Cometary Volatiles
Cometary Volatiles is a scientific construct referring to the class of low-boiling-point chemical compounds, predominantly water, carbon dioxide, ammonia, and methane, that sublimate readily from the solid phase to gas upon solar heating and are native to the icy matrix of comets, thereby driving cometary activity and providing diagnostic signatures of primordial solar system composition.
302
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20.3K
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976
Authors
364
Institutions
Publications per year
2017–2026
66
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302
A comet model. I. The acceleration of Comet Encke
Fred L. Whipple · The Astrophysical Journal · 1950 · 871 citations
Natural Sciences, Astronomy, Physics +15
1–5 of 302
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Johns Hopkins University Applied Physics Laboratory, United States
21 publications · 1.3K citations
17
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17
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364
Goddard Space Flight Center
Greenbelt, United States
32 h-index
182 publications
12.2K citations

Centre National de la Recherche Scientifique
Paris, France
30 h-index
222 publications
15.2K citations
University of Bern
Bern, Switzerland
24 h-index
138 publications
12.4K citations
Université Paris Cité
Paris, France
23 h-index
84 publications
6.1K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
23 h-index
77 publications
5.8K citations
Catholic University of America
Washington D.C., United States
22 h-index
52 publications
2.5K citations
University of America
Murrieta, United States
22 h-index
53 publications
2.4K citations

Southwest Research Institute
San Antonio, United States
20 h-index
42 publications
4.6K citations
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ApJ · 46 publications · 3.9K citations
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38 publications · 2.2K citations
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23 publications · 1.4K citations
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AJ · 21 publications · 752 citations
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16 publications · 3K citations
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