Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall

Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall

There is growing evidence that planet formation begins early, within the ≲1 Myr Class 0/I phase, when infall dominates disk dynamics. Our goal is to determine if Class 0/I disks reach the conditions needed to form planetesimals (∼100 km planet building blocks) by the streaming instability (SI). We f...

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Bibliographic Details
Main Authors: Daniel Carrera, Abigail Davenport, Jacob B. Simon, Hans Baehr, Til Birnstiel, Cassandra Hall, David Rea, Sebastian Markus Stammler
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Planet formation
Exoplanet formation
Protoplanetary disks
Online Access:https://doi.org/10.3847/1538-4357/adef46
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https://doi.org/10.3847/1538-4357/adef46

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