Proper Motion

Proper Motion is the apparent angular displacement of a celestial object on the celestial sphere, distinguished from other types of observed motion by representing the gradual change in position relative to distant background stars over time due to the object's true motion through space.

3.5K

Publications

251.9K

Citations

8.7K

Authors

1.4K

Institutions

Publications per year

2017–2026

842

Authors

8.7K

  1. JA
    Jay Anderson

    Space Telescope Science Institute, United States

    48 publications · 3.8K citations

    34

    h-index

  2. GG
    G. Gilmore

    University of Cambridge, United Kingdom

    36 publications · 4.7K citations

    33

    h-index

  3. AG
    Andrew Gould

    The Ohio State University, United States

    48 publications · 3K citations

    31

    h-index

  4. NC
    N. C. Hambly

    University of Edinburgh, United Kingdom

    38 publications · 4.3K citations

    31

    h-index

  5. MJ
    M. J. Reid

    Center for Astrophysics Harvard & Smithsonian, United States

    40 publications · 6K citations

    30

    h-index

1–5 of 8.7K

Venues

  1. The Astrophysical Journal

    ApJ · 835 publications · 66.5K citations

    131

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    599 publications · 38.8K citations

    96

    h-index

  3. The Astronomical Journal

    AJ · 486 publications · 39K citations

    96

    h-index

  4. Astronomy and Astrophysics

    461 publications · 32.2K citations

    90

    h-index

  5. The Astrophysical Journal Letters

    69 publications · 6.1K citations

    41

    h-index

1–5