Abstract
The mathematical model used in orbit determination problems must be as close to the actual dynamics as possible. On the contrary, accuracy constraints can be notably relaxed for orbit prediction purposes. For the latter, it is important to determine which is the simplified dynamical model that, while retaining the bulk of the dynamics, allow for faster predictions. Methods for doing that are commonly heuristic. We focus on perturbed Keplerian motion and explore how to ascertain the correct truncation of the dynamical model required in orbit prediction problems by investigating relevant particular solutions of the orbital motion: the so-called frozen orbits.
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Notes
- 1.
I do not discuss the case of other frozen orbits that may exist with gā āĀ±āĻ/2.
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Acknowledgements
The author acknowledges partial support by the Spanish State Research Agency and the European Regional Development Fund under Projects ESP2013-41634-P, ESP2014-57071-R and ESP2016-76585-R (AEI/ERDF, EU). Discussions with Hodei Urrutxua, University of Southampton, are acknowledged.
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Lara, M. (2018). Exploring Sensitivity of Orbital Dynamics with Respect to Model Truncation: The Frozen Orbits Approach. In: Vasile, M., Minisci, E., Summerer, L., McGinty, P. (eds) Stardust Final Conference. Astrophysics and Space Science Proceedings, vol 52. Springer, Cham. https://doi.org/10.1007/978-3-319-69956-1_4
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