Cometary Ice Composition

Cometary Ice Composition is a scientific construct that specifies the relative abundances and chemical identities of volatile ices, primarily composed of water, carbon dioxide, carbon monoxide, methane, and other organic and inorganic molecules, preserved within the nucleus of a comet and reflective of the conditions of the early solar nebula.

277

Publications

18.4K

Citations

1.1K

Authors

384

Institutions

Publications per year

2017–2026

58

Authors

1.1K

  1. DB
    D. Bockelée–Morvan

    Observatoire de Paris, France

    23 publications · 2.5K citations

    22

    h-index

  2. MF
    Michael F. A’Hearn

    University of Maryland, College Park, United States

    24 publications · 1.9K citations

    22

    h-index

  3. OG
    O. Groussin

    Laboratoire d’Astrophysique de Marseille, France

    19 publications · 1.4K citations

    18

    h-index

  4. NB
    N. Biver

    Observatoire de Paris, France

    17 publications · 2.2K citations

    17

    h-index

  5. LJ
    L. Jordá

    Laboratoire d’Astrophysique de Marseille, France

    16 publications · 1.3K citations

    16

    h-index

1–5 of 1.1K

Venues

  1. Icarus

    47 publications · 2.7K citations

    32

    h-index

  2. The Astrophysical Journal

    ApJ · 39 publications · 3.2K citations

    28

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    33 publications · 1.8K citations

    22

    h-index

  4. Astronomy and Astrophysics

    21 publications · 1.4K citations

    19

    h-index

  5. Science

    17 publications · 3.1K citations

    17

    h-index

1–5