What was the Role of Water in ILD Formation on Mars?: Insights from New CRISM Techniques

Details What was the Role of Water in ILD Formation on Mars?: Insights from New CRISM Techniques What was the Role of Water in ILD Formation on Mars?: Insights from New CRISM Techniques

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2082h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2082

Physics

1

Scientific paper

We hypothesise that ILD sediments are analogous to NPLD, which suggests
a climatic control dominated by orbital forcing. A statistical analysis
of the spectral variance of CRISM has shown a lack of hydrated minerals
over ILD features in Arabia Terra.

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