PIA16211: Trojan Colors Revealed (Artist's Concept)
 Mission:  Wide-field Infrared Survey Explorer (WISE)
 Instrument:  WISE Telescope
 Product Size:  3000 x 2400 pixels (w x h)
 Produced By:  IPAC-Caltech
 Full-Res TIFF:  PIA16211.tif (21.61 MB)
 Full-Res JPEG:  PIA16211.jpg (818.6 kB)

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Original Caption Released with Image:

New results from NASA's Wide-field Infrared Explorer, or WISE, reveal that the Jovian Trojans -- asteroids that lap the sun in the same orbit as Jupiter -- are uniformly dark with a hint of burgundy color, and have matte surfaces that reflect little sunlight. The results are illustrated in this artist's concept, showing both the leading and trailing packs of Trojans in orbit with Jupiter. Observations from WISE also confirmed the previous suspicion that there are more asteroids in the leading pack of Trojans (seen in the distance) than the trailing bunch.

The results are helping astronomers fill in missing pieces of the ongoing Jupiter Trojan puzzle: how and when did these asteroids form?

The data for this research come from the asteroid-hunting portion of the WISE survey, called NEOWISE.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages, and operated WISE for NASA's Science Mission Directorate. The spacecraft was put into hibernation mode after it scanned the entire sky twice, completing its main objectives. Edward Wright is the principal investigator and is at UCLA. The mission was selected competitively under NASA's Explorers Program managed by the agency's Goddard Space Flight Center in Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory in Logan, Utah. The spacecraft was built by Ball Aerospace & Technologies Corp. in Boulder, Colo. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA.

More information is online at http://www.nasa.gov/wise and http://wise.astro.ucla.edu.

Image Credit:
NASA/JPL-Caltech

Image Addition Date:
2012-10-15