Orbital Perturbations
Orbital Perturbations is a dynamical deviation in the trajectory of a celestial or artificial satellite from its ideal two-body Keplerian orbit, caused by external forces such as gravitational influences from third bodies, atmospheric drag, solar radiation pressure, or non-spherical mass distributions of the primary body.
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2017–2026
366
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Gravitational Radiation from Point Masses in a Keplerian Orbit
P. C. Peters, Jon Mathews · Physical Review · 1963 · 1.6K citations
Natural Sciences, Astronomy, Physics +17
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Electronics and Radar Development Establishment, India
18 publications · 444 citations
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Centre National de la Recherche Scientifique
Paris, France
40 h-index
201 publications
10.2K citations
Jet Propulsion Laboratory
Pasadena, United States
31 h-index
124 publications
10.6K citations
California Institute of Technology
Pasadena, United States
30 h-index
78 publications
8.7K citations
Observatoire de la Côte d’Azur
Nice, France
27 h-index
77 publications
4.3K citations
University of Colorado Boulder
Boulder, United States
27 h-index
102 publications
4.2K citations
The University of Texas at Austin
Austin, United States
25 h-index
59 publications
3.9K citations

Cornell University
Ithaca, United States
25 h-index
71 publications
5.7K citations
Goddard Space Flight Center
Greenbelt, United States
24 h-index
66 publications
2.8K citations
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ApJ · 99 publications · 8K citations
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AJ · 143 publications · 10.4K citations
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181 publications · 7.8K citations
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216 publications · 7.7K citations
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94 publications · 6.1K citations
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