Venusian Surface Composition
Venusian Surface Composition is a geoscientific construct that specifies the elemental, mineralogical, and chemical makeup of the planetary surface of Venus, distinguished from other terrestrial planetary surface compositions by its unique geochemical signatures, volcanic origins, and extreme surface conditions.
72
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3.4K
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212
Authors
98
Institutions
Publications per year
2017–2026
17
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72
Venus Surface Composition Constrained by Observation and Experiment
M. S. Gilmore, A. H. Treiman, J. Helbert et al. · Space Science Reviews · 2017 · 126 citations
Venus rock composition at the Vega 2 Landing Site
Yu. A. Surkov, L. P. Moskalyova, V. P. Kharyukova et al. · Journal of Geophysical Research Atmospheres · 1986 · 123 citations
Structure of the Venusian atmosphere from surface up to 100 km
L. V. Zasova, V. M. Linkin, I. Khatuntsev et al. · Cosmic Research · 2006 · 121 citations
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Massachusetts Institute of Technology, United States
4 publications · 106 citations
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1–5 of 212
98
Planetary Science Institute
Tucson, United States
10 h-index
22 publications
899 citations

Space Research Institute
Moscow, Russia
8 h-index
14 publications
928 citations
Massachusetts Institute of Technology
Cambridge, United States
7 h-index
27 publications
1K citations
Jet Propulsion Laboratory
Pasadena, United States
6 h-index
13 publications
456 citations
Cardiff University
Cardiff, United Kingdom
5 h-index
8 publications
298 citations
V.I. Vernadsky Institute of Geochemistry and Analytical Chemistry
Moscow, Russia
5 h-index
21 publications
1.5K citations
University of Cambridge
Cambridge, United Kingdom
4 h-index
5 publications
181 citations
American Institute of Aeronautics and Astronautics
Reston, United States
4 h-index
4 publications
140 citations
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26 publications · 1.1K citations
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JGR · 5 publications · 494 citations
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5 publications · 155 citations
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5 publications · 201 citations
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3 publications · 181 citations
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