Snow Line Evolution

Snow Line Evolution is a theoretical construct in planetary science that denotes the time-dependent migration of the radial distance in a protoplanetary disk beyond which volatile compounds such as water, ammonia, and methane can condense into solid ice grains, distinguishing it from static snow line models by incorporating dynamical changes due to disk cooling, accretion, and stellar radiation.

72

Publications

5.7K

Citations

231

Authors

155

Institutions

Publications per year

2017–2026

21

Authors

231

  1. SH
    Stefan Hastenrath

    University of Wisconsin–Madison, United States

    5 publications · 154 citations

    5

    h-index

  2. SO
    Satoshi Okuzumi

    Tokyo Institute of Technology, Japan

    4 publications · 269 citations

    4

    h-index

  3. SI
    Shigeru Ida

    Tokyo Institute of Technology, Japan

    3 publications · 498 citations

    3

    h-index

  4. SK
    Steven K. Baum

    Texas A&M University, United States

    2 publications · 87 citations

    2

    h-index

  5. RH
    Ryuki Hyodo

    Life Science Institute, Japan

    2 publications · 46 citations

    2

    h-index

1–5 of 231

Venues

  1. The Astrophysical Journal

    ApJ · 15 publications · 2K citations

    15

    h-index

  2. Astronomy and Astrophysics

    9 publications · 784 citations

    9

    h-index

  3. Journal of Glaciology

    5 publications · 150 citations

    5

    h-index

  4. 3

    h-index

  5. Science

    2 publications · 100 citations

    2

    h-index

1–5