Abstract
Orbit propagation algorithms for satellite relative motion relying on Runge–Kutta integrators are non-symplectic—a situation that leads to incorrect global behavior and degraded accuracy. Thus, attempts have been made to apply symplectic methods to integrate satellite relative motion. However, so far all these symplectic propagation schemes have not taken into account the effect of atmospheric drag. In this paper, drag-generalized symplectic and variational algorithms for satellite relative orbit propagation are developed in different reference frames, and numerical simulations with and without the effect of atmospheric drag are presented. It is also shown that high-order versions of the newly-developed variational and symplectic propagators are more accurate and are significantly faster than Runge–Kutta-based integrators, even in the presence of atmospheric drag.
Original language | English |
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Article number | 31 |
Journal | Celestial Mechanics and Dynamical Astronomy |
Volume | 130 |
Issue number | 4 |
DOIs | |
State | Published - 1 Apr 2018 |
Keywords
- Geometric numerical integration
- Hamiltonian dynamics
- Satellite relative motion
- Symplectic integration
- Variational integration
All Science Journal Classification (ASJC) codes
- Modelling and Simulation
- Mathematical Physics
- Astronomy and Astrophysics
- Space and Planetary Science
- Computational Mathematics
- Applied Mathematics