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Lovely album of photos from WISE
Posted By Emily Lakdawalla
2010/02/17 11:56 CST
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Today the Wide-field Survey Explorer (WISE) team released a small album of beautiful astrophotos, showing a colorful star-forming cloud, an absolutely glorious image of the Andromeda galaxy, a cluster of galaxies, and this one, of comet C/2007 Q3 (Siding Spring):

NASA / JPL / UCLA
Comet Siding Spring in infrared
Comet Siding Spring, also known as C/2007 Q3, was first discovered in 2007 by Australian astronomers when it was near its closest approach to Earth and the Sun at 1.2 and 2.2 AU, respectively. The comet is on a hyperbolic orbit, so will not return again to the neighborhood of the Sun. The Wide-field Infrared Survey Explorer observed it on January 10, 2010, by which time it was far north of the ecliptic plane. WISE views the sky in infrared wavelengths. The comet is 10 times colder than the background stars, so its emission is mostly in longer wavelengths, giving it its red color in this false-color view. (In this image, 3.4-micron light is colored blue; 4.6-micron light is green; 12-micron light is orange; and 22-micron light is red.) Visit the JPL Near Earth Object Program website to see an interactive diagram of C/2007 Q3 (Siding Spring)'s orbit.There was an interesting email from WISE team member Amy Mainzer to the Minor Planets Mailing List a few days ago, talking about why followup of WISE's discoveries is valuable:
As WISE's scans run from ecliptic pole to ecliptic pole, you will see WISE objects spanning a wider range of declinations than is normally covered by ground-based surveys. We realize this may present a challenge to follow up observers, but this sky coverage may reveal new knowledge of the distribution of orbits of solar system objects.The Siding Spring image is just one of several stunners released today; I am particularly enamored of the huge Andromeda Galaxy image, which I think I may have to print out and hang on my wall!You will note that there are now a number of WISE targets on the confirmation page. We encourage you to follow these up as WISE targets have high priority scientifically. The combination of visible light brightness measurements, improved orbit information and the WISE infrared fluxes will enable the determination of accurate diameters, albedos, surface properties, thermal forces, etc. This all requires ground-based follow-up. While most of our targets will be observed via established collaborations, the participation of the broader astronomical community plays a crucial role that has already been demonstrated for a number of WISE discoveries.
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