Dust growth and evolution in protoplanetary disks
arXiv:2312.13287 · doi:10.1146/annurev-astro-071221-052705
Abstract
Over the past decade, advancement of observational capabilities, specifically the Atacama Large Millimeter/submillimeter Array (ALMA) and SPHERE instrument, alongside theoretical innovations like pebble accretion, have reshaped our understanding of planet formation and the physics of protoplanetary disks. Despite this progress, mysteries persist along the winded path of micrometer-sized dust, from the interstellar medium, through transport and growth in the protoplanetary disk, to becoming gravitationally bound bodies. This review outlines our current knowledge of dust evolution in circumstellar disks, yielding the following insights: Theoretical and laboratory studies have accurately predicted the growth of dust particles to sizes that are susceptible to accumulation through transport processes like radial drift and settling. Critical uncertainties in that process remain the level of turbulence, the threshold collision velocities at which dust growth stalls, and the evolution of dust porosity. Symmetric and asymmetric substructure are widespread. Dust traps appear to be solving several long-standing issues in planet formation models, and they are observationally consistent with being sites of active planetesimal formation. In some instances, planets have been identified as the causes behind substructures. This underlines the need to study earlier stages of disks to understand how planets can form so rapidly. In the future, better probes of the physical conditions in optically thick regions, including densities, turbulence strength, kinematics, and particle properties will be essential for unraveling the physical processes at play.
Review to be published in Annual Reviews of Astronomy and Astrophysics (authors version, 48 pages including 11 figures and 314 references)
References in corpus (74)
- The NumPy array: a structure for efficient numerical computation
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Formation of methyl formate and other organic species in the warm-up phase of hot molecular cores
- Coagulation, fragmentation and radial motion of solid particles in protoplanetary disks
- Gas- and dust evolution in protoplanetary disks
- Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations
- Closed-form expressions for particle relative velocities induced by turbulence
- A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation
- Ring shaped dust accumulation in transition disks
- Towards planetesimals: dense chondrule clumps in the protoplanetary nebula
- Dust filtration at gap edges: Implications for the spectral energy distributions of discs with embedded planets
- Global simulations of protoplanetary disks with ohmic resistivity and ambipolar diffusion
- Planetesimal formation starts at the snow line
- How to form planetesimals from mm-sized chondrules and chondrule aggregates
- The M31 Velocity Vector. II. Radial Orbit Towards the Milky Way and Implied Local Group Mass
- Dust size distributions in coagulation/fragmentation equilibrium: Numerical solutions and analytical fits
- Grain Retention and Formation of Planetesimals near the Snow Line in MRI-driven Turbulent Protoplanetary Disks
- Dust coagulation in protoplanetary disks: porosity matters
- Close-in planetesimal formation by pile-up of drifting pebbles
- Three radial gaps in the disk of TW Hydrae imaged with SPHERE
- Bifurcation of planetary building blocks during Solar System formation
- A Millimeter Continuum Size-Luminosity Relationship for Protoplanetary Disks
- Multiple Disk Gaps and Rings Generated by a Single Super-Earth
- Contacts of Water Ice in Protoplanetary Disks - Laboratory Experiments
- The Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations
- Planetesimal formation around the snow line in MRI-driven turbulent protoplanetary disks
- Convective Overstability in radially stratified accretion disks under thermal relaxation
- On the formation of multiple concentric rings and gaps in protoplanetary disks
- A highly settled disk around Oph 163131
- Magnetic Flux Concentration and Zonal Flows in Magnetorotational Instability Turbulence
- Can dead zones create structures like a transition disk?
- Global MHD simulations of stratified and turbulent protoplanetary discs. II. Dust settling
- On the origin of horseshoes in transitional discs
- Turbulence sets the length scale for planetesimal formation: Local 2D simulations of streaming instability and planetesimal formation
- High Velocity Dust Collisions: Forming Planetesimals in a Fragmentation Cascade with Final Accretion
- Convective overstability in accretion disks: 3D linear analysis and nonlinear saturation
- A representative particle approach to coagulation and fragmentation of dust aggregates and fluid droplets
- Erosion and the limits to planetesimal growth
- The time evolution of dusty protoplanetary disc radii: observed and physical radii differ
- Water in the terrestrial planet-forming zone of the PDS 70 disk
- Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
- The efficiency of dust trapping in ringed proto-planetary discs
- Tracing water vapor and ice during dust growth
- New composite models of partially ionized protoplanetary disks
- DustPy: A Python Package for Dust Evolution in Protoplanetary Disks
- Planet formation by pebble accretion in ringed disks
- Growth and migration of solids in evolving protostellar disks I: Methods and Analytical tests
- Global magnetohydrodynamical models of turbulence in protoplanetary disks I. A cylindrical potential on a Cartesian grid and transport of solids
- Monte Carlo simulation of particle interactions at high dynamic range: Advancing beyond the Googol
- Distribution of solids in the rings of the HD 163296 disk: a multiwavelength study
- Leaky dust traps: How fragmentation impacts dust filtering by planets
- New Constraints From Dust Lines On The Surface Densities Of Protoplanetary Disks
- Testing the Jeans, Toomre and Bonnor-Ebert concepts for planetesimal formation: 3D streaming instability simulations of diffusion regulated formation of planetesimals
- Modeling dust growth in protoplanetary disks: The breakthrough case
- Linear growth of streaming instability in pressure bumps
- High Resolution Parameter Study of the Vertical Shear Instability
- On the millimetre continuum flux-radius correlation of proto-planetary discs
- Radiation pressure clear-out of dusty photoevaporating discs
- The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?
- Solving the Coagulation Equation by the Moments Method
- A large population study of protoplanetary disks: Explaining the millimeter size-luminosity relation with or without sub-structure
- Ionization and Dust Charging in Protoplanetary Disks
- Micrometer-Sized Water Ice Particles for Planetary Science Experiments: Influence of Surface Structure on Collisional Properties
- Streaming instability of multiple particle species II -- Numerical convergence with increasing particle number
- HD 143006: circumbinary planet or misaligned disc?
- Grain growth for astrophysics with Discontinuous Galerkin schemes
- Effects of photoevaporation on protoplanetary disc `isochrones'
- Turbulence-Induced Relative Velocity of Dust Particles II: The Bidisperse Case
- Constraining the Physical State of the Hot Gas Halos in NGC 4649 and NGC 5846
- Dust Traffic Jams in Inclined Circumbinary Protoplanetary Discs I. Morphology and Formation Theory
- Magnetic Properties and Flow Angle of the Inverse Evershed Flow at Its Downflow Points
- The general applicability of self-similar solutions for thermal disc winds
- A Search for the 3.5 keV Line from the Milky Way's Dark Matter Halo with HaloSat
- Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
Cited by in corpus (58)
- Formation and evolution of a protoplanetary disk: combining observations, simulations and cosmochemical constraints
- The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): I. Program Overview and Summary of First Results
- CO2-rich protoplanetary discs as a probe of dust radial drift & trapping
- Revising the Giant Planet Mass-Metallicity Relation: Deciphering the Formation Sequence of Giant Planets
- Solving for the 2D Water Snowline with Hydrodynamic Simulations. Emergence of gas outflow, water cycle and temperature plateau
- TriPoD: Tri-Population size distributions for Dust evolution. Coagulation in vertically integrated hydrodynamic simulations of protoplanetary disks
- The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
- The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): VI. Comparison of Dust Evolution Models to AGE-PRO Observations
- FAUST XXVI. The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks
- Planet formation in chemically diverse and evolving discs -- I. Composition of planetary building blocks
- Multi-frequency analysis of the ALMA and VLA high resolution continuum observations of the substructured disc around CI Tau. Preference for sub-mm-sized low-porosity amorphous carbon grains
- Formation of super-Earths and mini-Neptunes from rings of planetesimals
- Strong clumping in global streaming instability simulations with a dusty fluid
- UV-processing of icy pebbles in the outer parts of VSI-turbulent disks
- Edge-On Disk Study (EODS) II: Thermal Structure of the Flying Saucer Disk
- Clusters of tribocharged dust aggregates as pebbles in protoplanetary disks
- Confirmation of a ring structure in the disk around MP Mus (PDS 66) with ALMA Band 7 observations
- On the diversification and dissipation of protoplanetary disks
- The evolution of the flux-size relationship in protoplanetary discs by viscous evolution and radial pebble drift
- FAUST. XXVIII. High-Resolution ALMA Observations of Class 0/I Disks: Structure, Optical Depths, and Temperatures
- On the 3D time evolution of the dust size distribution in protostellar envelopes
- Dust Drift Timescales in Protoplanetary Disks at the Cusp of Gravitational Instability
- Dust trapping in protoplanetary discs after stellar flybys
- From small dust to micron-sized aggregates: the influence of structure and composition on the dust optical properties
- Planet Mass Function around M stars at 1-10 au: A Plethora of sub-Earth mass objects
- Dust enrichment and growth in the earliest stages of protoplanetary disk formation
- Peering through the veil: Investigating protoplanetary disk outer edges using backside visibility
- Early Solar System Turbulence Constrained by High Oxidation States of the Oldest Non-Carbonaceous Planetesimals
- Rossby wave instability in weakly ionized protoplanetary disks. II. radial B-fields
- Starlight-driven flared-staircase geometry in radiation hydrodynamic models of protoplanetary disks
- Origin of compact exoplanetary systems during disk infall
- The Impact of Silicate Grain Coagulation on Millimeter Emission from Massive Protostellar Disks
- Models and Observational Predictions of Dust Traps in Protoplanetary Discs
- Callisto's Nonresonant Orbit as an Outcome of Circum-Jovian Disk Substructure
- Timescales diagnostics for saving viscous and MHD-driven dusty discs from external photoevaporation
- Probing dust and grain growth in the optically thick circumbinary ring of V892 Tau
- How two-dimensional are planet-disc interactions? II. Radiation hydrodynamics and suitable cooling prescriptions
- Dust and Water in V883 Ori: Relics of a Retreating Snowline
- The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE
- Icy Volatile Enhancements in Evolving Protoplanetary Disks
- Large Dust Grains and a Possible Dust Trap in the Polar Circumbinary Disc of HD 98800B
- Evading the dust fragmentation barrier with the streaming instability in protoplanetary disks
- Dust growth and planet formation by disc fragmentation
- Gaps and Rings: A Near-Universal Trait of Extended Protoplanetary Discs
- Dust Growth in ALMA Rings: II. Dusty Rossby Wave Instability
- Dust-driven vortex cascades originating at water snow regions: A pathway to planetesimal formation
- Non-ideal MHD and protostellar feedback effects on disc formation and evolution in numerical simulations of star cluster formation
- Performance of a high-order MPI-Kokkos accelerated fluid solver
- Resolution and calibration effects in high contrast polarimetric imaging of circumstellar scattering regions
- Caustics of finitely dense inertial particles
- PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster
- Magnetic clumping of charged dust in the dense interstellar medium
- Gas dynamics around dust asymmetries in turbulent disks
- A multi-fluid approach for polydisperse pebble accretion: From particles to fluids, establishing the multifluid framework
- Reading between the rings: observed dust ring properties as probes of planet masses
- MINDS survey of silicates in T Tauri disks: Correlation between dust and gas
- Gravitational instability in planet-forming discs
- Setting the Stage: The Early History of the Solar System