Formation, Orbital and Internal Evolutions of Young Planetary Systems
arXiv:1604.07558 · doi:10.1007/s11214-016-0258-z
Abstract
The growing body of observational data on extrasolar planets and protoplanetary disks has stimulated intense research on planet formation and evolution in the past few years. The extremely diverse, sometimes unexpected physical and orbital characteristics of exoplanets lead to frequent updates on the mainstream scenarios for planet formation and evolution, but also to the exploration of alternative avenues. The aim of this review is to bring together classical pictures and new ideas on the formation, orbital and internal evolutions of planets, highlighting the key role of the protoplanetary disk in the various parts of the theory. We begin by briefly reviewing the conventional mechanism of core accretion by the growth of planetesimals, and discuss a relatively recent model of core growth through the accretion of pebbles. We review the basic physics of planet-disk interactions, recent progress in this area, and discuss their role in observed planetary systems. We address the most important effects of planets internal evolution, like cooling and contraction, the mass-luminosity relation, and the bulk composition expressed in the mass-radius and mass-mean density relations.
49 pages, 12 figures, accepted for publication in Space Science Reviews. Chapter in International Space Science Institute (ISSI) Book on "The Disk in Relation to the Formation of Planets and their Proto-atmospheres" to be published in Space Science Reviews by Springer
References in corpus (62)
- Dynamical Outcomes of Planet-Planet Scattering
- Most 1.6 Earth-Radius Planets are not Rocky
- Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations
- A giant comet-like cloud of hydrogen escaping the warm Neptune-mass exoplanet GJ 436b
- On the Luminosity of Young Jupiters
- Planet formation around stars of various masses: The snow line and the frequency of giant planets
- Line and Mean Opacities for Ultracool Dwarfs and Extrasolar Planets
- Tidal dissipation in stars and giant planets
- Toward a Deterministic Model of Planetary Formation V. Accumulation Near the Ice Line
- Models of the in situ formation of detected extrasolar giant planets
- The properties of brown dwarfs and low-mass hydrogen-burning stars formed by disc fragmentation
- Planetary population synthesis coupled with atmospheric escape: a statistical view of evaporation
- Can we constrain interior structure of rocky exoplanets from mass and radius measurements?
- Asymmetric features in the protoplanetary disk MWC758
- Global simulations of protoplanetary disks with ohmic resistivity and ambipolar diffusion
- The structure of protoplanetary discs around evolving young stars
- Inflating Hot Jupiters With Ohmic Dissipation
- Towards Chemical Constraints on Hot Jupiter Migration
- The Two Modes of Gas Giant Planet Formation
- On the corotation torque in a radiatively inefficient disk
- Transiting exoplanets from the CoRoT space mission VI. CoRoT-Exo-3b: The first secure inhabitant of the brown-dwarf desert
- The Mass of Kepler-93b and The Composition of Terrestrial Planets
- Ocean Planet or Thick Atmosphere: On the Mass-Radius Relationship for Solid Exoplanets with Massive Atmospheres
- Atmospheric Mass Loss During Planet Formation: The Importance of Planetesimal Impacts
- Resonant Repulsion of Kepler Planet Pairs
- Heat transport in giant (exo)planets: a new perspective
- Hall-effect Controlled Gas Dynamics in Protoplanetary Disks: II. Full 3D Simulations toward the Outer Disk
- Cavity opening by a giant planet in a protoplanetary disc and effects on planetary migration
- Accreting Circumplanetary Disks: Observational Signatures
- Migration of massive planets in accreting disks
- Exoplanet HD 209458b : Evaporation strengthened
- On disc protoplanet interactions in a non-barotropic disc with thermal diffusion
- Photometric Amplitude Distribution of Stellar Rotation of Kepler KOIs-Indication for Spin-Orbit Alignment of Cool Stars and High Obliquity for Hot Stars
- Formation of close in Super-Earths \& Mini-Neptunes: Required Disk Masses \& Their Implications
- Global Models of Planet Formation and Evolution
- Magnetic Flux Concentration and Zonal Flows in Magnetorotational Instability Turbulence
- An Atmospheric Structure Equation for Grain Growth
- Layered convection as the origin of Saturn's luminosity anomaly
- Evolution of Migrating Planets Undergoing Gas Accretion
- Dynamical corotation torques on low-mass planets
- Recovery of the Candidate Protoplanet HD 100546 b with Gemini/NICI and Detection of Additional (Planet-Induced?) Disk Structure at Small Separations
- A reassessment of the in situ formation of close-in super-Earths
- Grain opacity and the bulk composition of extrasolar planets. II. An analytical model for the grain opacity in protoplanetary atmospheres
- Determination of Three-dimensional Spin-orbit Angle with Joint Analysis of Asteroseismology, Transit Lightcurve, and the Rossiter-McLaughlin Effect: Cases of HAT-P-7 and Kepler-25
- Saturated torque formula for planetary migration in viscous disks with thermal diffusion: recipe for protoplanet population synthesis
- Grain opacity and the bulk composition of extrasolar planets. I. Results from scaling the ISM opacity
- Rapid Formation of Icy Super-Earths and the Cores of Gas Giant Planets
- On the gap-opening criterion of migrating planets in protoplanetary disks
- Testing Disk Instability Models for Giant Planet Formation
- Ohmic Dissipation in the Interiors of Hot Jupiters
- The dynamical role of the circumplanetary disc in planetary migration
- Deuterium burning in objects forming via the core accretion scenario - Brown dwarfs or planets?
- Constraining the Oblateness of Kepler Planets
- Spin-Orbit angle distribution and the origin of (mis)aligned hot Jupiters
- Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion
- Stellar irradiated discs and implications on migration of embedded planets III: viscosity transitions
- Numerical simulations of the type III migration:I. Disc model and convergence tests
- Spectral Energy Distributions of Accreting Protoplanets
- On type-I migration near opacity transitions. A generalized Lindblad torque formula for planetary population synthesis
- Understanding the assembly of Kepler's compact planetary systems
- Giant Planet Formation
- Type I Planet Migration in a Magnetized Disk. I. Effect of Large-Scale Vertical and Azimuthal Field Components
Cited by in corpus (55)
- Molecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and Highlights
- Compositional imprints in density-distance-time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation
- Observing transiting planets with JWST -- Prime targets and their synthetic spectral observations
- The New Generation Planetary Population Synthesis (NGPPS). I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems
- Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics
- Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation
- The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical results
- Planetary evolution with atmospheric photoevaporation I. Analytical derivation and numerical study of the evaporation valley and transition from super-Earths to sub-Neptunes
- How much does turbulence change the pebble isolation mass for planet formation?
- Rings and gaps in the disc around Elias 24 revealed by ALMA
- Catching drifting pebbles I. Enhanced pebble accretion efficiencies for eccentric planets
- Investigating the young AU~Mic system with SPIRou: large-scale stellar magnetic field and close-in planet mass
- Planetary population synthesis
- An Optical/near-infrared investigation of HD 100546 b with the Gemini Planet Imager and MagAO
- DREAM I. Orbital architecture orrery
- Effects of the Planetary Temperature on the Circumplanetary Disk and on the Gap
- One year of AU Mic with HARPS: II -- stellar activity and star-planet interaction
- An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561
- The determination of protoplanetary disk masses
- The Planetary Accretion Shock. II. Grid of Post-Shock Entropies and Radiative Shock Efficiencies for Non-Equilibrium Radiation Transport
- Transmission spectroscopy and Rossiter-McLaughlin measurements of the young Neptune orbiting AU Mic
- Planet formation around M dwarfs via disc instability: Fragmentation conditions and protoplanet properties
- A wide-orbit giant planet in the high-mass b Centauri binary system
- Mapping the exo-Neptunian landscape. A ridge between the desert and savanna
- The contribution of the ARIEL space mission to the study of planetary formation
- Planetary Population Synthesis and the Emergence of Four Classes of Planetary System Architectures
- 3D Simulations of Planet Trapping at Disc-Cavity Boundaries
- TOI-5005 b: A super-Neptune in the savanna near the ridge
- The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres. No evidence of enhanced evaporation in young planets
- Pebble Accretion in Turbulent Protoplanetary Disks
- Chemical inhomogeneities in the Pleiades: signatures of rocky-forming material in stellar atmospheres
- The influence of infall on the properties of protoplanetary discs
- The Metallicity-Period-Mass Diagram of low-mass exoplanets
- Dusty disc-planet interaction with dust-free simulations
- Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD235088 b (TOI-1430 b) with CARMENES
- Observational signatures of eccentric Jupiters inside gas cavities in protoplanetary discs
- An intermediate-luminosity-optical-transient (ILOT) model for the young stellar object ASASSN-15qi
- Migrating Low-Mass Planets in Inviscid Dusty Protoplanetary Discs
- Characterisation of the Warm-Jupiter TOI-1130 system with CHEOPS and photo-dynamical approach
- Creating retrogradely orbiting planets by prograde stellar fly-bys
- Effects of Radiative Diffusion on the Dynamical Corotation Torque in Three-Dimensional Protoplanetary Disks
- Simulated mass measurements of the young planet K2-33b
- How the planetary eccentricity influences the pebble isolation mass
- ATREIDES I. Embarking on a trek across the exo-Neptunian landscape with the TOI-421 system
- ODEA: Orbital Dynamics in a complex Evolving Architecture -- Application to the planetary system HD 106906
- The Likelihood of Detecting Young Giant Planets with High Contrast Imaging and Interferometry
- Calibrated Gas Accretion and Orbital Migration of Protoplanets in 1D Disc Models
- RW Aur A : SpeX Spectral Evidence for Differentiated Planetesimal Formation, Migration and Destruction in an 3 Myr Old Excited CTTS System
- The New Generation Planetary Population Synthesis (NGPPS). VII. Statistical comparison with the HARPS/Coralie survey
- Hidden under a warm blanket: If planets existed in protostellar disks, they would hardly produce observable substructures
- Planetesimals drifting through dusty and gaseous white dwarf debris discs: Types I, II and III-like migration
- TOI-1743 b, TOI-5799 b, TOI-5799 c and TOI-6223 b: TESS discovery and validation of four super-Earth to Neptune-sized planets around M dwarfs
- A high stellar multiplicity rate amongst TESS planet candidates in the Neptunian desert using Gaia DR3 astrometry
- Chemical diversity of the atmospheres and interiors of sub-Neptunes: a case study of GJ 436 b
- Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation