 203-ft (62 m) Long March 2F rocket on May 24.

Want to see the Tiangong space station for yourself? Then be sure to read our guide to tracking and photographing the orbital outpost, along with our roundups of the best cameras and lenses for astrophotography.

Editor's Note: If you would like to share your night sky photography with Space.com's readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.

Intel co-founder Gordon Moore observed that processing power doubles every two years whilst almost halving in cost. That should translate to older technology dropping in price and year on year seeing the cheapest prices in the sales, right? The reality is far from simple in the world of skywatching.

For stargazers who have dipped their toes into the world of binoculars and telescopes, prices stack up quickly and even one purchase can wipe out thousands of dollars. Now, there are levels to stargazing equipment, budget models like a Celestron Travel Scope 70 telescope and a pair of Celelestron Cometron 7x50 binoculars will run you between $50-$100 but don't expect the best optical performance. At the complete other end of the scale are premium options like smart telescopes and some image-stabilized binoculars which can run from just under $1,000 all the way to $5,000. There are obviously plenty of in-between models but whichever option you pick, you are still seeing a big chunk of money go out of the bank account when purchasing.

Shopping the sales: Prime Day and Black Friday

Sales events like Prime Day and Black Friday are the usual contenders for getting a good chunk of money off a big purchase. Prices fluctuate throughout the year but I would be inclined to say that the best prices on big purchases have been around Black Friday. Take this Unistellar Odyssey smart telescope, which is 15% off for their Father's Day 2026 sale, it had its last cheapest price on Black Friday 2025.

Does that mean you should wait until then for a guaranteed lowest price? It depends. If you are not in a hurry to get it and are happy to wait, then I would advise you to wait and see if you can get it cheaper. Although waiting for too long just means more time not using the instruments and observing the night sky. You could also fall into the trap of waiting too long and missing out on the best deal available at that time.

Changes to the skywatching industry

Take the Celestron Nexstar 8SE; it's currently $200 off, but this is a frequent reduction for this product. Its last cheapest Amazon price was in October 2025 with $300 off but that is a far sight from its cheapest ever Amazon price of $882. If you had kept waiting after seeing this saving, thinking it might get cheaper, you would have missed out on getting it at over $800 off its current full retail price. Bear in mind, this was in Dec. 2019 and a lot has happened since then. Demand for skywatching optics exploded during the COVID-19 pandemic, with people staying at home more and looking for outdoor hobbies. Pair this with rising US-China trade tariffs and general inflation and you have conditions for a huge price increase on these kinds of products. There was also a huge $32 million class action settlement reached in 2025, resulting from a legal battle involving major telescope manufacturers and brands following allegations of price fixing and artificially inflated costs.

Development and deployment of new technology can lead to high prices for the newest and most advanced models but it also makes obsolete or older technology much cheaper. The latest wave of fully smart telescopes are incredibly expensive because they represent the latest skywatching technology; they can automatically find objects (nothing new there) but they can also autofocus and image them straight from a smartphone, so you can get warm and toasty inside with a warm beverage if you so desire.

Their release has also driven down the prices of models with older GoTo technology and Wi-Fi-controlled mounts. For an easy comparison: the Celestron NexStar 8SE (2006) represents the first wave with GoTo technology and computerization, the NexStar Evolution 8 (2014) represents the second wave with Wi-Fi integration and the Celestron Origin Intelligent Obsevatory II (2026) represents the third wave, with full smart capabilities.

Binoculars: The new Frontier

Binocular manufacturers are also working with new technologies but more often than not, the best improvements are made in the quality of optics, resulting in cleaner and brighter images. Image-stabilized (IS) models have been getting releases since the 90s, with the consumer wave of electronic stabilization being kicked off by Canon with the release of their 12x36 IS model in 1997. This and their other IS models have been receiving minor upgrades to their functionality and optics, like the latest version of the Canon 18x50 IS binoculars, which feature super-spectra coatings, higher precision manufacturing and eco-glass optics.

In the years since, we have seen other companies hone this technology, make housing smaller, improve optical elements and develop smoother stabilization mechanisms. The 2025 release of Fujifilm's Fujinon Techno-Stabi 1640 image-stabilized binoculars represent brand beating stabilization and high optical quality, which makes them one of the best pairs of binoculars I have ever used. For the 2026 summer sales events, they are currently at their lowest ever price at Walmart.

The handheld optics world is entering a new wave of advancements with the advent of smart binoculars that can identify stars and animals directly through the eyepieces. The upcoming Unistellar Envision smart binoculars use an augmented reality (AR) overlay to identify night sky objects, locate trails and identify landscape features. Their pre-order price was $999, with their release retail price expected to be $1499, so sometimes it can benefit you to invest early with innovative technologies.

The Final Say

Is it worth buying now and risking the price dropping more in later years or waiting for a lower price, only to find that it never comes? Unless you have serious insider knowledge, it depends on what your personal circumstances and budget are right now. If you are going on holiday to a dark sky spot soon and have a once-in-a-lifetime opportunity for amazing stargazing or an event like a solar or lunar eclipse, you might be happier to sacrifice more money for that experience. If you are just casually interested in getting something but aren't super intent on needing it right now, then waiting could be better.

If you have a huge budget and need stargazing optics quickly, you may not be bothered by a potential price leeway and would benefit from just getting the instrument at a good price but not its best one. If you are a beginner with a low budget who is just getting into skywatching, it can definitely pay off to wait for the best ever price, at least at a yearly low, so that you can save money which might go towards a more advanced piece of equipment in the future.

There are heaps of streaming services available, and if you're anything like us, you'll have subscriptions to several — Apple TV for Severance, Disney+ for Avatar, Hulu for Solar Opposites, and more. What you need is something where you can access them all in one place, on any device, whether you're home or away.

This is where the Amazon Fire TV Stick 4K Plus comes in. If you have a device with an HDMI port, you can plug in this USB-esque device and log in to your favorite streamers with the supplied remote. No separate power source is required (unlike the Roku Ultra).

Sure, the user interface isn't as clean as we'd like, and is quite ad-heavy, but if you can bear with it, it's a small price to pay for such a nifty device that will become your new favorite entertainment-providing travel companion.

• We've got you covered with reviews and rankings of the best telescopes, binoculars, star projectors, cameras, drones, Lego, streaming and more.

There are several versions of the Amazon Fire TV Stick, so be sure to choose the one that suits you (especially when there's so little price difference between them at the moment).

The main difference between this model, the 4K Plus, and the 4K Max, currently selling for $34.99, is that the latter offers 'Fire TV Ambient Experience,' which transforms your TV into an Alexa-powered smart display. Display your own photos, widgets like weather, calendars, stick notes and more.

Key features: 4K Ultra HD streaming, Dolby Atmos audio, Alexa Voice Remote, 8GB storage

Product launched: 2026

Price history: The Amazon Fire TV Stick 4K Plus usually retails for around $50, but because it's Amazon's own product, it's regularly discounted, especially during events like Prime Day and Black Friday. If you don't have the cash in the bank right now, we're sure the price will dip again during the next big Amazon Sale.

Price comparison: Amazon: $24.99

Reviews consensus: The Fire TV Stick 4K Plus has earned 4.6 out of 5 stars from more than 110,000 reviews on Amazon - seriously impressive. Users praise its ease of use, reliability, picture quality, value for money and speed. The remote control has mixed reviews, with this seemingly retracting from its otherwise glowing reviews. It's worth noting that the remote can be purchased separately if you ever need a replacement. Remember, the Fire TV Stick has voice control too.

✅ Buy it if: You want a portable means of streaming all of your favorite shows from one cable-free device. Take it on vacation to your hotel, buy one for the guest bedroom, or simply keep it plugged into your TV at home.

❌ Don't buy it if: You don't have a device with an HDMI port (e.g., a MacBook Air) and don't want to have to use an adapter.

Check out our other guides to the best telescopes, binoculars, cameras, star projectors, drones, lego and much more.

The most beautiful of all the zodiacal constellations is now visible, low toward the south-southeast as darkness falls. This is Scorpius the Scorpion. It really does look like a scorpion, one of the few star patterns that readily suggests the mythical form assigned to it by the ancients. Composed of several fairly bright stars, its body is formed by the upper stars of this star pattern; its tail slants toward the horizon, then curves to the left and upward, a fine stream of stars ending in a close pair of stars marking its stinger.

George Lovi (1939-1993), a well-known astronomy lecturer and author, used to say that it always bothered him that a striking star pattern such as Scorpius was made to represent
"...a lowly, creepy-crawly thing that has few friends."

In his book, The Stars in Our Heaven, author Peter Lum (1911-1983) provides a perspective like Mr. Lovi's:

"The scorpion . . . is an odd-shaped, insignificant creature, but its sting is out of proportion to its size and, although seldom fatal, is extremely painful; hence it is usually disliked, feared and avoided by anyone who has ever come in contact with him."

Just as Orion is the most striking winter stellar pattern, such a distinction can be claimed for Scorpius for the summer season. Interestingly, one legend has Scorpius representing the creature that stung Orion to death. To honor Orion, the Scorpion was placed opposite him in the sky, so that these celestial antagonists will never meet again. Indeed, when Orion disappears below the western horizon during spring evenings, the Scorpion is poking his head up in the southeast. In addition, they were commonly thought of in opposition to each other: Orion was the constellation of life, Scorpius that of death.

And yet, the whole figure of the scorpion is a magnificent sight — sort of a "celestial fishhook" — and is best appreciated now in a dark sky without any interference from bright moonlight. It really looks like a huge scorpion, with its long stinging tail curled over its back. Two closely spaced stars known as Shaula and Lesath mark the Scorpion's stinger. Astronomy popularizer Hans A. Rey (1898-1977) christened these stars the "Cat's Eyes," noting, "You will find the name quite fitting."

Best seen from southern locales

Scorpius is a constellation that can be best appreciated by southerners. Those who live in the far-northern United States, southern Canada or the British Isles will have part or even all of its tail hidden below the southern horizon. Thus, it is well worth seeking out a good, clear horizon to appreciate this majestic figure. As one progresses farther south, the Scorpion slowly climbs the southern sky. Those who live in Australia, New Zealand, South Africa, northern Argentina, Uruguay, most of Brazil, northern Chile, and southern Peru see Scorpius high overhead. The Milky Way passes through the lower extremities of the Scorpion. Here, clouds of stars and dark interstellar dust combine in a bewildering array as seen in binoculars and telescopes.

Ruddy contender to Mars

The Scorpion's brightest star is the first magnitude Antares, displaying a reddish hue. Antares appears due south at 10:30 p.m. local daylight time on Independence Day; a month later, you'll find it there two hours earlier as darkness falls. To the ancients, its distinctive red color suggested the planet Mars and the name Antares means literally "The Rival of Ares," Ares being the Greek name for the God of War. There was good reason for this, for unlike the fixed stars, the planets could wander against the starry background, and this ability to move had a magical, god-like quality.

Evidence of this lies in the very names of the planets, which represented ancient deities, and of the five bright planets, the one whose color appeared to come closest to that of blood was called Mars in honor of the god of war. But although often referred to as the "red planet," in the sky, it really appears more yellowish orange, fiery, or pumpkin-hued as opposed to red.

In contrast, Antares is one of the reddest stars in the sky. On those occasions when Mars passes just north of Antares, it is obvious which one is redder. So even when Mars is near opposition and appears to glow many times brighter, Antares still rivals it at least in color.

A star of many names

In the time of Confucius, the Chinese called this star Ta Who, "The Great Fire," at the heart of the Dragon of the East. Another Chinese legend refers to Antares and its two attendants — two fainter stars that flank it — as the Ming T'ang, the "Hall of Light" or the "Emperor's Council Hall." Those two stars are about equally bright — Sigma Scorpii (+2.8) and Tau Scorpii (+2.9). They are sometimes called the Praecordia — "the outworks of the heart," the heart of course being Antares.

The Romans called this mighty star Cor Scorpionis, meaning "heart of the scorpion," a title the French also use — Le Coeur de Scorpion. Some 5,000 years ago, the Persians thought of Antares as one of the four Royal Stars, a guardian of heaven.

Enormous celestial beacon

Antares is a cool, red supergiant star, about 550 light-years away. It is some 76,000 times more luminous and about 680 times the diameter of our sun. It's an irregular variable star, meaning that it expands and contracts in an unpredictable manner, causing its brightness to fluctuate. It has been observed to shine as brightly as magnitude +0.9, while at other times, its brightness has been down to +1.2. It usually ranks as the 15th on the list of the twenty-one brightest stars in the sky.

If our solar system were centered on Antares, the orbit of the Earth would easily fit within this star. Yet, despite these impressive statistics, it should be noted that the overall mass of Antares is only 13 to 16 times that of the sun, so it is not very dense. Its insides might be like a very hot vacuum.

Antares is also relatively cool as stars go, only about 6,100º F (3,400 ºC), compared to 11,000º F (6,000 ºC) for the sun. Its low temperature accounts for its ruddy color. It has a small, very hot companion, bluish white in color, yet has been described as appearing
as ". . . a little spark of glittering emerald" because of its proximity and contrast to ruddy Antares. The pair orbit each other over a span of nearly 900 years, separated by a distance of about 500 times Earth's distance from the sun.

Caught in the claws

Scorpions have two large claws in front, but this one seems to have had its claws clipped; they were cut off to form the constellation of Libra the Scales, one of the constellations of the zodiac and associated with Themis, the Greek goddess of justice, whose attribute was a pair of scales. These stars still both carry Arabic names: Zubeneschamali ("northern claw") and Zubenelgenubi ("southern claw"), to help distinguish them as originally belonging to Scorpius.

Lastly, it must be emphasized to those newcomers to astronomy that the currently accepted name of this constellation is Scorpius, not Scorpio. Principally, astrologers (and some older astronomy books) use the latter for labeling the zodiacal sign of that name.

Just stingin' the nomenclature.

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope, The Old Farmer's Almanac and other publications.

A giant asteroid roughly the size of a skyscraper will pass within seven lunar distances of Earth on June 27. Here's how to watch the rare flyby during two livestreams on June 26 and June 27.

How can I watch the flyby online?

The Virtual Telescope Project will host two YouTube livestreams starting at 7 p.m. EDT (2300 GMT) on June 26 and 27, before and after asteroid 1997 NC1's closest approach to Earth. Each event will feature live views of the asteroid captured by a suite of robotic telescopes in Manciano, Italy, weather permitting.

"While this encounter is absolutely no cause for concern, it will be a very important and interesting opportunity," Virtual Telescope Project founder Gianluca Masi said in a press release sent to Space.com. "An asteroid of this size comes this close roughly once every ten years, becoming bright enough to be easily visible through small telescopes while it crosses the starry sky."

The asteroid designated 152637 1997 NC1 will make its closest approach to Earth at 7:16 a.m. EDT (1116 GMT) on June 27, when it will pass 1,594,339 miles (2,565,839 kilometers) from our planet, whipping by at 19,879 mph (31,992 km/h), according to NASA.

With an estimated diameter of 1,443 feet (440 meters), 1997 NC1's size and potential to pass close to Earth during future orbits have led to it being designated as a potentially hazardous asteroid by NASA. However, it will pose zero risk to our planet, or the moon during this week's flyby.

How can I see 1997 NC1 with my own telescope?

A pair of 10x50 binoculars or a small 4-inch telescope should be enough to reveal the asteroid as a point of light shifting through the stars of the constellation Ophiuchus on the night of the close approach, according to Masi.

1997 NC1 will reach a peak brightness, or magnitude of +10 at 8 p.m. EDT on June 27 (0000 GMT on June 28), marking an ideal time to observe the wandering asteroid. Magnitude is the scale used by astronomers to measure the apparent brightness of an object in the night sky. The lower the number, the brighter the object!

The streams will occur shortly before World Asteroid Day — an annual United Nations-backed event held on June 30 to raise awareness of the threat posed by potential asteroid strikes. The date was chosen to coincide with the anniversary of the Tunguska impact of 1908, when an asteroid exploded over Siberia, flattening millions of trees in an 830 square mile (2,148 sq km) area.

Full moons are overrated and, frankly, a pain. They wash out the stars, ruin deep-sky observing, and they all look the same. Technically, all of that is true. Yet every month — and particularly each June — I find myself standing outside at dusk waiting for the full moon to rise like it's an old friend arriving for an annual visit.

The main attraction of June's Strawberry Moon is that it stays so low, as seen from the Northern Hemisphere. It appears at an extreme southeasterly point on the horizon and rises slowly, almost reluctant to leave the horizon. It doesn't climb sharply upward like a winter full moon. Instead, it drifts sideways through the southern sky, hanging low and heavy in warm evening haze. People who never normally notice the moon suddenly stop and stare — the surefire way of telling that a celestial event has crossed the threshold and become simply an event.

Last year's Strawberry Moon rose absurdly low because it was at a major lunar standstill, the peak of an 18.6-year cycle that changes how extreme the moon's rising and setting positions become. It reached its most southerly moonrise point since 2006, and we won't see another stretch quite like that again until the 2040s. I was at an outdoor concert at the time, and spent much of the set looking in the complete opposite direction from the stage. It just looked so odd rising behind my city in a position I had never seen it rise before. It was like being in an alternate reality. Few around me even noticed.

It won't rise quite as far in the southeast this year, but June's low-hanging moon always feels bigger emotionally, even when you know the moon illusion is mostly a trick of human perception.

What's happening and when to look

You don't need to understand lunar cycles and celestial mechanics to appreciate the Strawberry Moon. You just need clear southeastern and then southern sightlines to watch it hug the horizon. However, I'm going to explain it anyway. The moon doesn't repeat the same apparent path through the sky every month. Its orbit is tilted about five degrees relative to the ecliptic — the apparent path of the sun through the sky — and those tilts combine and shift to create a cycle that repeats every 18.6 years.

Moreover, the full moon always sits opposite the sun in the sky. In June, the sun takes its highest and northernmost path of the year in the Northern Hemisphere. That's why it's summer — the sun is higher, so days last longer and there's more sunlight. The Strawberry Moon does the reverse: it follows the lowest and most southerly path possible. It rises late, well south of due east, follows a shallow arc across the sky and sets early, well south of due west, just like the sun in winter.

Southern Hemisphere observers get the opposite experience. June marks the beginning of winter there, so the Strawberry Moon rises much higher in the sky and appears more northerly. While Northern Hemisphere observers experience the famous "low-hanging fruit" effect, southern observers see a higher, more elevated full moon that remains visible for longer into the night.

That reversal is one of my favorite things to explain to beginners because it instantly makes the sky feel global rather than local.

How and when I'm watching it

The best way to experience the Strawberry Moon is to treat it less as an astronomical event and more as a landscape photograph. The moon itself changes surprisingly quickly during its rise. Scouting a location is important for the Strawberry Moon because it rises at its most extreme point. You need a clean southeastern horizon — a beach, an open field, a hilltop or even a long, straight road. Trees and buildings near the horizon matter. You can take a lot of the guesswork out by using Photo Ephemeris to show you exactly where the moon will rise from any location on Earth. That's important because it likely won't rise where you expect it to.

The sweet spot is during dusk, right around local moonrise time on June 29. That's when the moon still shares the sky with fading blue twilight, a far more dramatic sight than when it rises before or long after sunset.

And this is important: the orange color does not last long. People often assume the moon stays amber all night. It doesn't. The color comes largely from Earth's atmosphere scattering shorter wavelengths while the moon sits low on the horizon. As it climbs higher, it quickly returns to its ordinary bright white. You've got maybe 20 or 30 minutes of peak "Strawberry Moon mood" before physics quietly resets everything.

Stargazer's corner: June 26-July 2, 2026

As June draws to a close, the moon grows toward full, reaching its Strawberry Moon phase on Monday, June 29. In the nights leading up to it, moonlight increasingly dominates the evening sky, while after it, it rises a little later. Look low in the south after dark on Saturday, June 27, to see a near-full moon close to Antares in the constellation Scorpius. It will take a very early start, but in the northeast before dawn during the last days of June and into early July, Mars will hang below the Pleiades open cluster (M45), with Uranus nearby.

Constellation of the week: Aquila

Aquila — Latin for eagle — is anchored by Altair, a bright star that sits lower in the southern sky than Vega and Deneb, the other two stars in the famous Summer Triangle asterism now rising in the east after dark. What makes it easy to recognize is the straight line formed by bright Altair and orangey Tarazed.

I always think we should appreciate Altair more — at 17 light-years away, it's one of the closest stars to the sun we can easily see. It's also pretty weird, rotating every 12 hours (the sun takes 27 days) and bulging violently at its equator. Altair will become more prominent as summer progresses, so there's plenty of time to get to know it.

Canon is rightly regarded as one of the premier manufacturers of cameras and optical equipment, and the Canon EOS R5 is a reminder of why. Labelled 'a camera of epic proportions' by our reviewer Jacob Little, it's an astonishing $699 off for Prime Day.

Buy this Canon EOS R5 body from Amazon for $2599.

Couple this 45 megapixel Canon EOS R5 body with one of the best lenses for astrophotography and you'll be stunned by its image quality, as our expert was in their Canon EOS R5 review, where they awarded it 4.5/5 stars. It's ideal for astrophotography, but its super-accurate tracking (including eye, face and head detection) means it's also excellent for nature watching and weddings. It's overkill for newcomers but if you're a pro or semi-pro photography you won't regret purchasing this powerhouse of a camera.

• Check out our Amazon Prime Day hub, where we bring you the best deals of Prime Day 2026, including early Prime Day deals.
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Looking to level up your photography to the point where you can profit from it? Then the Canon EOS R5 is for you, especially now it's reduced for Prime Day. It may have been superseded by the R5 Mark II but this is still a top-tier camera, suitable for pros or would-be pros.

In our review of the Canon EOS R5, our expert remarked that "It might be the most complete camera Canon has ever produced". Not only is it excellent for astrophotography, bringing out the detail in low light conditions, its autofocus and image stabilization is particularly impressive, making it a gift for nature-watchers or event photographers.

It captures images at up to 45 megapixels, and can also save them in RAW format. It likewise captures video in 8K, saving both to or CFexpress or SD. We'd recommend you use RAW when shooting astrophotography to maximize your editing abilities and take advantage of this camera's "superlative resolution and image quality".

Key features: 45MP sensor, 8K video, 100 to 51,200 (expanded 50 to 102,400) ISO range, 5-axis stabilization, excellent tracking.

Product launched: July 2020

Price history: We've seen the Canon EOS R5 drop to this price briefly in February, but it's never been cheaper. Walmart and Best Buy have matched this price if Amazon runs out of stock.

Price comparison: Amazon: $2599 | Walmart: $2599 | Best Buy: $2599

Reviews consensus: In our Canon EOS R5 camera review, our expert called it "A very impressive piece of kit," praising its autofocus and stabilization, leading to some superb quality images. They were also impressed with how well it handled. The camera's Amazon reviews are just as positive, the only real criticism being its price, which this Prime Day deal addresses.

Space: ★★★★½ | LiveScience: ★★★★½

✅ Buy it if: You want the performance of a once pro-level camera but without the price tag.

❌ Don't buy it if: You have little astrophotography experience; for newcomers, this is overkill.