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Problems and Prospects in Planetesimal Formation

Published online by Cambridge University Press:  06 January 2014

Eugene Chiang ,
Ruth Murray-Clay  and
Ji-Ming Shi
Eugene Chiang
Affiliation:
Department of Astronomy, UC Berkeley Hearst Field Annex B-20, Berkeley CA 94720, USA email: echiang@astro.berkeley.edu, jmshi@berkeley.edu
Ruth Murray-Clay
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge MA 02138, USA email: rmurray-clay@cfa.harvard.edu
Ji-Ming Shi
Affiliation:
Department of Astronomy, UC Berkeley Hearst Field Annex B-20, Berkeley CA 94720, USA email: echiang@astro.berkeley.edu, jmshi@berkeley.edu
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Abstract

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On the long road from dust to planets there are planetesimals. We review and criticize proposed mechanisms for planetesimal formation, and point out topics for future work.

Keywords

planets and satellites: formationsolar system: formationinstabilitiesturbulenceKuiper Beltminor planetsasteroidsaccretionaccretion disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 136 - 139
Copyright
Copyright © International Astronomical Union 2013 

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