Antares is a red supergiant star that is nearing the end of its life. Once there is no more fuel left to burn, the star will collapse and explode into a supernova — "at which time its brightness will rival that of the rest of our galaxy put together," noted astrophysicists Paul Butterworth and Mike Arida for NASA's Imagine the Universe!

The star is among the 20 brightest visible in Earth's night sky, although its brightness varies. Amateur observers have pegged its apparent magnitude between 0.88 and 1.16. Additionally, it has a small neighbor star (Antares B) that looks bluish-white and is sometimes called "a little spark of glittering emerald." [The Brightest Stars in the Sky: A Starry Countdown]

In modern rocketry, Antares was the name of the lunar lander on the Apollo 14 moon mission, and it is also the name of a rocket being developed by Orbital Sciences Corp.

Antares, also called alpha Scorpii, is a prominent star in Scorpius (the Scorpion), a constellation that is visible in the southern night sky of most locations in the Northern Hemisphere. Antares is about 604 light-years from Earth. It is 700 times the sun's diameter, large enough to engulf the orbit of Mars, if the solar system were centered on it.

Despite its size, the overall density of Antares is less than one-millionth that of the sun. Antares is also relatively cool as stars go, only about 6,500 degrees Fahrenheit (3,593 degrees Celsius) compared to 10,000 F (5,500 C) for the photosphere of the sun. The star's low temperature accounts for its ruddy color.

Antares' position is:

  • Right ascension: 16 hours 29 minutes 24.4 seconds
  • Declination: -26 degrees 25 minutes 55 seconds

Though they look serene and silent from our vantage on Earth, stars are actually roiling balls of violent plasma. Test your stellar smarts with this quiz.
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Star Quiz: Test Your Stellar Smarts
Though they look serene and silent from our vantage on Earth, stars are actually roiling balls of violent plasma. Test your stellar smarts with this quiz.
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The word "Antares" means "anti-Ares" or "anti-Mars," likely because astronomers in ancient times thought the reddish star looked similar to the red planet. The planet, in fact, can sometimes get close to Antares in the Red Planet's travels across the night sky.

Antares' bright appearance got attention in many older cultures, according to Richard Hinckley Allen's "Star Names and Their Meanings." In Persia around 3000 B.C., it was named one of four royal stars in the sky. In Egypt, Antares was a symbol of the goddess Selkit (who is often referred to as the Scorpion Goddess.)

The star is so bright that it washed out its fainter companion, meaning that Antares B was not discovered until well into the telescopic age. Johann Tobias Bürg, an Austrian astronomer, spotted the fifth-magnitude star on April 13, 1819, when the moon covered Antares.

According to NASA, the star has eaten all its hydrogen and is now shining because it is fusing progressively heavier elements. Time-exposure pictures of the region around Antares reveal an unusually colorful area of gas: yellow, blue and red are all prominent in 2004 pictures from the Royal Observatory in Edinburgh and the Anglo-Australian Observatory.

This is due to a combination of gases whose atoms are excited by starlight, and light shining from Antares A and B, NASA said. Additionally, the area has several other objects crowding the field of view: the nebula (gas cloud) Rho Ophiuchi and M4, a globular cluster (or collection of stars.)

Antares was the inspiration for the name of a rocket now being tested by Orbital Sciences. On April 21, 2013, the private company's rocket launched into space for the first time from Virginia's Mid-Atlantic Regional Spaceport (MARS), which is located at NASA's Wallops Flight Facility.

Antares is often compared to other red supergiants of its type, so that scientists can better understand how these stars are structured and under what conditions they will eventually become supernovas. 

In a 2014 study, published in the journal Astronomy & Astrophysics, a science team looked at the envelope of dust surrounding Antares, comparing images taken by themselves in 2010 and another team in 1998. They could see four dust clumps moving in that short time frame, and a possible new clump forming in 2010 (because that clump wasn't visible in 1998). They did an estimate of the expansion velocity of these dust clouds, and concluded that it is difficult to explain these velocities based on a simple outflow of material from the star; perhaps the dust clouds are randomly ejected. 

A 2017 study that is scheduled for publication in A&A (and available in preprint version on Arxiv) examines convection as a possible mechanism for the mass loss of red supergiants. The team imaged Antares using infrared interferometry, providing the best-ever angular resolution on a star's disk. They interferometer signal suggests the presence of convective cells.