Dynamical Behaviour of Centaurus-Type Objects

Details Dynamical Behaviour of Centaurus-Type Objects Dynamical Behaviour of Centaurus-Type Objects

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26q.154l&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have analyzed the dynamical behavior of objects located in a position 22 < a < 26 AU which corresponds to the mean motion resonances 3:2 and 2:3 with Neptune and Uranus respectively. Mostly of the studied objects migrant toward the external part of the Solar System. Some of them are ejected from the Solar System with a great e. Of the test particles studied less than 10 cases becoming Earth and Mars crossers. Many objects make numerous close approaches to Jupiter and Saturn. Other clones, a few, can reach the region a approx 500 AU, e approx 0.78, i approx 15° like Sedna. This behavior of some clones occur when Neptune has a = 28 AU.

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