Secular Perturbations
Secular Perturbations is a type of long-term gravitational disturbance in celestial mechanics that produces gradual, non-periodic changes in the orbital elements of a celestial body over time, distinguishing it from short-period or periodic perturbations.
164
Publications
10.8K
Citations
306
Authors
152
Institutions
Publications per year
2017–2026
18
164
The motion of a close earth satellite
Yoshihide Kozai · The Astronomical Journal · 1959 · 502 citations
A three million year integration of the earth's orbit
Thomas Quinn, Scott Tremaine, Martin J. Duncan · The Astronomical Journal · 1991 · 277 citations
Natural Sciences, Astronomy, Physics +16
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152

Centre National de la Recherche Scientifique
Paris, France
10 h-index
41 publications
1.3K citations

Sorbonne Université
Paris, France
9 h-index
15 publications
735 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
7 h-index
9 publications
287 citations
Institut de Mécanique Céleste et de Calcul des Éphémérides
Paris, France
7 h-index
12 publications
492 citations

Observatoire de Paris
Paris, France
4 h-index
8 publications
402 citations

University of Pisa
Pisa, Italy
4 h-index
5 publications
289 citations

Smithsonian Astrophysical Observatory
Cambridge, United States
4 h-index
4 publications
2.8K citations
Roche (France)
Paris, France
4 h-index
8 publications
352 citations
1–8 of 152
17 publications · 833 citations
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AJ · 13 publications · 4.1K citations
13
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14 publications · 623 citations
12
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ApJ · 11 publications · 830 citations
11
h-index
9 publications · 214 citations
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