The CO snow line favours strong clumping by the streaming instability in protoplanetary discs with porous grains
Jean-Fran\c{c}ois Gonzalez, St\'ephane Michoulier

TL;DR
This study shows that the presence of the CO snow line in protoplanetary discs with porous grains significantly enhances conditions for streaming instability-driven clumping, aiding planetesimal formation within the first hundred thousand years.
Contribution
It demonstrates that the CO snow line promotes strong clumping via streaming instability in porous grain discs, a novel insight into planetesimal formation conditions.
Findings
Strong clumping occurs within 100,000 years near the CO snow line.
Neglecting the CO snow line delays or reduces clumping regions.
Porous grains facilitate conditions favorable for streaming instability.
Abstract
Context: The radial drift and fragmentation of small dust grains in protoplanetary discs impedes their growth past centimetre sizes. Several mechanisms have been proposed to overcome these planet formation barriers, such as dust porosity or the streaming instability (SI), which is today regarded as the most promising mechanism to form planetesimals. Aims: Here, we examine whether the conditions for the SI to lead to strong clumping, the first step in planetesimal formation, are realised in protoplanetary discs containing porous grains. Methods: We used results from previous simulations of the evolution of porous grains subjected to growth, fragmentation, compaction and bouncing in protoplanetary discs. In the ensuing disc structures, we determined the regions where the dust-to-gas ratio exceeds the critical value for strong clumping found in simulations of the SI including external…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
