Retrograde Orbits
Retrograde Orbits is an orbital configuration in which a satellite or celestial body revolves around its primary in the opposite direction to the primary's rotation, distinguished from prograde orbits by its negative orbital inclination relative to the equatorial plane.
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9.5K
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583
Authors
315
Institutions
Publications per year
2017–2026
64
Variants
Retrograde Orbit
Parents
213
Vasily Belokurov, Jason L. Sanders, Azadeh Fattahi et al. · Monthly Notices of the Royal Astronomical Society · 2020 · 286 citations · Full text
Natural Sciences, Astronomy, Physics +17
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California Institute of Technology
Pasadena, United States
11 h-index
28 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
24 publications
2.4K citations
University of Colorado Boulder
Boulder, United States
9 h-index
14 publications
375 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
28 publications
2.3K citations
University of Cambridge
Cambridge, United Kingdom
8 h-index
11 publications
1.1K citations
Universidade Estadual Paulista (Unesp)
São Paulo, Brazil
8 h-index
15 publications
969 citations
University of Geneva
Geneva, Switzerland
8 h-index
42 publications
3.6K citations

Australian National University
Canberra, Australia
7 h-index
12 publications
871 citations
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45 publications · 2.8K citations
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ApJ · 23 publications · 1.6K citations
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AJ · 24 publications · 907 citations
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14 publications · 544 citations
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11 publications · 605 citations
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