The Longitudinal Extent of a Layered Sequence in the Sub-Surface of Mars: Evidence for Diagenesis in the Hesperian

Details The Longitudinal Extent of a Layered Sequence in the Sub-Surface of Mars: Evidence for Diagenesis in the Hesperian The Longitudinal Extent of a Layered Sequence in the Sub-Surface of Mars: Evidence for Diagenesis in the Hesperian

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1254c&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1254

Physics

Scientific paper

Horizontal rock layers are visible at wall tops throughout Valles
Marineris, Mars. Similar layers are exposed by impact craters in the
whole equatorial region, except under the Tharsis. So, these layers
reflect a global process of rock formation.

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