Setting the Stage: Planet formation and Volatile Delivery
arXiv:2006.07127 · doi:10.1007/s11214-020-00700-y
Abstract
The diversity in mass and composition of planetary atmospheres stems from the different building blocks present in protoplanetary discs and from the different physical and chemical processes that these experience during the planetary assembly and evolution. This review aims to summarise, in a nutshell, the key concepts and processes operating during planet formation, with a focus on the delivery of volatiles to the inner regions of the planetary system.
Accepted for publication in Space Science Reviews. 25 pages of text, 19 pages of references. Part of ISSI special collection on Diversity of Atmospheres
References in corpus (180)
- The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets
- Rapid planetesimal formation in turbulent circumstellar discs
- A low mass for Mars from Jupiter's early gas-driven migration
- Streaming Instabilities in Protoplanetary Disks
- Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler
- The Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview
- Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data
- The origins and concentrations of water, carbon, nitrogen and noble gases on Earth
- Towards a Deterministic Model of Planetary Formation I: a Desert in the Mass and Semi Major Axis Distributions of Extra Solar Planets
- Rapid growth of gas-giant cores by pebble accretion
- Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
- A simple model for the evolution of the dust population in protoplanetary disks
- Kepler planets: a tale of evaporation
- Most 1.6 Earth-Radius Planets are not Rocky
- The evaporation valley in the Kepler planets
- Coagulation, fragmentation and radial motion of solid particles in protoplanetary disks
- Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
- Models of Giant Planet formation with migration and disc evolution
- Dust coagulation in protoplanetary disks: a rapid depletion of small grains
- The effect of gas drag on the growth of protoplanets -- Analytical expressions for the accretion of small bodies in laminar disks
- ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses
- On the width and shape of gaps in protoplanetary disks
- Growth Model Interpretation of Planet Size Distribution
- The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? I. Mapping the zoo of laboratory collision experiments
- Extrasolar planet population synthesis I: Method, formation tracks and mass-distance distribution
- Gravitational Instabilities in Circumstellar Disks
- Asteroids Were Born Big
- A torque formula for non-isothermal Type I planetary migration - II. Effects of diffusion
- An asteroseismic view of the radius valley: stripped cores, not born rocky
- Core-powered mass loss and the radius distribution of small exoplanets
- Two accreting protoplanets around the young star PDS 70
- Making other Earths: Dynamical Simulations of Terrestrial Planet Formation and Water Delivery
- Forming the cores of giant planets from the radial pebble flux in protoplanetary discs
- Separating gas-giant and ice-giant planets by halting pebble accretion
- Building the Terrestrial Planets: Constrained Accretion in the Inner Solar System
- Can giant planets form by direct gravitational instability?
- Protoplanetary Disk Structures in Ophiuchus II: Extension to Fainter Sources
- Sculpting the Valley in the Radius Distribution of Small Exoplanets as a by-product of Planet Formation: The Core-Powered Mass-Loss Mechanism
- Dust Properties of Protoplanetary Disks in the Taurus-Auriga Star Forming Region from Millimeter Wavelengths
- How Thermal Evolution and Mass Loss Sculpt Populations of Super-Earths and Sub-Neptunes: Application to the Kepler-11 System and Beyond
- Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core
- High-resolution simulations of the final assembly of Earth-like planets 1: terrestrial accretion and dynamics
- Reversing type II migration: resonance trapping of a lighter giant protoplanet
- A Kinematical Detection of Two Embedded Jupiter Mass Planets in HD 163296
- Dynamics of the giant planets of the solar system in the gaseous proto-planetary disk and relationship to the current orbital architecture
- On the theory of disc photoevaporation
- Pebble isolation mass --- scaling law and implications for the formation of super-Earths and gas giants
- Formation of the Terrestrial Planets from a Narrow Annulus
- Structure and evolution of pre-main sequence circumstellar disks
- Dust Evolution and the Formation of Planetesimals
- Dynamical Evolution of the Early Solar System
- Halting Type I planet migration in non-isothermal disks
- Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion
- Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations
- Initial Conditions of Planet Formation: Lifetimes of Primordial Disks
- Planetesimal formation starts at the snow line
- Compositional imprints in density-distance-time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation
- Water Delivery and Giant Impacts in the 'Grand Tack' Scenario
- The great dichotomy of the Solar System: small terrestrial embryos and massive giant planet cores
- Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk
- Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode
- Interior Models of Uranus and Neptune
- To Cool is to Accrete: Analytic Scalings for Nebular Accretion of Planetary Atmospheres
- Large dust particles in disks around T Tauri stars
- Constraints on the mass of a habitable planet with water of nebular origin
- Atmospheres of low-mass planets: the "boil-off"
- The Ophiuchus DIsc Survey Employing ALMA (ODISEA) - I : project description and continuum images at 28 au resolution
- Evolution of Protoplanetary Discs with Magnetically Driven Disc Winds
- The Structure and Emission of the Accretion Shock in T Tauri Stars II: the Ultraviolet Continuum Emission
- Fossilized condensation lines in the Solar System protoplanetary disk
- Large grains in the disk of CQ Tau
- Close-in planetesimal formation by pile-up of drifting pebbles
- In-situ Accretion of Hydrogen-Rich Atmospheres on Short-Period Super-Earths: Implications for the Kepler-11 Planets
- Dust Evolution in Protoplanetary Disks
- Hydrodynamics of Embedded Planets' First Atmospheres. II. A Rapid Recycling of Atmospheric Gas
- Theoretical models of planetary system formation: mass vs semi-major axis
- On the water delivery to terrestrial embryos by ice pebble accretion
- Planet migration in three-dimensional radiative discs
- Planet heating prevents inward migration of planetary cores
- Migration of massive planets in accreting disks
- Formation of planets by tidal downsizing of giant planet embryos
- Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object
- Measuring Turbulence in TW Hya with ALMA: Methods and Limitations
- Orbital migration of low-mass planets in evolutionary radiative models: Avoiding catastrophic infall
- Stellar irradiated discs and implications on migration of embedded planets I: equilibrium discs
- The newborn planet population emerging from ring-like structures in discs
- The Evolution of Stellar Rotation and the hydrogen atmospheres of habitable-zone Terrestrial Planets
- Reduced gas accretion on super-Earths and ice giants
- A water budget dichotomy of rocky protoplanets from Al-heating
- Planet formation with envelope enrichment: new insights on planetary diversity
- Origin of the Ocean on the Earth: Early Evolution of Water D/H in a Hydrogen-rich Atmosphere
- On the formation of multiple concentric rings and gaps in protoplanetary disks
- Formation of giant planets and brown dwarfs on wide orbits
- Planet formation models: the interplay with the planetesimal disc
- Dust evolution in protoplanetary discs and the formation of planetesimals. What have we learned from laboratory experiments?
- Gas Giant Formation with Small Cores Triggered by Envelope Pollution by Icy Planetesimals
- On Gas-Drag Induced Rapid Migration of Solids in a Non-Uniform Solar Nebula
- Migration of Earth-size planets in 3D radiative discs
- Jupiter's evolution with primordial composition gradients
- How much does turbulence change the pebble isolation mass for planet formation?
- Hydrodynamics of embedded planets' first atmospheres - III. The role of radiation transport for super-Earth planets
- The Frequency of Giant impacts on Earth-like Worlds
- Multiple Disk Gaps and Rings Generated by a Single Super-Earth: II. Spacings, Depths, and Number of Gaps, with Application to Real Systems
- The formation of Jupiter by hybrid pebble-planetesimal accretion
- The Delivery of Water During Terrestrial Planet Formation
- Massive planet migration: Theoretical predictions and comparison with observations
- Impacts of planet migration models on planetary populations. Effects of saturation, cooling and stellar irradiation
- Coorbital thermal torques on low-mass protoplanets
- Migration-driven diversity of super-Earth compositions
- Dust unveils the formation of a mini-Neptune planet in a protoplanetary ring
- Improved torque formula for low and intermediate mass planetary migration
- Short dissipation times of proto-planetary discs - an artifact of selection effects?
- Outward Migration of Jupiter and Saturn in Evolved Gaseous Disks
- Critical core mass for enriched envelopes: the role of H2O condensation
- Rapid Formation of Ice Giant Planets
- Planet population synthesis driven by pebble accretion in cluster environments
- How cores grow by pebble accretion I. Direct core growth
- Microlensing Results Challenge the Core Accretion Runaway Growth Scenario for Gas Giants
- Streaming Instability for Particle-Size Distributions
- Formation of close-in super-Earths in evolving protoplanetary disks due to disk winds
- The multifaceted planetesimal formation process
- Planetary population synthesis
- A Compound model for the origin of Earth's water
- Rocky super-Earths or waterworlds: the interplay of planet migration, pebble accretion and disc evolution
- Planet formation by pebble accretion in ringed disks
- HD far infrared emission as a measure of protoplanetary disk mass
- Suppression of atmospheric recycling of planets embedded in a protoplanetary disc by buoyancy barrier
- Range of outward migration and influence of the disc's mass on the migration of giant planet cores
- Giant planet formation in radially structured protoplanetary discs
- The origin of the high metallicity of close-in giant exoplanets: Combined effect of the resonant and aerodynamic shepherding
- Accretion and Evolution of ~2.5 Earth-mass Planets with Voluminous H/He Envelopes
- Improving the Accuracy of Planet Occurrence Rates from Kepler using Approximate Bayesian Computation
- Formation and accretion history of terrestrial planets from runaway growth through to late time: implications for orbital eccentricity
- The formation of mini-Neptunes
- Prograde rotation of protoplanets by accretion of pebbles in a gaseous environment
- New Formation Models for the Kepler-36 System
- Infall of planetesimals onto growing giant planets: onset of runaway gas accretion and metallicity of their gas envelopes
- Analysis of terrestrial planet formation by the Grand Tack model: System architecture and tack location
- Diverse outcomes of planet formation and composition around low-mass stars and brown dwarfs
- Water delivery by pebble accretion to rocky planets in habitable zones in evolving disks
- Coagulation Calculations of Icy Planet Formation at 15--150 AU: A Correlation Between the Maximum Radius and the Slope of the Size Distribution for Transneptunian Objects
- Jupiter's heavy-element enrichment expected from formation models
- Oligarchic planetesimal accretion and giant planet formation
- Threshold radii of volatile-rich planets
- Gravitational fragmentation and formation of giant protoplanets on tens-of-au orbits
- Azimuthal and Vertical Streaming Instability at High Dust-to-gas Ratios and on the Scales of Planetesimal Formation
- Simultaneous formation of Solar System giant planets
- Convergence zones for Type I migration: an inward shift for multiple planet systems
- Formation of solar system analogs I: looking for initial conditions through a population synthesis analysis
- The cool and distant formation of Mars
- Thermal torque effects on the migration of growing low-mass planets
- Consequences of the simultaneous formation of giant planets by the core accretion mechanism
- Hydrogen isotopic evidence for early oxidation of silicate Earth
- Metallicity effect and planet mass function in pebble-based planet formation models
- The role of planetesimal fragmentation on giant planet formation
- Planet Population Synthesis
- The distribution of heavy-elements in giant protoplanetary atmospheres: the importance of planetesimal-envelope interactions
- Are the observed gaps in protoplanetary discs caused by growing planets?
- 3D Simulations of Planet Trapping at Disc-Cavity Boundaries
- Oligarchic planetesimal accretion and giant planet formation II
- Giant planet formation at the pressure maxima of protoplanetary disks
- The Effects of Stellar Companions on Exoplanet Radius Distributions
- Realistic collisional water transport during terrestrial planet formation: Self-consistent modeling by an N-body--SPH hybrid code
- The role of the initial surface density profiles of the disc on giant planet formation: comparing with observations
- Planetary formation and water delivery in the habitable zone around solar-type stars in different dynamical environments
- Unified simulations of planetary formation and atmospheric evolution: Effects of pebble accretion, giant impacts, and stellar irradiations on super-Earth formation
- Impact of photoevaporative mass loss on masses and radii of water-rich sub/super-Earths
- Formation of Terrestrial Planets in Disks with Different Surface Density Profiles
- Trapping planets in an evolving protoplanetary disk: preferred time, locations and planet mass
- Formation of Terrestrial Planets
- Role of gaseous giants in the dynamical evolution of terrestrial planets and water delivery in the habitable zone
- Oscillatory migration of accreting protoplanets driven by a 3D distortion of the gas flow
- Diversity of planetary systems in low-mass disks: Terrestrial-type planet formation and water delivery
- Capture and migration of Jupiter and Saturn in mean motion resonance in a gaseous protoplanetary disc
- Formation of Solar system analogues II: post-gas phase growth and water accretion in extended discs via N-body simulations
- The formation of giant planets in wide orbits by photoevaporation-synchronised migration
- Connecting Planetary Composition with Formation
- Terrestrial-type planet formation: Comparing different types of initial conditions
- A limit on gas accretion onto close-in super-Earth cores from disk accretion
- Investigating the possibility of reversing giant planet migration via gap edge illumination
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- Astrochemistry and compositions of planetary systems
- Hydrogen dominated atmospheres on terrestrial mass planets: evidence, origin and evolution
- Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario
- Convective outgassing efficiency in planetary magma oceans: insights from computational fluid dynamics
- Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses
- Redox hysteresis of super-Earth exoplanets from magma ocean circulation
- System-level fractionation of carbon from disk and planetesimal processing
- The importance of thermal torques on the migration of planets growing by pebble accretion
- Long live the disk: lifetimes of protoplanetary disks in hierarchical triple star systems and a possible explanation for HD 98800 B
- Reduced late bombardment on rocky exoplanets around M-dwarfs
- Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets
- Stability of Hydrides in Sub-Neptune Exoplanets with Thick Hydrogen-Rich Atmospheres
- Heating, Excitation, Dissociation, and Ionization of Molecules by High-Energy Photons in Planetary Atmospheres
- Born Dry or Born Wet? A Palette of Water Growth Histories in TRAPPIST-1 Analogs and Compact Planetary Systems
- Formation of the four terrestrial planets in the Jupiter-Saturn chaotic excitation scenario: fundamental properties and water delivery
- Linking Outer Disk Pebble Dynamics and Gaps to Inner Disk Water Enrichment
- Gravitational instability in planet-forming discs