Periastron Precession
Periastron Precession is a relativistic orbital phenomenon in post-Newtonian gravity that describes the gradual advance of the point of closest approach in a binary system’s orbit due to the curvature of spacetime caused by the masses’ gravitational interaction.
154
Publications
7.6K
Citations
330
Authors
267
Institutions
Publications per year
2017–2026
52
Variants
Periastron Advance
Parents
154
Precession of Mercury’s Perihelion from Ranging to the MESSENGER Spacecraft
Ryan S. Park, W. M. Folkner, Alexander S. Konopliv et al. · The Astronomical Journal · 2017 · 208 citations
Natural Sciences, Astronomy, Physics +17
Phasing of gravitational waves from inspiralling eccentric binaries
Thibault Damour, A. Gopakumar, B. R. Iyer · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2004 · 182 citations · Full text
Natural Sciences, Astronomy, Physics +15
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267

Centre National de la Recherche Scientifique
Paris, France
8 h-index
8 publications
1K citations

University of Manchester
Manchester, United Kingdom
6 h-index
6 publications
411 citations
Princeton University
Princeton, United States
6 h-index
6 publications
315 citations
Université Larbi Tébessi
Tébessa, Algeria
6 h-index
6 publications
119 citations

Khazar University
Baku, Azerbaijan
6 h-index
6 publications
119 citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
5 h-index
5 publications
749 citations
California Institute of Technology
Pasadena, United States
5 h-index
5 publications
224 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
4 publications
413 citations
1–8 of 267
ApJ · 21 publications · 1.4K citations
19
h-index
21 publications · 643 citations
14
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12 publications · 806 citations
12
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9 publications · 272 citations
9
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7 publications · 956 citations
7
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