Accretional Heating
Accretional Heating is the process by which gravitational potential energy is converted into thermal energy during the successive impacts and coalescence of planetesimals in the formation of planetary bodies, contributing significantly to the internal heat budget during planetary accretion.
41
Publications
2.1K
Citations
136
Authors
90
Institutions
Publications per year
2017–2026
11
41
Magnesium isotope evidence that accretional vapour loss shapes planetary compositions
Remco C. Hin, Christopher D. Coath, Philip J. Carter et al. · Nature · 2017 · 202 citations · Full text
On the Snow Line in Dusty Protoplanetary Disks
The Astrophysical Journal · 2000 · 188 citations · Full text
Natural Sciences, Astronomy, Physics +17
Radiative efficiency of hot accretion flows
Fu‐Guo Xie · Monthly Notices of the Royal Astronomical Society · 2012 · 185 citations · Full text
Natural Sciences, Astronomy, Physics +17
A water budget dichotomy of rocky protoplanets from 26Al-heating
Tim Lichtenberg, Gregor Golabek, Remo Burn et al. · Nature Astronomy · 2019 · 146 citations · Full text
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Space Telescope Science Institute
Baltimore, United States
5 h-index
6 publications
341 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
4 h-index
4 publications
223 citations

Villanova University
Radnor, United States
3 h-index
7 publications
123 citations
Planetary Science Institute
Tucson, United States
3 h-index
5 publications
195 citations
University of Arizona
Tucson, United States
3 h-index
6 publications
152 citations
Jet Propulsion Laboratory
Pasadena, United States
3 h-index
4 publications
102 citations
University of California, Santa Cruz
Santa Cruz, United States
3 h-index
4 publications
307 citations
Arizona State University
Tempe, United States
2 h-index
2 publications
37 citations
1–8 of 90
ApJ · 8 publications · 427 citations
8
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3 publications · 251 citations
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3 publications · 96 citations
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JGR · 3 publications · 82 citations
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3 publications · 99 citations
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