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Detailed Reference Information |
Janes, D.M. and Squyres, S.W. (1995). Viscoelastic relaxation of topographic highs on Venus to produce coronae. Journal of Geophysical Research 100: doi: 10.1029/95JE01748. issn: 0148-0227. |
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Coronae on Venus are believed to result from the gravitationally driven relaxation of topography that was originally raised by mantle diapirs. We examine this relaxation using a viscoelastic finite element code, and show that an initially plateau shaped load will evolve to the characteristic corona topography of central raised bowl, annular rim, and surrounding moat. Stresses induced by the relaxation are consistent with the development of concentric extensional fracturing common on the outer margins of corona moats. However, relaxation is not expected to produce the concentric faulting often observed on the annular rim. The relaxation timescale is shorter than the diapir cooling timescale, so loss of thermal support controls the rate at which topography is reduced. The final corona shape is supported by buoyancy and flexural stresses and will persist through geologic time. Development of lower, flatter central bowls and narrower and more pronounced annular rims and moats enhanced by thicker crusts, higher thermal gradients, and crustal thinning over the diapir. ¿ American Geophysical Union 1995. |
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Abstract |
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Keywords
Tectonophysics, Stresses—crust and lithosphere, Tectonophysics, Dynamics, gravity and tectonics, Tectonophysics, Dynamics of lithosphere and mantle—general, Planetology, Solid Surface Planets, Tectonics |
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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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