Orbital Energy

Orbital Energy is the total mechanical energy of a celestial body in a Keplerian orbit, defined as the sum of its kinetic and gravitational potential energies, which remains constant in the absence of non-conservative forces.

542

Publications

37.7K

Citations

1.7K

Authors

733

Institutions

Publications per year

2017–2026

109

Authors

1.7K

  1. EJ
    Evert Jan Baerends

    Vrije Universiteit Amsterdam, Netherlands

    8 publications · 983 citations

    8

    h-index

  2. TT
    Takao Tsuneda

    The University of Tokyo, Japan

    6 publications · 680 citations

    6

    h-index

  3. JP
    John P. Perdew

    Tulane University, United States

    6 publications · 4.2K citations

    6

    h-index

  4. GE
    G. E. Becker

    Stanford University, United States

    5 publications · 467 citations

    5

    h-index

  5. GF
    Gernot Frenking

    Philipps University of Marburg, Germany

    5 publications · 238 citations

    5

    h-index

1–5 of 1.7K

Venues

  1. The Journal of Chemical Physics

    63 publications · 5.4K citations

    35

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    34 publications · 2.2K citations

    25

    h-index

  3. The Astrophysical Journal

    ApJ · 29 publications · 1.9K citations

    23

    h-index

  4. Journal of Chemical Theory and Computation

    JCTC · 13 publications · 1.1K citations

    13

    h-index

  5. Molecular Physics

    14 publications · 815 citations

    12

    h-index

1–5