Erosion and the limits to planetesimal growth

Context. The coagulation of microscopic dust into planetesimals is the first step towards the formation of planets. The composition, size, and shape of the growing aggregates determine the efficiency of this early growth. In particular, it has been proposed that fluffy ice aggregates can grow very e...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2015-02, Vol.574, p.A83
Hauptverfasser:	Krijt, S., Ormel, C. W., Dominik, C., Tielens, A. G. G. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aggregates Barriers Bouncing circumstellar matter Collisions Drift Erosion control methods: numerical Monte Carlo methods Planet formation planets and satellites: formation protoplanetary disks
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