Possible Exogenic and Impact Origins for Carbon Dioxide on the Surface of Callisto

Details Possible Exogenic and Impact Origins for Carbon Dioxide on the Surface of Callisto Possible Exogenic and Impact Origins for Carbon Dioxide on the Surface of Callisto

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1540h&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1540

Physics

Scientific paper

CO2 is ubiquitous on the surface of Callisto. The leading hemisphere:
CO2 is concentrated in ice-rich impact craters. Trailing hemisphere: a
global distribution as a sinusoid centered on the equator at 270o
longitude suggests effects from Jupiter's magnetic field.

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