Beagle Rupes and Rembrandt scarp: a comparison on Mercury surface

Details Beagle Rupes and Rembrandt scarp: a comparison on Mercury surface Beagle Rupes and Rembrandt scarp: a comparison on Mercury surface

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..963f&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.963

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Areas of crustal convergence and shortening on Earth, Mars and Venus are often characterized by structural domains where thrust faults are associated with strike-slip systems [1]. In the case of Mercury most structures maintain a wide elongated frontal scarp and only few of them show kinematic indicators of lateral slip. The comparison between two Mercurian linked fault systems like Beagle Rupes [2] [3] and Rembrandt scarp [4] could aid understanding of whether diverse hermean strike-slip structures are influenced by geological context such as surface heterogeneity and crustal layering or have different deformational history.

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