Circular Restricted Three-body Problem

The Circular Restricted Three-Body Problem is a specialized case of the three-body problem in celestial mechanics in which two massive bodies follow circular orbits around their common center of mass under mutual gravitational attraction, while a third body of negligible mass moves under their influence without perturbing their motion.

195

Publications

6.3K

Citations

284

Authors

174

Institutions

Publications per year

2017–2026

51

Authors

284

  1. CR
    Colin R. McInnes

    University of Strathclyde, United Kingdom

    6 publications · 273 citations

    6

    h-index

  2. JS
    Jagadish Singh

    Ahmadu Bello University, Nigeria

    6 publications · 123 citations

    6

    h-index

  3. AA
    Abdullah A. Ansari

    Majmaah University, Saudi Arabia

    6 publications · 84 citations

    6

    h-index

  4. KE
    K. E. Papadakis

    University of Patras, Greece

    4 publications · 142 citations

    5

    h-index

  5. KC
    Kathleen C. Howell

    Purdue University West Lafayette, United States

    5 publications · 113 citations

    5

    h-index

1–5 of 284

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    31 publications · 928 citations

    20

    h-index

  2. Journal of Guidance Control and Dynamics

    16 publications · 695 citations

    15

    h-index

  3. The Astronomical Journal

    AJ · 10 publications · 764 citations

    10

    h-index

  4. Astrophysics and Space Science

    9 publications · 375 citations

    9

    h-index

  5. 7

    h-index

1–5