Late Noachian to Hesperian Climate Change on Mars: Evidence from Crater Lakes and Thermokarst Terrain Near Ares Vallis

Details Late Noachian to Hesperian Climate Change on Mars: Evidence from Crater Lakes and Thermokarst Terrain Near Ares Vallis Late Noachian to Hesperian Climate Change on Mars: Evidence from Crater Lakes and Thermokarst Terrain Near Ares Vallis

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1320w&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1320

Physics

Scientific paper

We suggest that the presence of Hesperian-age crater outlet channels in
association with Hesperian-age alas-lake type thermokarst features
requires climate conditions that were favorable for the transient
occurrence of stable surface liquid water.

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