Issue |
A&A
Volume 696, April 2025
|
|
---|---|---|
Article Number | L23 | |
Number of page(s) | 7 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/202554100 | |
Published online | 29 April 2025 |
Letter to the Editor
Positive feedback: How a synergy between the streaming instability and dust coagulation forms planetesimals
1
New Mexico State University, Department of Astronomy, PO Box 30001 MSC 4500 Las Cruces, NM 88001, USA
2
Department of Physics and Astronomy, Iowa State University, Ames, IA 50010, USA
3
Institute for Advanced Computational Sciences, Stony Brook University, Stony Brook, NY 11794-5250, USA
4
Department of Astrophysics, American Museum of Natural History, 200 Central Park West, New York, NY 10024, USA
⋆ Corresponding author: carrera4@nmsu.edu
Received:
11
February
2025
Accepted:
4
April
2025
Context. One of the most important open questions in planet formation is how dust grains in a protoplanetary disk manage to overcome growth barriers and form the ∼100 km planet building blocks that we call planetesimals. There appears to be a gap between the largest grains that can be produce by coagulation, and the smallest grains that are needed for the streaming instability (SI) to form planetesimals.
Aims. Here we explore the novel hypothesis that dust coagulation and the SI work in tandem; in other words, they form a feedback loop where each one boosts the action of the other to bridge the gap between dust grains and planetesimals.
Methods. We developed a semi-analytical model of dust concentration due to the SI, and an analytic model of how the SI affects the fragmentation and radial drift barriers. We then combined them to model our proposed feedback loop.
Results. In the fragmentation-limited regime, we find a powerful synergy between the SI and dust growth that drastically increases both grain sizes and densities. We find that a midplane dust-to-gas ratio of ϵ ≥ 0.3 is a sufficient condition for the feedback loop to reach the planetesimal-forming region for turbulence values 10−4 ≤ α ≤ 10−3 and grain sizes 0.01 ≤ St ≤ 0.1. In contrast, the drift-limited regime only shows grain growth without significant dust accumulation. In other words, planetesimal formation remains challenging in the drift-dominated regime and dust traps may be required to allow planet formation at wide orbital distances.
Key words: planets and satellites: formation
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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