Angular momenta of collided rarefied preplanetesimals
arXiv:1412.8445 · doi:10.1017/S1743921313013008
Abstract
The angular momenta of rarefied preplanetesimals needed for formation of small-body binaries can be obtained at collisions of preplanetesimals. Trans-Neptunian objects, including trans-Neptunian binaries, could be formed from contracting rarefied preplanetesimals.
arXiv comment4 pages. Proc. IAU Symp. No. 293 "Formation, detection, and characterization of extrasolar habitable planets", ed. by Nader Haghighipour, Proceedings of the International Astronomical Union, vol. 8, Symposium S293, Cambridge University Press. pp. 285-288. (2014)
References in corpus (9)
- Rapid planetesimal formation in turbulent circumstellar discs
- Towards planetesimals: dense chondrule clumps in the protoplanetary nebula
- Formation of Kuiper Belt Binaries by Gravitational Collapse
- Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilities
- On the Size-Dependence of the Inclination Distribution of the Main Kuiper Belt
- Evidence for Two Populations of Classical Transneptunian Objects: The Strong Inclination Dependence of Classical Binaries
- High-resolution simulations of planetesimal formation in turbulent protoplanetary discs
- The Correlated Colors of Transneptunian Binaries
- The angular momentum of two collided rarefied preplanetesimals and the formation of binaries