Phil Armitage : Planetesimal formation as the key to planetary system architecture?

Quand :
26 juin 2017 @ 11 h 00 min – 12 h 00 min
2017-06-26T11:00:00+02:00
2017-06-26T12:00:00+02:00
Où :
Univers 21
33600 Pessac
France

The first gravitationally bound bodies to form in protoplanetary disks, the 1-100 km sized planetesimals, are a key intermediate step in planet formation. After decades of uncertainty, at least one viable path to planetesimal fomation – based on radial drift of small solid particles, the streaming instability, and gravitational collapse – has now been securely established. I will discuss numerical simulations of planetesimal formation, and their (speculative) implications for planetary system architecture. I will argue that the somewhat restrictive conditions for planetesimal formation constitute a key bottleneck in the planet formation process, that can link variable disk properties to the architecture of resulting planetary systems.