The triaxiality role in the spin-orbit dynamics of a rigid body
From MaRDI portal
Publication:2690583
DOI10.21042/AMNS.2018.1.00015OpenAlexW2896055932WikidataQ129063800 ScholiaQ129063800MaRDI QIDQ2690583
Francisco Crespo, A. Cantero, Sebastián Ferrer
Publication date: 17 March 2023
Published in: Applied Mathematics and Nonlinear Sciences (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.21042/amns.2018.1.00015
Related Items (3)
Poisson Structure and Reduction by Stages of the Full Gravitational $N$-Body Problem ⋮ Study of the roto-orbital motion using intermediaries: numerical experiments ⋮ Hamiltonian structure, equilibria, and stability for an axisymmetric gyrostat motion in the presence of gravity and magnetic fields
Cites Work
- Unnamed Item
- Unnamed Item
- The Hill--Brown theory of the Moon's motion. Its coming-to-be and short-lived ascendancy (1877-1984)
- Attitude stability of artificial satellites subject to gravity gradient torque
- Elimination of the nodes when the satellite is a non spherical rigid body
- Integrable approximation of \(J_2\)-perturbed relative orbits
- Minimum energy configurations in the \(N\)-body problem and the celestial mechanics of granular systems
- Andoyer's variables and phases in the free rigid body
- Elimination of the nodes in problems ofn bodies
- The elimination of the parallax in satellite theory
- Generic bifurcation of Hamiltonian vector fields with symmetry
- Extrapolation methods and derivatives of limits of sequences
- Explicit expansion of the three-body disturbing function for arbitrary eccentricities and inclinations
- On the motion of a satellite about its center of mass under the action of gravitational moments
- Effects of gravity-gradient torque on the rotational motion of A triaxial satellite in a precessing elliptic orbit
This page was built for publication: The triaxiality role in the spin-orbit dynamics of a rigid body
