On the Crystallinity of Silicate Dust in Evolving Protoplanetary Disks due to Magnetically Driven Disk Winds
- 1 October 2021
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 920 (1), 27
- https://doi.org/10.3847/1538-4357/ac157e
Abstract
We present a novel mechanism for the outward transport of crystalline dust particles: the outward radial drift of pebbles. A dust-ring structure is frequently observed in protoplanetary disks. One of the plausible mechanisms for the formation of dust rings is the accumulation of pebbles around the pressure maximum, which is formed by the mass loss due to magnetically driven disk winds. Due to magnetically driven disk winds, dust particles in evolving protoplanetary disks can migrate outwardly from the crystallization front to the pressure maximum by radial drift. We found that the outward radial drift process can transport crystalline dust particles efficiently when the radial drift timescale is shorter than the advection timescale. Our model predicts that the crystallinity of silicate dust particles could be as high as 100% inside the dust-ring position.Funding Information
- MEXT ∣ Japan Society for the Promotion of Science (JP20J00598)
- MEXT ∣ Japan Society for the Promotion of Science (JP17H01103)
- MEXT ∣ Japan Society for the Promotion of Science (JP18H05441)
This publication has 71 references indexed in Scilit:
- The effects of disk building on the distributions of refractory materials in the solar nebulaMeteoritics & Planetary Science, 2012
- The distributions and ages of refractory objects in the solar nebulaIcarus, 2010
- FORMATION OF COSMIC CRYSTALS IN HIGHLY SUPERSATURATED SILICATE VAPOR PRODUCED BY PLANETESIMAL BOW SHOCKSThe Astrophysical Journal, 2010
- Two-dimensional transport of solids in viscous protoplanetary disksIcarus, 2009
- DISK WINDS DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND DISPERSAL OF PROTOPLANETARY DISKSThe Astrophysical Journal, 2009
- Dust crystallinity in protoplanetary disks: the effect of diffusion/viscosity ratioAstronomy & Astrophysics, 2007
- Crystalline Silicates as a Probe of Disk Formation HistoryThe Astrophysical Journal, 2006
- Dust Diffusion in Protoplanetary Disks by Magnetorotational TurbulenceThe Astrophysical Journal, 2005
- Evolving Optical Properties of Annealing Silicate Grains: From Amorphous Condensate to Crystalline MineralThe Astrophysical Journal, 2000
- Accretion and the Evolution of T Tauri DisksThe Astrophysical Journal, 1998