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Co-Orbital Motion with Slowly Varying Parameters

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Abstract

We consider the dynamics of a test particle co-orbital with a satellite of mass m s which revolves around a planet of mass M 0m s with a mean motion n s and semi-major axis a s. We study the long term evolution of the particle motion under slow variations of (1) the mass of the primary, M 0, (2) the mass of the satellite, m s and (3) the specific angular momentum of the satellite J s. The particle is not restricted to small harmonic oscillations near L 4 or L 5, and may have any libration amplitude on tadpole or horseshoe orbits. In a first step, no torque is applied to the particle, so that its motion is described by a Hamiltonian with slowly varying parameters. We show that the torque applied to the satellite, as measured by ∈s = js/(n s J s) induces an distortion of the phase space which is entirely described by an asymmetry coefficient α = ∈s/μ, where μ = m s/M. The adiabatic invariance of action implies furthermore that the long term evolution of the particle co-orbital motion depends only on the variation of m s a s with time. Applying a constant torque to the particle, as measured by ∈s = js/(n s J p) is then merely equivalent to replacing α = ∈s/μ by α = (∈s − ∈p)/μ. However, if the torque acting on the particle exhibits a radial gradient, then the action is no more conserved and the evolution of the particle orbit is no more controlled by m s a s only. We show that even mild torque gradients can dominate the orbital evolution of the particle, and eventually decide whether the latter will be pulled towards the stable equilibrium points L 4 or L 5, or driven away from them. Finally, we show that when the co-orbital bodies are two satellites with comparable masses m 1 and m 2, we can reduce the problem to that of a test particle co-orbital with a satellite of mass m 1 + m 2. This new problem has then parameters varying at rates which are combinations, with appropriate coefficients, of the changes suffered by each satellite.

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Sicardy, B., Dubois, V. Co-Orbital Motion with Slowly Varying Parameters. Celestial Mechanics and Dynamical Astronomy 86, 321–350 (2003). https://doi.org/10.1023/A:1024579912307

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  • DOI: https://doi.org/10.1023/A:1024579912307

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