Plate tectonics on Venus?

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چکیده

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Volcanism and Tectonics on Venus

We review recent developments in the study of volcanism and tectonics on Venus. Venus’s crust is basaltic, dry, and probably about 30 km thick. The mantle convects, giving rise to plumes, and has a similar composition and mean temperature (∼1300◦C), but a higher viscosity (∼1020 Pa s), than that of the Earth. Inferred melt generation rates constrain the lithospheric thickness to between 80 and ...

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ژورنال

عنوان ژورنال: The Journal of the Geological Society of Japan

سال: 1990

ISSN: 0016-7630,1349-9963

DOI: 10.5575/geosoc.96.297