Cometary Nucleus Composition

Cometary Nucleus Composition is a scientific construct that characterizes the physical and chemical makeup of the solid core of a comet, distinguishing it from other cometary features by specifying the proportions and identities of ices, refractory materials, organic compounds, and dust within the nucleus.

544

Publications

30.4K

Citations

1.6K

Authors

472

Institutions

Publications per year

2017–2026

71

Authors

1.6K

  1. MF
    Michael F. A’Hearn

    University of Maryland, College Park, United States

    48 publications · 3K citations

    33

    h-index

  2. HU
    H. U. Keller

    Max Planck Institute for Solar System Research, Germany

    28 publications · 2.3K citations

    24

    h-index

  3. PL
    P. Lamy

    Laboratoire d’Astrophysique de Marseille, France

    28 publications · 2.1K citations

    24

    h-index

  4. MR
    M. R. Combi

    University of Michigan, United States

    30 publications · 2.8K citations

    24

    h-index

  5. DB
    D. Bockelée–Morvan

    Observatoire de Paris, France

    31 publications · 2.3K citations

    24

    h-index

1–5 of 1.6K

Venues

  1. Icarus

    89 publications · 5.1K citations

    46

    h-index

  2. The Astrophysical Journal

    ApJ · 65 publications · 3.7K citations

    34

    h-index

  3. Astronomy and Astrophysics

    52 publications · 3.1K citations

    31

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    40 publications · 1.9K citations

    27

    h-index

  5. Science

    28 publications · 4.3K citations

    26

    h-index

1–5