Perihelion precession in power-law potentials: Hénon's theorem

Author:

Dmitrašinović V.1,Janković Marija R.2

Affiliation:

1. Institute of Physics, Belgrade University, Pregrevica 118, Zemun, P.O. Box 57, 11080 Beograd, Serbia

2. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom

Abstract

In 1977, Michel Hénon proved a remarkable theorem for planar N-body orbits in power-law potentials that relates the rate of change of the perihelion angle (the precession rate), the rate of change of the period evaluated at constant energy, the angular momentum of an orbit, and the power law of the potential. We provide a simple proof of this theorem for two bodies in periodic orbits that interact via a radial power-law force, which is, of course, equivalent to a one-body problem with a power-law central potential. We discuss this theorem's underlying assumptions and implications, including its relation to Bertrand's and Bohlin's theorems, and we illustrate it with several numerically calculated examples.

Funder

Science Fund of the Republic of Serbia

Publisher

American Association of Physics Teachers (AAPT)

Subject

General Physics and Astronomy

Reference31 articles.

1. A relation in families of periodic solutions

2. “Power-law” and “homogeneous” are synonyms in the context of one- and two-body problems, as there is only one distance variable involved. That is not the case anymore as the number of bodies increases.

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