Geometric Albedo

Geometric Albedo is the ratio of the brightness of a celestial body at zero phase angle to that of a perfectly diffusing disk of the same size and distance, serving as a measure of its reflectivity under direct illumination.

311

Publications

15.5K

Citations

1.3K

Authors

445

Institutions

Publications per year

2017–2026

66

Authors

1.3K

  1. MG
    M. Gillon

    University of Liège, Belgium

    10 publications · 905 citations

    10

    h-index

  2. TM
    Thomas Müller

    Max Planck Institute for Extraterrestrial Physics, Germany

    9 publications · 315 citations

    9

    h-index

  3. SS
    Sara Seager

    Massachusetts Institute of Technology, United States

    9 publications · 1.2K citations

    9

    h-index

  4. AP
    András Pál

    Konkoly Observatory, Hungary

    8 publications · 260 citations

    8

    h-index

  5. AC
    A. Collier Cameron

    University of St Andrews, United Kingdom

    8 publications · 401 citations

    8

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 42 publications · 2.9K citations

    28

    h-index

  2. The Astronomical Journal

    AJ · 47 publications · 2.1K citations

    28

    h-index

  3. Icarus

    37 publications · 2.1K citations

    24

    h-index

  4. Astronomy and Astrophysics

    33 publications · 1.2K citations

    23

    h-index

  5. 17

    h-index

1–5