Comparing Carbon Dioxide Distributions on Ganymede and Callisto

Details Comparing Carbon Dioxide Distributions on Ganymede and Callisto Comparing Carbon Dioxide Distributions on Ganymede and Callisto

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1263h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1263

Physics

2

Scientific paper

CO2 is found in the optical surfaces of Ganymede and Callisto. The CO2
is likely hosted in the non-ice materials and is endogenic. Low-energy
particles in the magnetosphere alters the surface, increasing the CO2 on
the trailing side of Callisto.

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