Keplerian Motion
Keplerian Motion is the idealized two-body orbital motion of a celestial object governed solely by Newtonian gravitation, where the trajectory follows one of Kepler’s laws of planetary motion.
1K
Publications
60.1K
Citations
1.8K
Authors
783
Institutions
Publications per year
2017–2026
107
1K
Gravitational Radiation from Point Masses in a Keplerian Orbit
P. C. Peters, Jon Mathews · Physical Review · 1963 · 1.6K citations
Natural Sciences, Astronomy, Physics +17
A terrestrial planet candidate in a temperate orbit around Proxima Centauri
G. Anglada‐Escudé, P. J. Amado, J. R. Barnes et al. · Nature · 2016 · 1.3K citations · Full text
Natural Sciences, Astronomy, Physics +11
1–5 of 1K
1.8K
18
h-index
18
h-index
18
h-index
18
h-index
17
h-index
1–5 of 1.8K
783

Centre National de la Recherche Scientifique
Paris, France
35 h-index
287 publications
19.7K citations
Institut d'Astrophysique de Paris
Paris, France
26 h-index
73 publications
5.7K citations

Ames Research Center
Mountain View, United States
26 h-index
165 publications
29.3K citations
California Institute of Technology
Pasadena, United States
23 h-index
36 publications
6.5K citations
University of California, Berkeley
Berkeley, United States
21 h-index
45 publications
7.2K citations
University of California, Santa Cruz
Santa Cruz, United States
21 h-index
40 publications
7.5K citations
University of Geneva
Geneva, Switzerland
21 h-index
73 publications
10.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
19 h-index
94 publications
18.2K citations
1–8 of 783
ApJ · 57 publications · 6.3K citations
40
h-index
57 publications · 3.1K citations
32
h-index
84 publications · 2.7K citations
29
h-index
34 publications · 2.6K citations
28
h-index
51 publications · 3.5K citations
26
h-index
1–5