Orbital Dynamics about a Slowly Rotating Asteroid

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We analyze orbital stability of satellites (moon, spacecraft) about a slowly rotating axisymmetric asteroid. We consider both orbits lying in and transverse to the plane of rotation. Using simple point mass models as a guide, we discover an unstable region near the equatorial plane of an indented body. The existence of stable/unstable regions is confirmed numerically for a realistic ``peanut" model asteroid. The stable region is found to survive modest asteroid rotation about an axis of maximum moment of inertia.

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