How to see the moon and Comet Pan-STARRS tonight
Comet Pan-STARRS and the moon should be visible for about half an hour before they disappear into the haze located near the horizon.
Tue, Mar 12, 2013 at 10:00 AM
Astrophotographer Adam Block of the Mt. Lemmon SkyCenter took this photo of Comet Pan-STARRS (C/2011 L4) on March 10 over Tucson, Ariz. (Photo: Adam Block)
Many stargazers attempting to view the Comet Pan-STARRS on recent nights have been thwarted by the comet's low position in the western sky. But tonight (March 12), the thin crescent moon will lend a hand.
Over the past weekend countless observers across in North America and Europe tried — and for the most part failed — to see Comet Pan-STARRS, in part due to its low altitude above the west-northwest horizon. The bright glare of the evening twilight sky is also a hurdle, since it can make the comet harder to see just after sunset.
But fret not, comet lovers! Weather permitting, observing conditions will improve by this evening, since Comet Pan-STARR's position above the horizon will be noticeably higher and the moon can be used as a benchmark to point your way.
Clear western view essential
The best suggestion I can make for your Tuesday night comet watch is to first find an observation site with the least amount of obstructions in the western part of the sky. [How to see the comet]
If you end up successfully catching a glimpse of them, the moon and the comet will not be any higher than 10 degrees above the horizon. (That is about the size of your clenched fist, held out at arm's length.)
If you have a house or some trees in your line of sight, then you're going to have to find another viewing site.
Step 1: Find the moon
In order to boost your chances of seeing Comet Pan-STARRS, be sure to arrive at your viewing site in time to see the sunset. Take note of where on the horizon the sun sets.
Now wait about 30 minutes as the sky slowly begins to darken. It will still be rather bright looking toward the west a half hour after the sunset … this was one of the main problems people have had in recent days in trying to see the comet.
But first things first: Let's locate the moon. Take your clenched fist and measure off 10 degrees up from that point on the horizon where the sun disappeared about a half hour before. Now look a bit to the right from the top of your fist. That's where the crescent moon will be.
Seeing the moon will be a challenge in itself because it will be very narrow, appearing only about 28 hours after passing its new phase. Because of this, the lunar disk will be only 1 percent illuminated. It will be oriented with its bright sliver down, resembling a cup or a thin smile on the sky.
If you can't see the moon with your unaided eye, then use binoculars. Once you pick it up with binoculars, you should be able to find it without optical aid.
The progression of comet Pan-STARRS across the night sky in March 2013 is shown in this NASA graphic. (Image: Science@NASA)
Finding Comet Pan-STARRS
With the moon found in the evening sky, it is time to use it as a guide to spot Comet Pan-STARRS.
The comet will be located about 5 degrees to the left of the moon. Once again, you might not initially see it with your eyes, so use binoculars if you need to. Five degrees measures roughly "half a fist" in length.
You'll know Comet Pan-STARRS when you see it. It will appear as a bright, star-like "head" with a short, stubby tail extending from the head upwards and slightly to the left from the bright end. Like the moon, once you find it with binoculars, you should, with time, be able to make it out against the bright twilight sky.
Comet Pan-STARRS and the moon should be visible for about a half hour before they disappear into the murky haze always located near the horizon.
Not so 'Great Comet'?
Comet Pan-STARRS was discovered in June 2011 by a team of astronomers using the Panoramic Survey Telescope and Rapid Response System (or PAN-STARRS), a telescope in Hawaii. The comet is officially designated as C/2011 L4 (PANSTARRS) and is thought to take more than 100 million years to make a single orbit around the sun. [Comet Pan-STARRS Explained (Infographic)]
Right now the brightness of Comet Pan-STARRS, according to viewers who spotted it in the Southern Hemisphere, ranks at about first-magnitude on the astronomy brightness scale. That is about as bright as the brightest stars.
Normally, a comet as bright as this would be categorized as a "Great Comet," but most observers feel that Pan-STARRS does not fall into this category because it's not visible against a fully dark sky. The bright twilight background is working against making it a prominent, eye-catching sight.
And the comet's dust tail is not breathtakingly long, but short and stubby. To the naked eye, not much of the tail may be visible at all, though in big binoculars or small telescopes, some say that Pan-STARRS is a rather impressive sight.
Comet Pan-STARRS is one of at least three comets in the night sky currently thrilling stargazers. Another comet (the Comet Lemmon) is currently visible to observers in Southern Hemisphere, while the third object is Comet ISON.
Comet ISON is a promising celestial object that was discovered by amateur astronomers in 2012 and is expected to make its closest approach to the sun in late November. The comet will be only 800,000 miles (1.2 million kilometers) from the sun at its closest point, and could put on a dazzling night sky spectacle. But it could also fizzle out, NASA scientists have said.
NASA astronomers and stargazers around the world are regularly tracking Comet ISON, as well as comets Pan-STARRS and Lemmon as they shine in the night sky.
Editor's note: If you snap an amazing photo of Comet Pan-STARRS in the night sky, or any other celestial object, and you'd like to share for a possible story or image gallery, please send images, comments and location information to email@example.com.
Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. Follow us @Spacedotcom, Facebook or Google+.This article was first published on SPACE.com.
Related on SPACE.com and MNN: