Possible Secondary Aqueous Deposits in West Candor Chasma, Mars

Details Possible Secondary Aqueous Deposits in West Candor Chasma, Mars Possible Secondary Aqueous Deposits in West Candor Chasma, Mars

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1952l&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1952

Physics

1

Scientific paper

Possible channels with inverted relief on Ceti Mensa merge with a lobe
of rounded, blocky deposits, suggesting that aqueous processes formed
lobes on this ILD mound. Younger, finely layered materials in troughs
below the mound may be secondary and eroded from the mensa.

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