Formation of Martian Valley Networks: Melting of Low to Mid-latitude Snowpacks During Periods of High Obliquity?

Details Formation of Martian Valley Networks: Melting of Low to Mid-latitude Snowpacks During Periods of High Obliquity? Formation of Martian Valley Networks: Melting of Low to Mid-latitude Snowpacks During Periods of High Obliquity?

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1183c&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1183

Physics

Scientific paper

Martian valley networks may be cold climate features formed by melting
of snowpacks during periods of high obliquity.

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