Solar System Formation

Solar System Formation is the astrophysical process of planetary system development through the gravitational collapse and accretion of a primordial molecular cloud into a central star and its surrounding disk, from which planets, moons, asteroids, and comets originate via condensation, coagulation, and dynamical evolution specific to the Sun’s circumstellar environment.

525

Publications

42.2K

Citations

1.5K

Authors

553

Institutions

Publications per year

2017–2026

145

Authors

1.5K

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    17 publications · 2.2K citations

    16

    h-index

  2. AN
    Alexander N. Krot

    University of Hawaiʻi at Mānoa, United States

    16 publications · 2K citations

    15

    h-index

  3. DN
    David Nesvorný

    Southwest Research Institute, United States

    9 publications · 486 citations

    9

    h-index

  4. GR
    G. R. Huss

    University of Hawaiʻi at Mānoa, United States

    9 publications · 568 citations

    9

    h-index

  5. YA
    Y. Alibert

    University of Bern, Switzerland

    9 publications · 637 citations

    9

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 96 publications · 7.6K citations

    52

    h-index

  2. Astronomy and Astrophysics

    45 publications · 2.4K citations

    28

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    42 publications · 1.8K citations

    26

    h-index

  4. Science

    23 publications · 4.3K citations

    21

    h-index

  5. The Astronomical Journal

    AJ · 24 publications · 2.1K citations

    20

    h-index

1–5