Venusian Tectonics
Venusian Tectonics is a geological framework that characterizes the deformational processes and structural evolution of Venus's lithosphere, distinguished from terrestrial tectonics by the absence of global plate recycling and the prominence of crustal thickening, radial fracturing, and mantle-driven resurfacing mechanisms.
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5.6K
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190
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2017–2026
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E. R. Stofan, V. L. Sharpton, G. Schubert et al. · Journal of Geophysical Research Atmospheres · 1992 · 307 citations
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Brown University
Providence, United States
13 h-index
29 publications
1.2K citations
Jet Propulsion Laboratory
Pasadena, United States
8 h-index
21 publications
1.4K citations

Lunar and Planetary Institute
Houston, United States
7 h-index
11 publications
573 citations
Southern Methodist University
Dallas, United States
6 h-index
8 publications
559 citations
University of California, Los Angeles
Los Angeles, United States
5 h-index
6 publications
295 citations
Arizona State University
Tempe, United States
5 h-index
7 publications
337 citations
Russian Academy of Sciences
Moscow, Russia
4 h-index
5 publications
226 citations
Planetary Science Institute
Tucson, United States
4 h-index
6 publications
247 citations
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JGR · 22 publications · 1.6K citations
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