Barycentric Coordinate Systems

Barycentric Coordinate Systems is a reference frame in celestial mechanics that uses the center of mass of a system of bodies, typically the Solar System, as the origin to describe the positions and motions of celestial objects with respect to this common gravitational center.

224

Publications

13.2K

Citations

479

Authors

243

Institutions

Publications per year

2017–2026

43

Variants

Barycentric Reference Systems

Authors

479

  1. KH
    Kai Hormann

    Università della Svizzera italiana, Switzerland

    10 publications · 1.2K citations

    10

    h-index

  2. CG
    Craig Gotsman

    Technion – Israel Institute of Technology, Israel

    8 publications · 763 citations

    8

    h-index

  3. ZL
    Zhiyun Lin

    Zhejiang University, China

    5 publications · 263 citations

    5

    h-index

  4. MS
    Michael S. Floater

    University of Oslo, Norway

    5 publications · 1K citations

    5

    h-index

  5. BH
    Bernd Hamann

    University of California, Davis, United States

    4 publications · 143 citations

    4

    h-index

1–5 of 479

Venues

  1. ACM Transactions on Graphics

    TOG · 13 publications · 1.5K citations

    13

    h-index

  2. Computer Graphics Forum

    14 publications · 658 citations

    12

    h-index

  3. 7

    h-index

  4. Numerische Mathematik

    7 publications · 529 citations

    7

    h-index

  5. Physical Review

    5 publications · 203 citations

    5

    h-index

1–5