West Candor Chasma, Mars. What is New?

Details West Candor Chasma, Mars. What is New? West Candor Chasma, Mars. What is New?

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1490l&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1490

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Geologic mapping showed many stratigraphic discontinuities but major
unconformities are scarce. Interbedded resistant dark layers could be
volcanic. Curvilinear reentrants on Ceti Mensa may be caused by
gravitational failure combined with erosion.

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