Kuiper Belt evolution due to dynamical friction

Abstract

In this paper we study the role of dynamical friction on the evolution of a population of large objects ($m>10^{22}$ g) at heliocentric distances $>70$ AU in the Kuiper Belt. We show that the already flat distribution of these objects must flatten further due to non-spherically symmetric distribution of matter in the Kuiper Belt. Moreover the dynamical drag, produced by dynamical friction, causes objects of masses $\ge 10^{24}g$ to lose angular momentum and to fall through more central regions in a timescale $\approx 10^{9}yr$. This mechanism is able to transport inwards objects of the size of Pluto, supposing it was created beyond 50 AU, according to a Stern & Colwell's (1997b) suggestion.

10 pages, 4 encapsulated figures; accepted by A&A