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Detailed Reference Information |
Chapman, M.G. and Kirk, R.L. (1996). A migratory mantle plume on Venus: Implications for Earth?. Journal of Geophysical Research 101: doi: 10.1029/96JB00883. issn: 0148-0227. |
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A spatially fixed or at least internally rigid hotspot reference frame has been assumed for determining relative plate motions on Earth. Recent 1:5,000,000 scale mapping of Venus, a planet without terrestrial-style plate tectonics and ocean cover, reveals a systematic age and dimensional progression of corona-like arachnoids occurring in an uncinate chain. The nonrandom associations between arachnoids indicate they likely formed from a deep-seated mantle plume in a manner similar to terrestrial hotspot features. However, absence of expected convergent ''plate'' margin deformation suggests that the arachnoids are the surface expression of a migratory mantle plume beneath a stationary surface. If mantle plumes are not stationary on Venus, what if any are the implications for Earth? |
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Abstract |
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Keywords
Tectonophysics, Dynamics, convection currents and mantle plumes, Planetology, Solid Surface Planets, Interiors, Planetology, Solar System Objects, Venus, Planetology, Solid Surface Planets, Volcanism |
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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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