Mercury Thermal Evolution
Mercury Thermal Evolution is a planetary science theory that elucidates the temporal development and dissipation of internal heat within Mercury, distinguishing itself by integrating the planet's unique thermochemical properties, rapid cooling history, and prolonged tectonic deformation to explain observed surface features and global contraction.
129
Publications
5.5K
Citations
385
Authors
203
Institutions
Publications per year
2017–2026
18
Parents
129
Mantle differentiation and thermal evolution of Mars, Mercury, and Venus
Tilman Spohn · Icarus · 1991 · 165 citations
1–5 of 129
385
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Institut Préparatoire aux Études d'Ingénieurs de Monastir, Tunisia
3 publications · 67 citations
3
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3
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1–5 of 385
203

Carnegie Institution for Science
Washington, United States
7 h-index
7 publications
267 citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
20 publications
578 citations
California Institute of Technology
Pasadena, United States
6 h-index
10 publications
959 citations

Southwest Research Institute
San Antonio, United States
6 h-index
8 publications
744 citations
Massachusetts Institute of Technology
Cambridge, United States
6 h-index
9 publications
700 citations
Carnegie Observatories
Pasadena, United States
5 h-index
5 publications
216 citations
University of Münster
Münster, Germany
4 h-index
8 publications
435 citations
Arizona State University
Tempe, United States
4 h-index
8 publications
724 citations
1–8 of 203
15 publications · 1.3K citations
13
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10 publications · 482 citations
10
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7 publications · 112 citations
7
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5 publications · 91 citations
5
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5 publications · 175 citations
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