Models of Giant Planet formation with migration and disc evolution

Abstract

We present a new model of giant planet formation that extends the core-accretion model of Pollack etal (1996) to include migration, disc evolution and gap formation. We show that taking into account these effects can lead to a much more rapid formation of giant planets, making it compatible with the typical disc lifetimes inferred from observations of young circumstellar discs. This speed up is due to the fact that migration prevents the severe depletion of the feeding zone as observed in in situ calculations. Hence, the growing planet is never isolated and it can reach cross-over mass on a much shorter timescale. To illustrate the range of planets that can form in our model, we describe a set of simulations in which we have varied some of the initial parameters and compare the final masses and semi-major axes with those inferred from observed extra-solar planets.

Accepted in Astronomy & Astrophysics

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• Heavy-element Accretion by Proto-Jupiter in a Massive Planetesimal Disk, Revisited
• Building protoplanetary disks from the molecular cloud: redefining the disk timeline
• The influence of general-relativity effects, dynamical tides and collisions on planet-planet scattering close to the star
• Radial Distribution of Planets. Predictions based on the Core Accretion Gas Capture Planet formation Model
• Photoevaporation of the Jovian circumplanetary disk I. Explaining the orbit of Callisto and the lack of outer regular satellites
• N-body simulations of terrestrial planet growth with resonant dynamical friction
• A coronagraphic search for wide sub-stellar companions among members of the Ursa Major moving group
• Modeling Planetary System Formation with N-Body Simulations: Role of Gas Disk and Statistics Comparing to Observations
• Internal Structure of Giant and Icy Planets: Importance of Heavy Elements and Mixing
• HD 83443c: A highly eccentric giant planet on a 22-year orbit
• Assessing the processes behind planet engulfment and its imprints
• Difficulty in Formation of Counter-orbiting Hot Jupiters from Near-coplanar Hierarchical Triple Systems: A Sub-stellar Perturber
• Radial Drift and Concurrent Ablation of Boulder-Sized Objects
• The Likelihood of Detecting Young Giant Planets with High Contrast Imaging and Interferometry
• Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-stars
• DIPSY: A new Disc Instability Population SYnthesis, II. The Populations of Companions Formed Through Disc Instability
• Terrestrial Planet Formation in Extra-Solar Planetary Systems
• Formation and Dynamical Evolution of the Neptune Trojans - the Influence of the Initial Solar System Architecture
• Unveiling wide-orbit companions to K-type stars in Sco-Cen with Gaia EDR3
• The influence of planetesimal fragmentation on planet formation
• Calibrated Gas Accretion and Orbital Migration of Protoplanets in 1D Disc Models
• The long wavelength view of GG Tau A: Rocks in the Ring World
• Searching for Hot Water World Candidates with CHEOPS: Refining the radii and analysing the internal structures and atmospheric lifetimes of TOI-238 b and TOI-1685 b
• Possible Outcomes of Coplanar High-eccentricity Migration: Hot Jupiters, Close-in Super-Earths, and Counter-orbiting Planets
• Theoretical planetary mass spectra - a predition for COROT
• The New Generation Planetary Population Synthesis (NGPPS). VII. Statistical comparison with the HARPS/Coralie survey
• MOA-2019-BLG-008Lb: a new microlensing detection of an object at the planet/brown dwarf boundary
• Type I migration in optically thick accretion discs
• Increased isolation mass for pebble accreting planetary cores in pressure maxima of protoplanetary discs
• Relative occurrence rates of terrestrial planets orbiting FGK stars
• The paradox of youth for ALMA planet candidates
• Planet Formation
• DIPSY: A new Disc Instability Population SYnthesis, I. Modeling, evolution of individual systems, and tests
• The New Generation Planetary Population Synthesis (NGPPS) VIII. Impact of host star metallicity on planet occurrence rates, orbital periods, eccentricities, and radius valley morphology
• Formation and tidal evolution of hot super-Earths in multiple planetary systems
• New Dynamical State and Habitability of the HD 45364 Planetary System
• Space based microlensing planet searches
• The PAIRS project: a global formation model for planets in binaries. II. Gravitational perturbation effects from secondary stars
• The PAIRS project: a global formation model for planets in binaries. I. Effect of disc truncation on the growth of S-type planets
• Planet Formation Imager (PFI): science vision and key requirements
• Understanding exoplanet formation, structure and evolution in 2010
• Disk dissipation, giant planet formation and star-formation-rate fluctuations in the past three-million-year history of Gould's Belt
• Adapting a gas accretion scenario for migrating planets in FARGO3D
• Architecture of planetary systems predicted from protoplanetary disks observed with ALMA II: evolution outcomes and dynamical stability
• MANGOS II: Five new giant planets orbiting low-mass stars
• Survival of satellites during the migration of a Hot Jupiter
• Planetary population synthesis
• Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
• Dust photophoretic transport around a T Tauri star: Implications for comets composition
• The Effect of Accretion Rate and Composition on the Structure of Ice-rich Super-Earths
• Radial velocity analysis of stars with debris discs
• ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791
• The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog
• Adapting a solid accretion scenario for migrating planets in FARGO3D
• Compositional Turbulence and Layering in the Gaseous Envelopes of Forming Planets
• On the Period-Ratio-Mass-Ratio Correlation of Extra-Solar Multi-Planet Systems
• Planets in Spin-Orbit Misalignment and the Search for Stellar Companions
• Searching for GEMS: Three warm Saturns and a super-Jupiter orbiting four early M-dwarfs
• AU Mic b is the Youngest Planet to have a Spin-Orbit Alignment Measurement
• Planetesimal fragmentation and giant planet formation: the role of planet migration
• GENGA II: GPU planetary N-body simulations with non-Newtonian forces and high number of particles
• TOI-6884b: A low-mass brown dwarf transiting a slightly evolved star
• Rapid and Predictive Planet Population Synthesis Model (RAPPS) I. Upgraded model and resulting synthetic populations
• Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b
• Panchromatic View of the Frigid Jovian Exoplanet COCONUTS-2 b