PIA13457: Comets WISE -- A Family Portrait
 Target Name:  Comet
 Mission:  Wide-field Infrared Survey Explorer (WISE)
 Instrument:  WISE Telescope
 Product Size:  3754 x 3004 pixels (w x h)
 Produced By:  IPAC-Caltech
JPL News Release 2011-031
 Full-Res TIFF:  PIA13457.tif (33.83 MB)
 Full-Res JPEG:  PIA13457.jpg (1.278 MB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

During its one-year mission, NASA's Wide-field Infrared Survey Explorer, or WISE, mapped the entire sky in infrared light. Among the multitudes of astronomical bodies that have been discovered by the NEOWISE portion of the WISE mission are 20 comets.

This collage shows those 20 new comets all together in a kind of family portrait. Most of the comets are named WISE. In three cases, the comet does not bear the name WISE because the object was known before to be an asteroid. The WISE observations revealed their true nature. These objects did not turn out to be stony and/or metallic space rocks as is the case for asteroids. Instead, they were shown to be comets -- snowy dust balls with clouds of dust and gas surrounding them.

When most people think of comets, they think of the popular images of Halley's Comet or Comet Hale-Bopp, with bright, enormous tails. A comet tail forms as the object travels closer to the sun. The ices in the comet are heated and become a gas, escaping the surface of the comet and lifting dust particles away as well. This fuzzy cloud around the comet nucleus is called a coma. As a comet gets closer and closer to the sun, the solar wind and sunlight push the coma away, forming the long tail.

Comets are named by the International Astronomical Union's Minor Planet Center, and the names indicate the circumstances of discovery. The designations of the comets in the collage, from left to right, top to bottom are: 237P/LINEAR (2002 LN13), 233P/La Sagra (2009 WJ50), P/2009 WX51 (Catalina), P/2010 B2 (WISE), P/2010 D1 (WISE), P/2010 D2 (WISE), C/2010 D3 (WISE), C/2010 D4 (WISE), C/2010 DG56 (WISE), C/2010 E3 (WISE), C/2010 FB87 (WISE-Garradd), C/2010 G3 (WISE), C/2010 J4 (WISE), P/2010 K2 (WISE), C/2010 KW7 (WISE), 245P/WISE (2010 L1), C/2010 L4 (WISE), C/2010 L5 (WISE), P/2010 N1 (WISE), and P/2010 P4 (WISE).

The fuzzy background in each picture is due to random fluctuations in infrared light, primarily from dust in our own solar system. Stars cannot be seen because they are subtracted out during the process of combining multiple WISE pictures together to make this view centered on the moving comets.

The colors in the pictures are representational. Infrared light of 4.6, 12 and 22 microns is colored blue, green and red, respectively. The light emitted from comets in infrared is due to their temperatures, so the cooler objects appear to have more red, while warmer objects will appear more bluish.

Image Credit:

Image Addition Date: