Insight to the Evolution of Wrinkle Ridges in Hesperia Planum, Mars

Details Insight to the Evolution of Wrinkle Ridges in Hesperia Planum, Mars Insight to the Evolution of Wrinkle Ridges in Hesperia Planum, Mars

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1135g&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1135

Physics

3

Scientific paper

Wrinkle ridges are linear to arcuate, asymmetric, topographic highs; the
precise origin is unknown. Study results reveal NE-striking wrinkle
ridges formed prior to NW-striking wrinkle ridges, and the deposits of
Hesperia Planum are thin, <2km.

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