Dust Coagulation in the Vicinity of a Gap-Opening Jupiter-Mass Planet
arXiv:1512.03945 · doi:10.3847/0004-637X/823/2/80
Abstract
We analyze the coagulation of dust in and around a gap opened by a Jupiter-mass planet. To this end, we carry out a high-resolution magnetohydrodynamic (MHD) simulation of the gap environment, which is turbulent due to the magnetorotational instability. From the MHD simulation, we obtain values of the gas velocities, densities and turbulent stresses a) close to the gap edge, b) in one of the two gas streams that accrete onto the planet, c) inside the low-density gap, and d) outside the gap. The MHD values are then supplied to a Monte Carlo dust coagulation algorithm, which models grain sticking and compaction. We consider two dust populations for each region: one whose initial size distribution is monodisperse, with monomer radius equal to 1 m, and another one whose initial size distribution follows the Mathis-Rumpl-Nordsieck distribution for interstellar dust grains, with an initial range of monomer radii between 0.5 and 10 m. Our Monte Carlo calculations show initial growth of dust aggregates followed by compaction in all cases but one, that of aggregates belonging to the initially monodisperse population subject to gas conditions outside the gap. In this latter case, the mass-weighted (MW) average porosity of the population reaches extremely high final values of 98\%. The final MW porosities in all other cases range between 30\% and 82\%. The efficiency of compaction is due to high turbulent relative speeds between dust particles. Future studies will need to explore the effect of different planet masses and electric charge on grains.
5 pages, 4 figures. Submitted to ApJL
References in corpus (16)
- First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region
- Athena: A New Code for Astrophysical MHD
- Dust and Gas in the disc of HL Tauri: Surface density, dust settling, and dust-to-gas ratio
- Dust size distributions in coagulation/fragmentation equilibrium: Numerical solutions and analytical fits
- Dust coagulation in protoplanetary disks: porosity matters
- An Atmospheric Structure Equation for Grain Growth
- Dust Trapping by Vortices in Transitional Disks: Evidence for Non-ideal MHD Effects in Protoplanetary Disks
- ALMA images of discs: are all gaps carved by planets?
- Dust accretion onto high-mass planets
- Co-Accretion of Chondrules and Dust in the Solar Nebula
- The effect of a planet on the dust distribution in a 3D protoplanetary disk
- Charging of Aggregate Grains in Astrophysical Environments
- The accumulation and trapping of grains at planet gaps: effects of grain growth and fragmentation
- How do giant planetary cores shape the dust disk? HL Tau system
- Accreting planets as dust dams in `transition' discs
- Magnetic fields in gaps surrounding giant protoplanets
Cited by in corpus (3)
- Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
- Three-dimensional Global Simulations of Type-II Planet-disk Interaction with a Magnetized Disk Wind: I. Magnetic Flux Concentration and Gap Properties
- Ionization and Dust Charging in Protoplanetary Disks