Apsidal Precession
Apsidal precession is the gradual rotation of the line connecting the closest and farthest points of an orbiting body’s elliptical trajectory around a central mass, arising from secular perturbations that perturb the orbital elements over time, thereby distinguishing it from other forms of orbital precession by specifically affecting the orientation of the orbit's apsides.
185
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9.1K
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513
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270
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Publications per year
2017–2026
42
185
Eclipsing binaries in open clusters. II. V453Cyg in NGC6871 ⋆
J. Southworth, P. F. L. Maxted, B. Smalley · 2008 · 246 citations
Natural Sciences, Astronomy, Physics +13
Apsidal Motion in Binary Stars
T. E. Sterne · Monthly Notices of the Royal Astronomical Society · 1939 · 207 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Astronomical Institute of the Slovak Academy of Sciences, Slovakia
7 publications · 170 citations
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270

Cornell University
Ithaca, United States
11 h-index
22 publications
858 citations
California Institute of Technology
Pasadena, United States
10 h-index
21 publications
2.4K citations
Charles University
Prague, Czechia
10 h-index
15 publications
275 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
14 publications
1.6K citations
Princeton University
Princeton, United States
8 h-index
17 publications
1.4K citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
8 h-index
12 publications
220 citations
Jet Propulsion Laboratory
Pasadena, United States
7 h-index
13 publications
309 citations

Keele University
Newcastle-under-Lyme, United Kingdom
7 h-index
12 publications
1.5K citations
1–8 of 270
51 publications · 2.7K citations
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ApJ · 29 publications · 1.7K citations
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18 publications · 613 citations
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AJ · 14 publications · 647 citations
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8 publications · 541 citations
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