Physics
Scientific paper
Mar 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1646i&link_type=abstract
37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1646
Physics
Scientific paper
Martian gullies are formed on the slopes with high inclination and their
distribution seems to be consistent with distribution of seasonal
condensation of CO2 at high obliquity. This may suggest that gullies
have been formed by avalanches of CO2 ice.
Ishii Takaaki
Miyamoto Hideaki
Sasaki Satoshi
Tajika Eiichi
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