Physics
Scientific paper
Apr 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006georl..3308202d&link_type=abstract
Geophysical Research Letters, Volume 33, Issue 8, CiteID L08202
Physics
4
Planetary Sciences: Solid Surface Planets: Tectonics (8149), Planetary Sciences: Solar System Objects: Mars, Structural Geology: Dynamics And Mechanics Of Faulting (8118), Tectonophysics: Stresses: Crust And Lithosphere, Tectonophysics: Dynamics: Gravity And Tectonics
Scientific paper
Current stress solutions for Mars match the long wavelength signal of present day topography and gravity but fail to match many surface faults, including the normal faults in northern Claritas Fossae north to Tantalus and Alba Fossae. A deviatoric stress field associated with horizontal gradients of gravitational potential energy (GPE) provides an excellent fit, as measured by objective functions, to many of the normal faults in the western Martian hemisphere as well as wrinkle ridges circumferential to Tharsis; ~70% of the faults have a misfit <= 0.1. The fit of faults to the GPE-derived stress field reflects the thermal state of the planet at the times of faulting, and suggests that at such times elastic thicknesses and membrane stresses were small, and topography was supported by buoyancy forces.
Dimitrova Lada L.
Haines John Allan
Holt William E.
Schultz Richard A.
No associations
LandOfFree
Toward understanding the history and mechanisms of Martian faulting: The contribution of gravitational potential energy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Toward understanding the history and mechanisms of Martian faulting: The contribution of gravitational potential energy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Toward understanding the history and mechanisms of Martian faulting: The contribution of gravitational potential energy will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1499098