Light Layer and Sinuous Ridges on Plateau Near Juventae Chasma, Mars

Details Light Layer and Sinuous Ridges on Plateau Near Juventae Chasma, Mars Light Layer and Sinuous Ridges on Plateau Near Juventae Chasma, Mars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1500l&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1500

Computer Science

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Scientific paper

The layer is associated with ridges topped by channels, indicating
inverted relief. Dark flows overlap the light layer, suggesting
interbedding with lavas, and strengthening the idea that light,
incompetent layers occur in the walls of the Valles Marineris.

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