Analytical and Numerical Estimates for Solar Radiation Pressure Semi-secular Resonances
Roberto Paoli

TL;DR
This paper provides analytical and numerical estimates of solar radiation pressure-induced resonances affecting objects with high area-to-mass ratios, including their locations, amplitudes, and dynamics, validated through phase space analysis.
Contribution
It introduces new analytical formulas for resonance locations and amplitudes, and validates these estimates with numerical tools like FLI maps and bifurcation diagrams.
Findings
Resonance locations can be estimated analytically.
Maximum eccentricity variation amplitudes are derived.
Numerical validation confirms the analytical estimates.
Abstract
The aim of this work is to provide new insights on the dynamics associated to the resonances which arise as a consequence of the coupling of the effect due to the oblateness of the Earth and the Solar Radiation Pressure (SRP) effect for an uncontrolled object with moderate to high area-to-mass ratio. Analytical estimates for the location of the resulting resonant equilibrium points are provided, together with formulas to compute the maximum amplitude of the corresponding variation in the eccentricity, as a function of the initial conditions of the object and of its area-to-mass ratio. The period of the variations of the eccentricity and inclinations due to such resonances is estimated using classical formulas. A classification based on the strength of the SRP resonances is provided. The estimates presented in the paper are validated using numerical tools, including the use of Fast…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsMagnetic and Electromagnetic Effects · Solar and Space Plasma Dynamics · Astrophysics and Star Formation Studies
