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arXiv · 2202.13891

Dust resurgence in protoplanetary disks due to planetesimal-planet interactions

Lia Marta Bernabò·Diego Turrini·Leonardo Testi·Francesco Marzari·Danai Polychroni
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Abstract

Observational data on the dust content of circumstellar disks show that the median dust content in disks around pre-main sequence stars in nearby star forming regions seem to increase from about 1 Myr to about 2 Myr, and then decline with time. This behaviour challenges the models where the small dust grains steadily decline by accumulating into larger bodies and drifting inwards on a short timescale (less than about 1 Myr). In this Letter we explore the possibility to reconcile this discrepancy in the framework of a model where the early formation of planets dynamically stirs the nearby planetesimals and causes high energy impacts between them, resulting in the production of second-generation dust. We show that the observed dust evolution can be naturally explained by this process within a suite of representative disk-planet architectures.

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Lia Marta Bernabò, Diego Turrini, Leonardo Testi, Francesco Marzari, Danai Polychroni. 2022-02-28. Dust resurgence in protoplanetary disks due to planetesimal-planet interactions. https://arxiv.org/abs/2202.13891

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