Climate Change on Mars from Erosion Rates at the Mars Exploration Rover Landing Sites

Details Climate Change on Mars from Erosion Rates at the Mars Exploration Rover Landing Sites Climate Change on Mars from Erosion Rates at the Mars Exploration Rover Landing Sites

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3034g&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3034

Physics

1

Scientific paper

The gradation history of the Gusev and Meridiani plains argues for a dry
and desiccating environment since the Late Hesperian, in contrast to the
sedimentary evaporites in Meridiani Planum that document a warmer and
wetter environment in the Noachian.

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