Planetary motion in Alpha Centauri

Details Planetary motion in Alpha Centauri Planetary motion in Alpha Centauri

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jansc..35..359h&link_type=abstract

Journal of the Astronautical Sciences (ISSN 0021-9142), vol. 35, July-Sept. 1987, p. 359-361; Author's Reply, p. 363-365.

Astronomy and Astrophysics

Astronomy

A Stars, Binary Stars, Extrasolar Planets, Planetary Orbits, Centaurus Constellation, Eccentric Orbits, Three Body Problem

Scientific paper

Numerical simulation of the orbit of a planet revolving about Alpha
Centauri A at a distance to produce earth-like temperatures show that
the eccentricity is periodic with a period of about 8000 years and an
amplitude of just under 0.1. Hence, the orbit appears to be dynamically
stable.

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