Interpreting Mascon Wrinkle Ridges on Isidis Planitia, Mars Using Axial Surface Mapping Techniques: Reconstructing Structural Development and Stress Environments

Details Interpreting Mascon Wrinkle Ridges on Isidis Planitia, Mars Using Axial Surface Mapping Techniques: Reconstructing Structural Development and Stress Environments Interpreting Mascon Wrinkle Ridges on Isidis Planitia, Mars Using Axial Surface Mapping Techniques: Reconstructing Structural Development and Stress Environments

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1430w&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1430

Physics

Scientific paper

Isidis Planitia on Mars is a mascon containing radial and concentric
wrinkle ridges, surrounded by concentric graben. Using axial surface
mapping techniques, we analyze the wrinkle ridges to constrain their
blind thrust geometry at depth in order to constrain the nature of basin
rheology.

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