The evolution of a circumplanetary disc with a dead zone
arXiv:2011.01384 · doi:10.1093/mnras/staa3427
Abstract
We investigate whether the regular Galilean satellites could have formed in the dead zone of a circumplanetary disc. A dead zone is a region of weak turbulence in which the magnetorotational instability (MRI) is suppressed, potentially an ideal environment for satellite formation. With the grid-based hydrodynamic code, FARGO3D, we examine the evolution of a circumplanetary disc model with a dead zone. Material accumulates in the dead zone of the disc leading to a higher total mass and but a similar temperature profile compared to a fully turbulent disc model. The tidal torque increases the rate of mass transport through the dead zone leading to a steady state disc with a dead zone that does not undergo accretion outbursts. We explore a range of disc, dead zone and mass inflow parameters and find that the maximum mass of the disc is around 0.001 MJ . Since the total solid mass of such a disc is much lower, we find that there is not sufficient material in the disc for in situ formation of the Galilean satellites and that external supplement is required.
arXiv comment10 pages, 6 figures
References in corpus (90)
- Using FU Orionis Outbursts to Constrain Self-Regulated Protostellar Disk Models
- Rapid growth of gas-giant cores by pebble accretion
- Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations
- Accretion disc viscosity: how big is alpha?
- Wind-driven Accretion in Protoplanetary Disks. I: Suppression of the Magnetorotational Instability and Launching of the Magnetocentrifugal Wind
- Planetesimal Formation by Gravitational Instability
- Turbulence in Accretion Disks. Vorticity Generation and Angular Momentum Transport via the Global Baroclinic Instability
- Rapid Coagulation of Porous Dust Aggregates Outside the Snow Line: A Pathway to Successful Icy Planetesimal Formation
- Disk Accretion Onto High-Mass Planets
- Magnetorotational Instability in Protoplanetary Disks. II. Ionization State and Unstable Regions
- Dust Filtration by Planet-Induced Gap Edges: Implications for Transitional Disks
- Mass Flow and Accretion through gaps in Accretion Discs
- Dynamics of Solids in the Midplane of Protoplanetary Disks: Implications for Planetesimal Formation
- Eccentricity Evolution for Planets in Gaseous Disks
- Episodic accretion in magnetically layered protoplanetary discs
- Local Magnetohydrodynamical Models of Layered Accretion Disks
- Three-dimensional Calculations of High and Low-mass Planets Embedded in Protoplanetary Discs
- Gas Flow Across Gaps in Protoplanetary Disks
- FARGO3D: A new GPU-oriented MHD code
- MHD simulations of the magnetorotational instability in a shearing box with zero net flux. II. The effect of transport coefficients
- Non-steady Accretion in Protostars
- Dust size distributions in coagulation/fragmentation equilibrium: Numerical solutions and analytical fits
- Distribution of Accreting Gas and Angular Momentum onto Circumplanetary Disks
- The tidally induced warping, precession and truncation of accretion discs in binary systems: three-dimensional simulations
- On the Location of the Snow Line in a Protoplanetary Disk
- Evolution of Protoplanetary Discs with Magnetically Driven Disc Winds
- Accretion of Jupiter-mass Planets in the Limit of Vanishing Viscosity
- Dust flow in gas disks in the presence of embedded planets
- Turbulent Mixing and the Dead Zone in Protostellar Disks
- Heat and Dust in Active Layers of Protostellar Disks
- Nested-grid calculations of disk-planet interaction
- On the water delivery to terrestrial embryos by ice pebble accretion
- Protoplanetary Disk Winds by Magnetorotational Instability : Formation of an Inner Hole and a Crucial Assist for Planet Formation
- Tidal Truncation of Inclined Circumstellar and Circumbinary Discs in Young Stellar Binaries
- Dead Zone Accretion Flows in Protostellar Disks
- The Hot Inner Disk of FU Ori
- On the origin of episodic accretion in Dwarf Novae
- On the Evolution of the Snow Line in Protoplanetary Discs
- Modeling Magnetorotational Turbulence in Protoplanetary Disks with Dead Zones
- The Kozai-Lidov Mechanism in Hydrodynamical Disks
- Meridional circulation of gas into gaps opened by giant planets in three-dimensional low-viscosity disks
- Saturation of the corotation resonance in a gaseous disk
- Gas accretion onto planetary cores: three-dimensional self-gravitating radiation hydrodynamical calculations
- Global hydromagnetic simulations of a planet embedded in a dead zone: gap opening, gas accretion and formation of a protoplanetary jet
- Baroclinic Vorticity Production in Protoplanetary Disks; Part I: Vortex Formation
- Thermo-Hydrodynamics of Circumstellar Disks with High-mass Planets
- The hydrodynamical response of a tilted circumbinary disc: linear theory and non-linear numerical simulations
- The baroclinic instability in the context of layered accretion. Self-sustained vortices and their magnetic stability in local compressible unstratified models of protoplanetary disks
- Do Proto-Jovian Planets Drive Outflows?
- Diffusion and Concentration of Solids in the Dead Zone of a Protoplanetary Disk
- Turbulent Torques on Protoplanets in a Dead Zone
- The Gravo-Magneto Limit Cycle in Accretion Disks
- The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? III. Sedimentation driven coagulation inside the snow-line
- Angular Momentum Accretion onto a Gas Giant Planet
- On the Radio Detectability of Circumplanetary Discs
- Tidal Torques on Misaligned Disks in Binary Systems
- Planet-Disc Interactions and Early Evolution of Planetary Systems
- On the physical nature of accretion disc viscosity
- 3D MHD Simulations of Planet Migration in Turbulent Stratified Disks
- Dust accretion onto high-mass planets
- Turbulent diffusion in protoplanetary discs: the effect of an imposed magnetic field
- On the Viability of the Magnetorotational Instability in Circumplanetary Disks
- Dead Zones around Young Stellar Objects: Dependence on Physical Parameters
- On the angular momentum transport due to vertical convection in accretion discs
- Shock-driven Accretion in Circumplanetary Disks: Observables and Satellite Formation
- On the dynamics of planetesimals embedded in turbulent protoplanetary discs with dead zones
- Dead Zones around Young Stellar Objects: FU Orionis Outbursts and Transition Discs
- On Hydrodynamic Motions in Dead Zones
- The Galilean Satellites Formed Slowly from Pebbles
- Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk: Ideal Unstratified Disks
- Resolution Dependence of Magnetorotational Turbulence in the Isothermal Stratified Shearing Box
- Observability of Forming Planets and their Circumplanetary Disks I. -- Parameter Study for ALMA
- Magnetorotational turbulence transports angular momentum in stratified disks with low magnetic Prandtl number but magnetic Reynolds number above a critical value
- Gravito-Turbulent Disks in 3D: Turbulent Velocities vs. Depth
- Angular momentum transport and large eddy simulations in magnetorotational turbulence: the small Pm limit
- On the Nature of Magnetic Turbulence in Rotating, Shearing Flows
- Physical and chemical structure of planet-forming disks probed by millimeter observations and modeling
- Saturn's formation and early evolution at the origin of Jupiter's massive moons
- Accretion Outbursts in Circumplanetary Disks
- Accretion of gas onto gap-opening planets and circumplanetary flow structure in magnetized turbulent disks
- On the convergence of Magnetorotational turbulence in stratified isothermal shearing boxes
- The Planetary Luminosity Problem: "Missing Planets" and the Observational Consequences of Episodic Accretion
- Orbital Evolution of Moons in Weakly Accreting Circumplanetary Disks
- The gravo-magneto disc instability with a viscous dead zone
- Investigating the gas-to-dust ratio in the protoplanetary disk of HD 142527
- Growth and evolution of satellites in a Jovian massive disc
- Dead Zones In Circumplanetary Discs as Formation Sites For Regular Satellites
- A fast-growing tilt instability of detached circumplanetary disks
- On the growth and orbital evolution of giant planets in layered protoplanetary disks
- [The Impact of Nuclear Star Formation on Gas Inflow to AGN