Annotation
This paper discusses patterns in the distribution of Centaurs, scattered disks, and Kuiper belt objects according to the semi-major axes, eccentricities and inclinations of their orbits. Over half of them are found to move in resonant orbits and these were predicted earlier. An interpretation is given for the divergence of the maximum in the observed semi-major axis distribution with an exact orbital resonance determined within the classical three-body problem.
Received: 2009 July 8
Approved: 2010 May 28
PACS:
96.30.Xa Kuiper belt, trans-Neptunian objects
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
B.R. Mushailov, V.S. Teplitskaya
Astrometry Department, Sternberg Astronomical Institute, Moscow State University, Universitetskii pr., Moscow, 119992, Russia
Astrometry Department, Sternberg Astronomical Institute, Moscow State University, Universitetskii pr., Moscow, 119992, Russia