Sidereal Rotation

Sidereal Rotation is the rotational period of a celestial body measured relative to the fixed stars, distinguishing it from synodic or solar rotation by using distant stellar references as a fixed background.

70

Publications

3.6K

Citations

631

Authors

200

Institutions

Publications per year

2017–2026

15

Variants

Sidereal Rotational Period

Authors

631

  1. HO
    Hari Om Vats

    Physical Research Laboratory, India

    4 publications · 145 citations

    4

    h-index

  2. RB
    R. Brajša

    University of Zagreb, Croatia

    3 publications · 155 citations

    3

    h-index

  3. DV
    David Vokrouhlický

    Charles University, Czechia

    3 publications · 141 citations

    3

    h-index

  4. HW
    H. Wöhl

    Institut für Sonnenphysik, Germany

    3 publications · 155 citations

    3

    h-index

  5. II
    I. I. Shapiro

    Massachusetts Institute of Technology, United States

    3 publications · 134 citations

    3

    h-index

1–5 of 631

Venues

  1. Astronomy and Astrophysics

    14 publications · 475 citations

    14

    h-index

  2. The Astronomical Journal

    AJ · 10 publications · 740 citations

    10

    h-index

  3. The Astrophysical Journal

    ApJ · 9 publications · 490 citations

    9

    h-index

  4. Icarus

    4 publications · 93 citations

    4

    h-index

  5. 4

    h-index

1–5