The role of pebble fragmentation in planetesimal formation II. Numerical simulations

Research output: Contribution to journalArticle

Abstract

Some scenarios for planetesimal formation go through a phase of collapse of gravitationally bound clouds of millimeter- to centimeter-size pebbles. Such clouds can form, for example, through the streaming instability in protoplanetary disks. We model the collapse process with a statistical model to obtain the internal structure of planetesimals with solid radii between 10 and 1000 km. During the collapse, pebbles collide, and depending on their relative speeds, collisions have different outcomes. A mixture of particle sizes inside a planetesimal leads to better packing capabilities and higher densities. In this paper we apply results from new laboratory experiments of dust aggregate collisions (presented in a companion paper) to model collision outcomes. We find that the internal structure of a planetesimal is strongly dependent on both its mass and the applied fragmentation model. Low-mass planetesimals have no/few fragmenting pebble collisions in the collapse phase and end up as porous pebble piles. The number of fragmenting collisions increases with increasing cloud mass, resulting in wider particle size distributions and higher density. The collapse is nevertheless "cold" in the sense that collision speeds are damped by the high collision frequency. This ensures that a significant fraction of large pebbles survive the collapse in all but the most massive clouds. Our results are in broad agreement with the observed increase in density of Kuiper Belt objects with increasing size, as exemplified by the recent characterization of the highly porous comet 67P/Churyumov-Gerasimenko.

Details

Authors
Organisations
External organisations
  • Technical University of Braunschweig
Research areas and keywords

Subject classification (UKÄ) – MANDATORY

  • Astronomy, Astrophysics and Cosmology

Keywords

  • methods: analytical, methods: numerical, planets and satellites: formation
Original languageEnglish
Article number109
JournalAstrophysical Journal
Volume835
Issue number1
Publication statusPublished - 2017 Jan 20
Publication categoryResearch
Peer-reviewedYes

Related research output

Karl Wahlberg Jansson, 2017 Apr, Lund: Lund University, Faculty of Science, Department of Astronomy and Theoretical Physics. 131 p.

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