Snow Line Evolution
Snow Line Evolution is a theoretical construct in planetary science that denotes the time-dependent migration of the radial distance in a protoplanetary disk beyond which volatile compounds such as water, ammonia, and methane can condense into solid ice grains, distinguishing it from static snow line models by incorporating dynamical changes due to disk cooling, accretion, and stellar radiation.
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2017–2026
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Planetesimal formation starts at the snow line
Astronomy and Astrophysics · 2017 · 276 citations · Full text
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Centre National de la Recherche Scientifique
Paris, France
12 h-index
23 publications
1.1K citations
Tokyo Institute of Technology
Tokyo, Japan
11 h-index
19 publications
1.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
6 h-index
9 publications
889 citations
University of Wisconsin–Madison
Madison, United States
5 h-index
8 publications
243 citations
Life Science Institute
Tokyo, Japan
4 h-index
4 publications
202 citations
University of Arizona
Tucson, United States
4 h-index
7 publications
881 citations
Observatoire de la Côte d’Azur
Nice, France
4 h-index
4 publications
311 citations

Space Telescope Science Institute
Baltimore, United States
3 h-index
4 publications
480 citations
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ApJ · 15 publications · 2K citations
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9 publications · 784 citations
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5 publications · 150 citations
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