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Detailed Reference Information |
Grott, M., Hauber, E., Werner, S.C., Kronberg, P. and Neukum, G. (2005). High heat flux on ancient Mars: Evidence from rift flank uplift at Coracis Fossae. Geophysical Research Letters 32: doi: 10.1029/2005GL023894. issn: 0094-8276. |
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We have identified flexural uplift at the flanks of the Coracis Fossae Rift valley. Modeling the topography the elastic thickness is constrained to 10.3--12.5 km, the corresponding mechanical thickness and thermal gradient are 15--19 km and 27--33 K km-1, respectively. The time of rifting is dated by evaluating the crater size-frequency distribution of key surface units related to the rifting. Thus, the heat flux between 3.5 and 3.9 Ga is calculated to be 54--66 mW m-2. Furthermore, the stresses supported by the rift bounding faults are estimated to be below 5 MPa. We speculate that this weakness may be connected to the presence of water below the surface. |
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Abstract![](/images/icons/spacer.gif) |
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Keywords
Planetary Sciences, Solid Surface Planets, Heat flow, Planetary Sciences, Solar System Objects, Mars, Tectonophysics, Continental tectonics, extensional, Tectonophysics, Lithospheric flexure, Tectonophysics, Stresses, crust and lithosphere |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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