PIA17833: NEOWISE Spies Comet C/2013 A1 Siding Spring


NEOWISE Spies Comet C/2013 A1 Siding Spring

Caption:

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Figure 1
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NASA's NEOWISE mission captured images of comet C/2013 A1 Siding Spring, which is slated to make a close pass by Mars on Oct. 19, 2014. The infrared pictures reveal a comet that is active and very dusty even though it was about 355 million miles (571 million kilometers) away from the sun on Jan. 16, 2014, when this picture was taken.

The infrared measurements will allow astronomers to determine the sizes and quantity of dust particles being flung off the comet. The measurements will also give engineers some indications of what orbiting spacecraft at Mars might expect when the comet gets close. Preliminary analysis of the data indicate approximately 220 pounds (100 kilograms) of dust are being ejected from the comet's surface each second, assuming the grains are dark and nearly the density of water-ice. The comet's activity is expected to increase as it gets closer to Mars.

Background Info:

JPL manages NEOWISE for NASA's Science Mission Directorate at the agency's headquarters in Washington. The Space Dynamics Laboratory in Logan, Utah, built the science instrument. Ball Aerospace & Technologies Corp. of Boulder, Colo., built the spacecraft. 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 and http://www.jpl.nasa.gov/wise .

Cataloging Keywords:

Name Value Additional Values
Target C/2013 A1 (Siding Spring)
System
Target Type Comet
Mission Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE)
Instrument Host NEOWISE
Host Type Space Telescope
Instrument NEOWISE Telescope
Detector
Extra Keywords Color, Dust, Infrared, Water
Acquisition Date
Release Date 2014-01-28
Date in Caption 2014-01-16 2014-10-19
Image Credit NASA/JPL-Caltech
Source photojournal.jpl.nasa.gov/catalog/PIA17833
Identifier PIA17833