Dust Evolution and the Formation of Planetesimals

Abstract

The solid content of circumstellar disks is inherited from the interstellar medium: dust particles of at most a micrometer in size. Protoplanetary disks are the environment where these dust grains need to grow at least 13 orders of magnitude in size. Our understanding of this growth process is far from complete, with different physics seemingly posing obstacles to this growth at various stages. Yet, the ubiquity of planets in our galaxy suggests that planet formation is a robust mechanism. This chapter focuses on the earliest stages of planet formation, the growth of small dust grains towards the gravitationally bound "planetesimals", the building blocks of planets. We will introduce some of the key physics involved in the growth processes and discuss how they are expected to shape the global behavior of the solid content of disks. We will consider possible pathways towards the formation of larger bodies and conclude by reviewing some of the recent observational advances in the field.

43 pages, 6 figures. Chapter in International Space Science Institute (ISSI) Book on "The Disk in Relation to the Formation of Planets and their Proto-atmospheres", published in Space Science Reviews by Springer

References in corpus (178)

• Disk Frequencies and Lifetimes in Young Clusters
• Spectral Energy Distributions of T Tauri Stars With Passive Circumstellar Disks
• The Spitzer c2d Legacy Results: Star Formation Rates and Efficiencies; Evolution and Lifetimes
• Protoplanetary Disks and Their Evolution
• Rapid planetesimal formation in turbulent circumstellar discs
• Streaming Instabilities in Protoplanetary Disks
• First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region
• Rapid growth of gas-giant cores by pebble accretion
• Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting observed SEDs using a large grid of pre-computed models
• Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
• A simple model for the evolution of the dust population in protoplanetary disks
• Catastrophic disruptions revisited
• Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDs
• The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts
• A Spitzer Survey of Young Stellar Clusters within One Kiloparsec of the Sun: Cluster Core Extraction and Basic Structural Analysis
• Coagulation, fragmentation and radial motion of solid particles in protoplanetary disks
• Protoplanetary Disk Structures in Ophiuchus
• Dust coagulation in protoplanetary disks: a rapid depletion of small grains
• Gas- and dust evolution in protoplanetary disks
• Resolved Images of Large Cavities in Protoplanetary Transition Disks
• Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations
• The effect of gas drag on the growth of protoplanets -- Analytical expressions for the accretion of small bodies in laminar disks
• A Major Asymmetric Dust Trap in a Transition Disk
• The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? II. Introducing the bouncing barrier
• The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? I. Mapping the zoo of laboratory collision experiments
• Dynamics of Protoplanetary Disks
• Spitzer Space Telescope study of disks in the young $\sigma$ Orionis cluster
• Flaring vs. self-shadowed disks: the SEDs of Herbig Ae/Be stars
• On the Submillimeter Opacity of Protoplanetary Disks
• Closed-form expressions for particle relative velocities induced by turbulence
• The Minimum-Mass Extrasolar Nebula: In-Situ Formation of Close-In Super-Earths
• Forming the cores of giant planets from the radial pebble flux in protoplanetary discs
• The Spitzer Space Telescope Survey of the Orion A & B Molecular Clouds - Part I: A Census of Dusty Young Stellar Objects and a Study of their Mid-IR Variability
• 2-D Radiative Transfer in Protostellar Envelopes: II. An Evolutionary Sequence
• Radial Flow of Dust Particles in Accretion Disks
• Linear and nonlinear evolution of the vertical shear instability in accretion discs
• 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
• Ring shaped dust accumulation in transition disks
• High Resolution Submillimeter Constraints on Circumstellar Disk Structure
• Protoplanetary Disk Structures in Ophiuchus II: Extension to Fainter Sources
• The Disk Population of the Taurus Star-Forming Region
• Dust Filtration by Planet-Induced Gap Edges: Implications for Transitional Disks
• A Survey and Analysis of Spitzer Infrared Spectrograph Spectra of T Tauri Stars in Taurus
• Dust Properties of Protoplanetary Disks in the Taurus-Auriga Star Forming Region from Millimeter Wavelengths
• Discovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory
• Zonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotational Turbulence
• Observations of gas flows inside a protoplanetary gap
• Towards planetesimals: dense chondrule clumps in the protoplanetary nebula
• Gaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations
• Dynamics of Solids in the Midplane of Protoplanetary Disks: Implications for Planetesimal Formation
• Evidence of fast pebble growth near condensation fronts in the HL Tau protoplanetary disk
• A Submillimeter View of Circumstellar Dust Disks in $\rho$ Ophiuchus
• The stickiness of micrometer-sized water-ice particles
• Dust filtration at gap edges: Implications for the spectral energy distributions of discs with embedded planets
• A 10 micron spectroscopic survey of Herbig Ae star disks: grain growth and crystallization
• A dual-frequency sub-arcsecond study of proto-planetary disks at mm wavelengths: First evidence for radial variations of the dust properties
• Asymmetric features in the protoplanetary disk MWC758
• Structure and evolution of pre-main sequence circumstellar disks
• The Stellar Population of the Chamaeleon I Star-Forming Region
• The TW Hya Disk at 870 microns: Comparison of CO and Dust Radial Structures
• The Role of Multiplicity in Disk Evolution and Planet Formation
• Star and protoplanetary disk properties in Orion's suburbs
• Transitional and Pre-Transitional disks: Gap Opening by Multiple Planets?
• Protoplanetary disc evolution and dispersal: the implications of X-ray photoevaportion
• Dust coagulation and fragmentation in molecular clouds. I. How collisions between dust aggregates alter the dust size distribution
• Fluffy dust forms icy planetesimals by static compression
• How to form planetesimals from mm-sized chondrules and chondrule aggregates
• 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
• Pre-main-sequence isochrones -- II. Revising star and planet formation timescales
• Constraints on the Radial Variation of Grain Growth in the AS 209 Circumstellar Disk
• Large-Scale Asymmetries in the Transitional Disks of SAO 206462 and SR 21
• Large dust particles in disks around T Tauri stars
• Structures in the protoplanetary disk of HD142527 seen in polarized scattered light
• Planets opening dust gaps in gas disks
• Formation of Kuiper Belt Binaries by Gravitational Collapse
• Dust grain growth in rho-Ophiuchi protoplanetary disks
• The Onset of Planet Formation in Brown Dwarf Disks
• Planetesimal formation by sweep-up: How the bouncing barrier can be beneficial to growth
• Large grains in the disk of CQ Tau
• Material enhancement in protoplanetary nebulae by particle drift through evaporation fronts
• LkH$\alpha$ 330: Evidence for dust clearing through resolved submillimeter imaging
• Evidence for dust clearing through resolved submillimeter imaging
• Initial Results from The Spitzer Young Stellar Cluster Survey
• A young protoplanet candidate embedded in the circumstellar disk of HD100546
• Dust settling in local simulations of turbulent protoplanetary disks
• Dust diffusion in protoplanetary discs by magnetorotational turbulence
• A search for evolved dust in Herbig Ae stars
• Unveiling the gas and dust disk structure in HD 163296 using ALMA observations
• Possible planet-forming regions on submillimetre images
• The subcritical baroclinic instability in local accretion disc models
• Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilities
• A Spitzer Census of Transitional Protoplanetary Disks with AU-Scale Inner Holes
• Numerical Modeling of the Coagulation and Porosity Evolution of Dust Aggregates
• Polarimetric Imaging of Large Cavity Structures in the Pre-transitional Protoplanetary Disk around PDS 70: Observations of the disk
• Micrometer-sized ice particles for planetary-science experiments - I. Preparation, critical rolling friction force, and specific surface energy
• Extrasolar planets in stellar multiple systems
• Gas and Dust Emission at the Outer Edge of Protoplanetary Disks
• Investigating planet formation in circumstellar disks: CARMA observations of RY Tau and DG Tau
• Dust retention in protoplanetary disks
• Standing on the shoulders of giants: Trojan Earths and vortex trapping in low mass self-gravitating protoplanetary disks of gas and solids
• The Nature of Transition Circumstellar Disks I. The Ophiuchus Molecular Cloud
• Gaps in the HD169142 protoplanetary disk revealed by polarimetric imaging: Signs of ongoing planet formation?
• Steady state of dust distributions in disk vortices: Observational predictions and applications to transitional disks
• Evidence for Two Populations of Classical Transneptunian Objects: The Strong Inclination Dependence of Classical Binaries
• On the Outer Edges of Protoplanetary Dust Disks
• Survival of the mm-cm size grain population observed in protoplanetary disks
• Sub-arcsec imaging of the AB Aur molecular disk and envelope at millimeter wavelengths: a non Keplerian disk
• Breaking through: The effects of a velocity distribution on barriers to dust growth
• High-resolution simulations of planetesimal formation in turbulent protoplanetary discs
• Can dust coagulation trigger streaming instability?
• Three-Dimensional Radiation Transfer in Young Stellar Objects
• Can grain growth explain transition disks?
• Simulations of dust-trapping vortices in protoplanetary discs
• Global MHD simulations of stratified and turbulent protoplanetary discs. II. Dust settling
• The missing cavities in the SEEDS polarized scattered light images of transitional protoplanetary disks: a generic disk model
• Lopsided dust rings in transition disks
• Emergent Mesoscale Phenomena in Magnetized Accretion Disc Turbulence
• From dust to planetesimals: an improved model for collisional growth in protoplanetary disks
• Asymmetric transition disks: Vorticity or eccentricity?
• Gravoturbulent Planetesimal Formation: The Positive Effect of long-lived Zonal Flows
• GASPS - a Herschel survey of gas and dust in Protoplanetary Disks: Summary and Initial Statistics
• On the structure of the transition disk around TW Hya
• On the Transitional Disk Class: Linking Observations of T Tauri Stars & Physical Disk Models
• Formation of Giant Planets by Concurrent Accretion of Solids and Gas inside an Anti-Cyclonic Vortex
• Young Stellar Objects in Lynds 1641: Disks, Accretion, and Star Formation History
• Effects of dust feedback on vortices in protoplanetary disks
• SPITZER/IRAC-MIPS Survey of NGC2244: Protostellar Disk Survival in the Vicinity of Hot Stars
• High Velocity Dust Collisions: Forming Planetesimals in a Fragmentation Cascade with Final Accretion
• Subaru Imaging of Asymmetric Features in a Transitional Disk in Upper Scorpius
• Dust-trapping Rossby vortices in protoplanetary disks
• A representative particle approach to coagulation and fragmentation of dust aggregates and fluid droplets
• The Transitional Protoplanetary Disk Frequency as a Function of Age: Disk Evolution in the Coronet Cluster, Taurus, and Other 1--8 Myr-old Regions
• Erosion and the limits to planetesimal growth
• Formation of pebble-pile planetesimals
• Short dissipation times of proto-planetary discs - an artifact of selection effects?
• The Structure of the Evolved Circumbinary Disk around V4046 Sgr
• Assembling the Building Blocks of Giant Planets around Intermediate Mass Stars
• A break in the gas and dust surface density of the disc around the T Tauri star IM Lup
• Star formation and disk properties in Pismis 24
• The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? III. Sedimentation driven coagulation inside the snow-line
• The Nature of Transition Circumstellar Disks III. Perseus, Taurus, and Auriga
• A panoptic model for planetesimal formation and pebble delivery
• Two populations of transition discs?
• Observations of Solids in Protoplanetary Disks
• GASPS observations of Herbig Ae/Be stars with PACS/Herschel. The atomic and molecular content of their protoplanetary discs
• Global magnetohydrodynamical models of turbulence in protoplanetary disks I. A cylindrical potential on a Cartesian grid and transport of solids
• On the Feeding Zone of Planetesimal Formation by the Streaming Instability
• Growth and migration of solids in evolving protostellar disks I: Methods and Analytical tests
• A Parameter Study for Baroclinic Vortex Amplification
• A Herschel Survey of Cold Dust in Disks Around Brown Dwarfs and Low-Mass Stars
• Monte Carlo simulation of particle interactions at high dynamic range: Advancing beyond the Googol
• Co-Accretion of Chondrules and Dust in the Solar Nebula
• On the nature of the transition disk around LkCa 15
• Mapping H-band Scattered Light Emission in the Mysterious SR21 Transitional Disk
• Short Lifetime of Protoplanetary Disks in Low-metallicity Environments
• Bouncing Behavior of Microscopic Dust Aggregates
• Transitional disks and their origins: an infrared spectroscopic survey of Orion A
• Dynamical Stability of Imaged Planetary Systems in Formation: Application to HL Tau
• Efficiency of Particle Trapping in the Outer Regions of Protoplanetary Disks
• Correlation between the spatial distribution of circumstellar disks and massive stars in the young open cluster NGC 6611. II: Cluster members selected with Spitzer/IRAC
• Constraints on the radial distribution of the dust properties in the CQ Tau protoplanetary disk
• Relative Velocity of Inertial Particles in Turbulent Flows
• The Physics of Protoplanetesimal Dust Agglomerates. V. Multiple Impacts of Dusty Agglomerates at Velocities Above the Fragmentation Threshold
• Young stars in Epsilon Cha and their disks: disk evolution in sparse associations
• Modeling dust growth in protoplanetary disks: The breakthrough case
• SPH simulations of grain growth in protoplanetary disks
• Dust properties and disk structure of evolved protoplanetary disks in Cep OB2: Grain growth, settling, gas and dust mass, and inside-out evolution
• Photometric determination of the mass accretion rates of pre-main sequence stars. III. Results in the Large Magellanic Cloud
• Scattered Light from Dust in the Cavity of the V4046 Sgr Transition Disk
• High-Resolution Submillimeter and Near-Infrared Studies of the Transition Disk around Sz 91
• Turbulence-Induced Relative Velocity of Dust Particles II: The Bidisperse Case
• Dust crystallinity in protoplanetary disks: the effect of diffusion/viscosity ratio
• The Herschel/PACS view of the Cep OB2 region: Global protoplanetary disk evolution and clumpy star formation
• On the secular behavior of dust particles in an eccentric protoplanetary disk with an embedded massive gas giant planet
• Accretion through the inner hole of transitional disks: What happens to the dust?

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• The Ring Structure in the MWC 480 Disk Revealed by ALMA
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• Hydrogen dominated atmospheres on terrestrial mass planets: evidence, origin and evolution
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• On the Numerical Robustness of the Streaming Instability: Particle Concentration and Gas Dynamics in Protoplanetary Disks
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• Hayabusa2 Extended Mission: New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period
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• The Anatomy of an Unusual Edge-on Protoplanetary Disk I. Dust Settling in a Cold Disk
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