Solar Motion

Solar Motion is a kinematic construct in galactic astronomy that denotes the peculiar velocity of the Sun relative to the local standard of rest, distinguished by its characterization of the Sun's absolute motion through the Galaxy as inferred from the systematic proper motions and radial velocities of nearby stars.

211

Publications

14.7K

Citations

555

Authors

258

Institutions

Publications per year

2017–2026

29

Variants

Sun's Peculiar Motion

Authors

555

  1. IC
    Ivanka Charvátová

    Czech Academy of Sciences, Institute of Geophysics, Czechia

    8 publications · 256 citations

    8

    h-index

  2. SR
    Steven R. Majewski

    University of Virginia, United States

    5 publications · 257 citations

    5

    h-index

  3. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    5 publications · 315 citations

    5

    h-index

  4. WL
    W. L. Peters

    Florida Agricultural and Mechanical University, United States

    5 publications · 160 citations

    5

    h-index

  5. GG
    G. Gilmore

    University of Cambridge, United Kingdom

    4 publications · 314 citations

    4

    h-index

1–5 of 555

Venues

  1. The Astrophysical Journal

    ApJ · 39 publications · 3.8K citations

    26

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    33 publications · 4.1K citations

    22

    h-index

  3. The Astronomical Journal

    AJ · 24 publications · 1.1K citations

    17

    h-index

  4. Solar Physics

    10 publications · 363 citations

    10

    h-index

  5. Astronomy and Astrophysics

    9 publications · 448 citations

    9

    h-index

1–5