Planetary System Stability
Planetary System Stability is a theoretical construct in astrophysics that characterizes the long-term dynamical persistence of orbital configurations within a planetary system, distinguishing it from transient or chaotic arrangements by its reliance on gravitational interactions that maintain bounded, non-colliding trajectories over astronomical timescales.
325
Publications
19.3K
Citations
732
Authors
353
Institutions
Publications per year
2017–2026
71
325
Are There Unstable Planetary Systems around White Dwarfs?
The Astrophysical Journal · 2002 · 453 citations · Full text
Natural Sciences, Astronomy, Physics +17
Spin-orbit angle measurements for six southern transiting planets
A. H. M. J. Triaud, A. Collier Cameron, D. Queloz et al. · Astronomy and Astrophysics · 2010 · 450 citations · Full text
Natural Sciences, Astronomy, Physics +16
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732
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353

Centre National de la Recherche Scientifique
Paris, France
24 h-index
85 publications
4.3K citations

Ames Research Center
Mountain View, United States
18 h-index
46 publications
12.9K citations
Nicolaus Copernicus University
Torun, Poland
16 h-index
24 publications
976 citations

UNSW Sydney
Sydney, Australia
16 h-index
53 publications
3.6K citations
University of Vienna
Vienna, Austria
15 h-index
37 publications
1.6K citations
University of Arizona
Tucson, United States
14 h-index
41 publications
2.7K citations

Sorbonne Université
Paris, France
13 h-index
25 publications
1.4K citations
Princeton University
Princeton, United States
12 h-index
20 publications
1.1K citations
1–8 of 353
ApJ · 63 publications · 5.4K citations
46
h-index
65 publications · 2.9K citations
36
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36 publications · 1.9K citations
25
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AJ · 25 publications · 1.7K citations
18
h-index
17 publications · 1.4K citations
16
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