Apsidal Alignment Stability
Apsidal Alignment Stability is a theoretical construct in orbital dynamics that denotes the persistence of a fixed angular relationship between the pericenters of two or more gravitationally interacting orbits, ensuring long-term configurational coherence against perturbative torques.
8
Publications
341
Citations
18
Authors
12
Institutions
Publications per year
2017–2026
3
Parents
8
The Apsidal Antialignment of the HD 82943 System
Jianghui Ji, Hiroshi Kinoshita, Lin Liu et al. · Celestial Mechanics and Dynamical Astronomy · 2003 · 56 citations · Full text
1–5 of 8
18
2
h-index
2
h-index
2
h-index
2
h-index
2
h-index
1–5 of 18
12
University of California, Berkeley
Berkeley, United States
2 h-index
2 publications
101 citations

University of Leicester
Leicester, United Kingdom
2 h-index
2 publications
101 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
2 h-index
4 publications
264 citations
National Astronomical Observatories
Beijing, China
2 h-index
5 publications
320 citations
University of California, Santa Barbara
Santa Barbara, United States
2 h-index
2 publications
101 citations
Princeton University
Princeton, United States
2 h-index
2 publications
101 citations
Purple Mountain Observatory
Nanjing, China
2 h-index
4 publications
264 citations

Joint Institute for Laboratory Astrophysics
Boulder, United States
2 h-index
4 publications
202 citations
1–8 of 12
ApJ · 2 publications · 130 citations
2
h-index
2 publications · 48 citations
2
h-index
1 publications · 16 citations
1
h-index
AJ · 1 publications · 44 citations
1
h-index
Repository · 1 publications · 47 citations
1
h-index
1–5