Orbital Eccentricity

Orbital Eccentricity is a dimensionless scalar parameter in conic section orbits that quantifies the deviation of an orbit from a perfect circle, specifically defined as the ratio of the distance between the foci of the conic to its major axis length.

900

Publications

61.1K

Citations

4.5K

Authors

871

Institutions

Publications per year

2017–2026

229

Authors

4.5K

  1. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    19 publications · 989 citations

    17

    h-index

  2. DQ
    D. Queloz

    University of Geneva, Switzerland

    16 publications · 1.2K citations

    16

    h-index

  3. RP
    R. Paul Butler

    Carnegie Institution for Science, United States

    14 publications · 3.3K citations

    14

    h-index

  4. GW
    Geoffrey W. Marcy

    University of California, Berkeley, United States

    14 publications · 3.5K citations

    14

    h-index

  5. SU
    S. Udry

    University of Geneva, Switzerland

    13 publications · 915 citations

    13

    h-index

1–5 of 4.5K

Venues

  1. The Astrophysical Journal

    ApJ · 165 publications · 16.6K citations

    74

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    146 publications · 8.6K citations

    53

    h-index

  3. Astronomy and Astrophysics

    73 publications · 4.5K citations

    38

    h-index

  4. The Astronomical Journal

    AJ · 87 publications · 4K citations

    36

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 36 publications · 2.5K citations

    26

    h-index

1–5