As 2004 draws to a close,
skywatchers have yet another opportunity to view a naked-eye comet. Comet Machholz
has been brightening steadily and conditions are now prime.
So far this year, there
have been four comets that have managed to attain naked-eye visibility. Last
spring, comets Bradfield (C/2004 F4), NEAT (C/2001 Q4), and LINEAR (C/2002 T7)
all reached third magnitude, while in July another comet discovered by the automated
LINEAR project (C/2003 K4) briefly peaked at sixth magnitude.
On the astronomers'
magnitude scale, smaller numbers denote brighter objects. The dimmest objects
visible under perfectly dark skies are about magnitude 6.5.
Discovered on Aug. 27 by
veteran comet hunter Donald E. Machholz of Colfax, California, comet Machholz
(C/2004 Q2) has been brightening steadily during the past several months while
approaching both the Sun and Earth.
Getting brighter
This comet currently is
glowing at around magnitude 3.5 and is visible to the naked eye in dark, non-light
polluted skies, though much better seen in binoculars or telescopes. This kind
of brightness makes Machholz a very fine comet from the viewpoint of a serious
amateur astronomer, but it doesn't appear that this comet will become the kind
of spectacle that Comet Hale-Bopp was in grabbing the broader public's attention.
Yet this is an auspicious
circumstance, as Machholz is now the fifth naked eye comet in 2004. Twice before,
in 1911 and again in 1970, four comets managed to reach naked-eye brightness
within a single calendar year.
But when Andrew Pearce of
Noble Falls, Western Australia saw the comet without any optical aid on Nov.
19, it put 2004 into the books as a record year for naked-eye comets.
At this moment the comet's
motion across the sky is toward the north, making it increasingly well placed
for Northern Hemisphere observers. During January, according to calculations
made by Brian Marsden of the Smithsonian Observatory in Cambridge, Massachusetts,
the comet will move north of the celestial equator, tracking from southern Taurus
on up into the constellation Perseus.
From a brightness standpoint,
the comet has also been performing excellently; in fact, running nearly twice
as bright as predictions had originally suggested.
Observers who have looked
for the comet during the late evening hours could readily see its bright, bluish-white
head surrounded by a fuzzy cloud of dust and gas called the coma.
Happy comet campers
A couple of weeks ago, Mike
Begbie, observing from Harare, Zimbabwe with 15x60 binoculars, said, "The
comet is becoming spectacular. The coma is highly condensed and the dust tail
is broad and prominent."
"I couldn't take my
binoculars off the comet!" exclaims Brian Summers, a magazine editor from
Katonah, New York. "It was an 'instant pickup' - just point the binoculars
and there it was!"
"Machholz's comet very
much reminds me of Comet Kobayashi-Berger-Millon," said Long Island, New
York amateur, Sam Storch. "I remember that comet from the summer of 1975
and like Machholz, it passed relatively near to the Earth and also displayed
a very condensed nucleus and a large coma."
John E. Bortle, a well-known
comet observer from Stormville, New York, describes Comet Machholz as "a
strange looking beast; its tails are relatively weak, but the separation (lag-angle)
between the classic ion tail and the "thing" that passes for a dust tail, is
huge (more than 90 degrees!)."
Bortle believes "the
comet will continue to be a very nice sight in January when we can view it high
in the evening sky."
During mid-December, the
comet's coma appeared ½ degrees across (equal to the apparent
size of the full Moon). That size translated into an actual diameter of 384,000
miles and with Machholz continuing to approach both the Sun and Earth in the
coming days, the coma's size can only continue to grow larger.
Comet Machholz will be closest
to Earth on the night of Jan. 5-6, 2005, when it will be 32,256,000 miles away.
On the evening of Jan. 7,
it will conveniently pass just a couple of degrees to the west of the famous
Pleiades star cluster, making for a pretty sight in binoculars [Map].
The comet will probably be cresting at its brightest right around this time,
perhaps peaking at around magnitude +3.3, which would make it equal in brightness
to Megrez, the star that joins the handle with the bowl of the Big Dipper.
"I have been most impressed
with recent views of comet Machholz from Palm Springs, California," writes
Robert Victor, an astronomer who served for many years at the Abrams Planetarium
of Michigan State University. "I am looking forward to its passage near
the Pleiades in early January."
From the discoverer
"It has been a pleasure
for me to watch this comet grow and develop," Don Machholz told SPACE.com. "I
have also had a few months to plan for the time when the comet reaches
this point. As a result of having a bit of lead time, I wrote a PowerPoint
talk, giving it at local astronomy (and other) clubs during the last
couple of months.
"In recent weeks, while
the comet has been rising during the mid-evening hours, I've been inviting friends
and neighbors to my house for 'private' viewing of the comet," Machholz said. "Other
local astronomers and I will be holding a series of public star parties at various
locations in the foothills, showing the comet and Saturn and other stuff to
the public. We've been doing public star parties for years, but I believe
this is the first time we've been able to show a Comet Machholz."
A schedule of upcoming talks
by Don Machholz can be found here.
January and beyond
Continuing northward, the
comet will slip less 2 degrees to the east of the famous variable star, Algol
in Perseus on the night of Jan. 16-17. The comet will reach perihelion at around
22 hours G.M.T./5:00 p.m. EST on Jan. 24, when it will be 112,019,920 miles
from the Sun.

The position of comet Machholz at 9 p.m. local time from mid-northern latitudes
on various nights as it climbed higher into the sky during December. Click
to Enlarge |
Since the comet will be
more-or-less opposite the Sun all during this "flyby," it should easily be visible
in a dark sky.
Then during February, March
and April, Comet Machholz will become circumpolar from mid-northern latitudes.
Or in other words, during this time frame it will always remain above the horizon,
appear to neither rise nor set. During the second week of March, it will pass
within half-dozen degrees of Polaris, the North Star.
Our latest "guesstimates"
Machholz's brightness in the coming weeks, is for it to gradually dim to about
fourth magnitude by the end of January and to around fifth magnitude by the
third week of February. Those blessed with very dark skies might even be able
to continue following the comet with just their unaided eyes until about the
middle of March. Of course, the comet could always dim much more rapidly . .
. or, conversely, a sudden unexpected flare-up could also occur as well.
But these are extreme cases.
So far, the comet has performed very well and there is no reason not to believe
that it will continue to delight Northern Hemisphere observers for at least
several more weeks.
Once again, we should stress
that the darker your observing site, the better the comet will appear. With
the bright Moon pretty much out of the way during the first half of January,
prospective comet observers are likely to have their greatest success.
After comet Machholz whirls
around the Sun on Jan. 24, it will head far out into space. Traveling in a highly
elongated orbit, taking it far beyond the known limits of our solar system,
it could again return to the vicinity of the Earth and Sun about 119,000 years
from now.
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Joe Rao
serves as an instructor and guest lecturer at New York's Hayden Planetarium.
He writes about astronomy for The New York Times and other publications, and
he is also an on-camera meteorologist for News
12 Westchester, New York.
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DEFINITIONS
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Degrees
measure apparent sizes of objects or distances in the sky, as seen from
our vantage point. The Moon is one-half degree in width. The width of
your fist held at arm's length is about 10 degrees.
1 AU, or
astronomical unit, is the distance from the Sun to Earth, or about 93
million miles.
Magnitude
is the standard by which astronomers measure the apparent brightness
of objects that appear in the sky. The lower the number, the brighter
the object. The brightest stars in the sky are categorized as zero or
first magnitude. Negative magnitudes are reserved for the most brilliant
objects: the brightest star is Sirius (-1.4); the full Moon is -12.7;
the Sun is -26.7. The faintest stars visible under dark skies are around
+6.
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