The evolution of bodies orbiting in the trans-Neptunian region on to intermediate-type orbits

Details The evolution of bodies orbiting in the trans-Neptunian region on to intermediate-type orbits The evolution of bodies orbiting in the trans-Neptunian region on to intermediate-type orbits

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mnras.318..482m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 318, Issue 2, pp. 482-492.

Astronomy and Astrophysics

Astronomy

4

Celestial Mechanics, Stellar Dynamics, Minor Planets, Asteroids, Planets And Satellites: General

Scientific paper

We investigate the dynamical evolution of 210 hypothetical massless bodies initially situated between 10 and 30au from the Sun in order to determine the general characteristics of the evolved system. This is of particular relevance to the understanding of the origin of Edgeworth-Kuiper belt objects on scattered intermediate orbits, such as 1996TL66, which have high eccentricity and semimajor axis but nevertheless have perihelion in the region between 30 and 50au from the Sun.

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