Comet C/2013 UQ4 (Catalina) has been observed by NASA’s Near-Earth Object
Wide-field Infrared Survey Explorer (NEOWISE) spacecraft just one day after
passing through its closest approach to the sun.
The comet glows brightly in
infrared wavelengths, with a dust tail streaking more than 62,000 miles (100,000
kilometers) across the sky. Its spectacular activity is driven by the
vaporization of ice that has been preserved from the time of planet formation
4.5 billion years ago.
"The tail forms a faint fan as the smaller dust particles are more easily
pushed away from the sun by the radiation pressure of the sunlight," said James
Bauer, researcher at NASA’s Jet Propulsion Laboratory in Pasadena,
California.
C/2013 UQ4 takes more than 450 years to orbit the sun once and spends most of
its time far away at very low temperatures. Its orbit is also retrograde, which
means that the comet moves around the sun in the opposite direction to the
planets and asteroids.
The comet was originally thought to be an asteroid, as it appeared inactive
when discovered by the Catalina Sky Survey on October 23, 2013. NEOWISE also
observed the comet to be inactive on New Year's Eve, 2013, but since then the
comet has become highly active, allowing astronomers around the world to observe
it. The comet's activity should decline as it once again returns to the cold
recesses of space.
NASA’s Jet Propulsion Laboratory manages the NEOWISE mission for NASA's
Science Mission Directorate in Washington.
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