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

Publications

9.1K

Citations

513

Authors

270

Institutions

Publications per year

2017–2026

42

Authors

513

  1. KF
    Kh. F. Khaliullin

    Astronomical Institute of the Slovak Academy of Sciences, Slovakia

    7 publications · 170 citations

    8

    h-index

  2. MW
    M. Wolf

    Charles University, Czechia

    7 publications · 141 citations

    7

    h-index

  3. DL
    Dong Lai

    Cornell University, United States

    5 publications · 204 citations

    6

    h-index

  4. JP
    J. Patterson

    Columbia University, United States

    6 publications · 340 citations

    6

    h-index

  5. MZ
    Miloslav Zejda

    Masaryk University, Czechia

    5 publications · 102 citations

    5

    h-index

1–5 of 513

Venues

  1. Monthly Notices of the Royal Astronomical Society

    51 publications · 2.7K citations

    29

    h-index

  2. The Astrophysical Journal

    ApJ · 29 publications · 1.7K citations

    23

    h-index

  3. Astronomy and Astrophysics

    18 publications · 613 citations

    14

    h-index

  4. The Astronomical Journal

    AJ · 14 publications · 647 citations

    13

    h-index

  5. The Astrophysical Journal Letters

    8 publications · 541 citations

    8

    h-index

1–5