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Chapman & Kirk 1996
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.

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?

BACKGROUND DATA FILES

Abstract

Keywords
Tectonophysics, Dynamics, convection currents and mantle plumes, Planetology, Solid Surface Planets, Interiors, Planetology, Solar System Objects, Venus, Planetology, Solid Surface Planets, Volcanism
Journal
Journal of Geophysical Research
http://www.agu.org/journals/jb/
Publisher
American Geophysical Union
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