Nodal Precession
Nodal Precession is a type of secular perturbation in orbital mechanics characterized by the gradual, continuous rotation of the orbital plane of a celestial body about the symmetry axis of the central body, due to non-spherical gravitational forces, specifically manifesting as the precession of the line of nodes.
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2.9K
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216
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141
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2017–2026
23
Variants
Precession Of The Nodes
Parents
63
Planetary Systems in Binaries. I. Dynamical Classification
The Astrophysical Journal · 2008 · 104 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Cornell University
Ithaca, United States
6 h-index
12 publications
643 citations

Space Telescope Science Institute
Baltimore, United States
5 h-index
7 publications
555 citations
California Institute of Technology
Pasadena, United States
4 h-index
13 publications
560 citations
The University of Texas at Austin
Austin, United States
4 h-index
6 publications
301 citations
University of California, Santa Cruz
Santa Cruz, United States
3 h-index
7 publications
348 citations
Northwestern University
Evanston, United States
3 h-index
6 publications
522 citations
NASA Exoplanet Science Institute
Pasadena, United States
3 h-index
3 publications
166 citations
Columbia University
New York, United States
2 h-index
4 publications
248 citations
1–8 of 141
19 publications · 1K citations
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ApJ · 7 publications · 455 citations
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AJ · 3 publications · 122 citations
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3 publications · 124 citations
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Repository · 2 publications · 30 citations
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