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The Plane of the Kuiper Belt

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© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Michael E. Brown and Margaret Pan 2004 AJ 127 2418 DOI 10.1086/382515

1538-3881/127/4/2418

Abstract

We present a robust method for measuring the effective plane of the Kuiper belt. The derived plane has an inclination with respect to the ecliptic of 1fdg86 and an ascending node of 81fdg6, with a 1 σ error in pole position of the plane of 0fdg37. The plane of the Kuiper belt is inconsistent with the invariable plane, the plane of Jupiter, and the plane of Neptune at the greater than 3 σ level. Using linear secular perturbation theory, we show that the plane of the Kuiper belt is expected to oscillate about the position of the invariable plane with a period of 1.9 million years and an amplitude of 1fdg2. The present predicted position of the plane of the Kuiper belt has an inclination with respect to the ecliptic of 1fdg74 and an ascending node of 86fdg7, within 0fdg20 of our measured position.

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10.1086/382515