Restricted Three-body Problem

The Restricted Three-Body Problem is a specialized case of the three-body problem in celestial mechanics in which one of the three masses is assumed to be negligibly small compared to the other two, such that it does not influence the motion of the larger bodies, which follow Keplerian orbits about their common center of mass.

1.3K

Publications

53.5K

Citations

1.6K

Authors

728

Institutions

Publications per year

2017–2026

167

Authors

1.6K

  1. JS
    Jagadish Singh

    Ahmadu Bello University, Nigeria

    40 publications · 1.3K citations

    22

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  2. EI
    Elbaz I. Abouelmagd

    National Research Institute of Astronomy and Geophysics, Egypt

    25 publications · 1.2K citations

    21

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  3. BI
    B. Ishwar

    Babasaheb Bhimrao Ambedkar Bihar University, India

    16 publications · 482 citations

    14

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  4. EA
    E. A. Perdios

    University of Patras, Greece

    18 publications · 452 citations

    14

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  5. CR
    Colin R. McInnes

    University of Strathclyde, United Kingdom

    14 publications · 786 citations

    13

    h-index

1–5 of 1.6K

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    177 publications · 6.9K citations

    44

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  2. Astrophysics and Space Science

    95 publications · 3.1K citations

    33

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  3. Journal of Guidance Control and Dynamics

    51 publications · 2.4K citations

    29

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  4. 28

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  5. The Astronomical Journal

    AJ · 69 publications · 3.2K citations

    27

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