Disk Instability Theory
Disk Instability Theory is a theoretical model of planetary formation in which gravitational instabilities within a protoplanetary disk lead to the direct collapse of gas and dust into planet-sized bodies, distinguishing it from core accretion models that require gradual solid core growth followed by gas capture.
151
Publications
14.3K
Citations
392
Authors
272
Institutions
Publications per year
2017–2026
25
Variants
Gravitational Instability ModelGravitational Instability Theory
Parents
151
On the gravitational stability of a disk of stars
Alar Toomre · The Astrophysical Journal · 1964 · 3.3K citations
Natural Sciences, Astronomy, Physics +15
Clustering instability in dissipative gases
I. Goldhirsch, Gianluigi Zanetti · Physical Review Letters · 1993 · 925 citations
Yoji Osaki · Publications of the Astronomical Society of the Pacific · 1996 · 487 citations · Full text
Natural Sciences, Astronomy, Physics +16
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272

Centre National de la Recherche Scientifique
Paris, France
13 h-index
26 publications
1.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
10 h-index
13 publications
935 citations
Max Planck Institute for Astrophysics
Garching, Germany
8 h-index
8 publications
664 citations

Carnegie Institution for Science
Washington, United States
8 h-index
8 publications
1K citations

Kyoto University
Kyoto, Japan
7 h-index
23 publications
615 citations

Space Telescope Science Institute
Baltimore, United States
7 h-index
13 publications
727 citations
University of Arizona
Tucson, United States
7 h-index
11 publications
694 citations
Institut d'Astrophysique de Paris
Paris, France
7 h-index
10 publications
922 citations
1–8 of 272
ApJ · 57 publications · 8K citations
38
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16 publications · 870 citations
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14 publications · 647 citations
13
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11 publications · 281 citations
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8 publications · 389 citations
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