Periapsis Precession is the gradual rotation of the line of apsides in a Keplerian orbit due to perturbations in a two-body orbital system, manifesting as a continuous shift in the position of closest approach between the orbiting bodies over successive revolutions.
12
Publications
612
Citations
32
Authors
22
Institutions
Publications per year
2017–2026
6
Publications
12
1–5 of 12
Authors
32
- KI
1
h-index
- AS
1
h-index
- KN
1
h-index
- JR
1
h-index
- WL
1
h-index
1–5 of 32
Institutions
22
Canadian Institute for Theoretical Astrophysics
Toronto, Canada
2 h-index
2 publications
87 citations
California Institute of Technology
Pasadena, United States
2 h-index
3 publications
364 citations
Jet Propulsion Laboratory
Pasadena, United States
2 h-index
2 publications
34 citations
United States Air Force Research Laboratory
Wright-Patterson AFB, United States
1 h-index
1 publications
20 citations
Universidad Politécnica de Madrid
Madrid, Spain
1 h-index
4 publications
56 citations
University of Colorado Boulder
Boulder, United States
1 h-index
2 publications
40 citations
Toyota Technological Institute
Nagoya, Japan
1 h-index
3 publications
39 citations
Rikkyo University
Tokyo, Japan
1 h-index
1 publications
18 citations
1–8 of 22
Venues
- Monthly Notices of the Royal Astronomical Society
4 publications · 344 citations
4
h-index
- Physical review. D/Physical review. D.
PRD · 2 publications · 31 citations
2
h-index
- Classical and Quantum Gravity
1 publications · 101 citations
1
h-index
- Journal of Guidance Control and Dynamics
1 publications · 20 citations
1
h-index
- Celestial Mechanics and Dynamical Astronomy
1 publications · 14 citations
1
h-index
1–5