Crustal Thickness Control on Martian Wrinkle Ridge Spacing

Details Crustal Thickness Control on Martian Wrinkle Ridge Spacing Crustal Thickness Control on Martian Wrinkle Ridge Spacing

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1879m&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1879

Physics

1

Scientific paper

The spacing of wrinkle ridges in the Martian northern lowlands is about
twice that in ridged plains. This can be explained by the thinner crust
in the lowlands: there is no ductile lower crust, making the brittle
upper lithosphere twice thicker.

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