Born-big TNOs and the shallow size distribution of faint objects in the Edgeworth-Kuiper belt

Details Born-big TNOs and the shallow size distribution of faint objects in the Edgeworth-Kuiper belt Born-big TNOs and the shallow size distribution of faint objects in the Edgeworth-Kuiper belt

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..601c&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.601

Physics

Scientific paper

ALICANDEP (Asteroid-LIke Collisional ANd Dynamical Evolution Package) is a collisional evolution code [1] including a) statistical elimination of objects by dynamical effects within the frame of a disc that migrates and is excited dynamically, and b) the dynamical migration of objects within the disc itself, as described by the Nice model [2]. The model meets the Nice model requirements and matches available current observables (the existence of Pluto and the rest of dwarf planets in the region; the number of objects larger than 100 km in different dynamical populations and the corresponding size distributions, as found by the Canadian France Ecliptic Plane Survey, CFEPS [3,4])

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