Growth of Jupiter: Enhancement of core accretion by a voluminous low-mass envelope

@article{DAngelo2014GrowthOJ,
  title={Growth of Jupiter: Enhancement of core accretion by a voluminous low-mass envelope},
  author={Gennaro D’Angelo and S. J. Weidenschilling and Jack J. Lissauer and Peter H. Bodenheimer},
  journal={Icarus},
  year={2014},
  volume={241},
  pages={298-312}
}
View PDF on arXiv
19 Citations
Background Citations
5
Methods Citations
2

19 Citations

Growth of Jupiter: Formation in disks of gas and solids and evolution to the present epoch
CAPTURE AND EVOLUTION OF PLANETESIMALS IN CIRCUMJOVIAN DISKS
We study the evolution of planetesimals in evolved gaseous disks that orbit a solar-mass star and harbor a Jupiter-mass planet at a p ≈ 5 ?> AU. The gas dynamics are modeled with a three-dimensional…
Exploring the conditions for forming cold gas giants through planetesimal accretion
The formation of cold gas giants similar to Jupiter and Saturn in orbit and mass is a great challenge for planetesimal-driven core accretion models because the core growth rates far from the star are…
Detailed Calculations of the Efficiency of Planetesimal Accretion in the Core-accretion Model
We present the results of a study of the accretion rate of planetesimals by a growing proto-Jupiter in the core-accretion model. The purpose of our study is to test the assumptions of Pollack et al.…
Forming Planets via Pebble Accretion
The detection and characterization of large populations of pebbles in protoplanetary disks have motivated the study of pebble accretion as a driver of planetary growth. This review covers all aspects…
IN SITU AND EX SITU FORMATION MODELS OF KEPLER 11 PLANETS
We present formation simulations of the six Kepler 11 planets. Models assume either in situ or ex situ assembly, the latter with migration, and are evolved to the estimated age of the system, .…
Effects of the Planetary Temperature on the Circumplanetary Disk and on the Gap
Circumplanetary disks (CPDs) regulate the late accretion to the giant planet and serve as the birthplace for satellites. Understanding their characteristics via simulations also helps to prepare for…
Particle accretion onto planets in discs with hydrodynamic turbulence
The growth process of protoplanets can be sped up by accreting a large number of solid, pebble-sized objects that are still present in the protoplanetary disc. It is still an open question on how…
Disk masses around solar-mass stars are underestimated by CO observations
Gas in protostellar disks provides the raw material for giant planet formation and controls the dynamics of the planetesimal-building dust grains. Accurate gas mass measurements help map the observed…
Circumstellar Dust Distribution in Systems with Two Planets in Resonance
We investigate via numerical modeling the effects of two planets locked in resonance, and migrating outward, on the dust distribution of the natal circumstellar disk. We aim to test whether the dust…
...
...

References

SHOWING 1-10 OF 82 REFERENCES
Rapid growth of gas-giant cores by pebble accretion
The observed lifetimes of gaseous protoplanetary discs place strong constraints on gas and ice giant formation in the core accretion scenario. The approximately 10-Earth-mass solid core responsible…
Formation of gas giant planets: core accretion models with fragmentation and planetary envelope
Giant planet formation with pebble accretion
DEUTERIUM BURNING IN MASSIVE GIANT PLANETS AND LOW-MASS BROWN DWARFS FORMED BY CORE-NUCLEATED ACCRETION
Using detailed numerical simulations, we study the formation of bodies near the deuterium-burning limit according to the core-nucleated giant planet accretion scenario. The objects, with…
Timescales for planetary accretion and the structure of the protoplanetary disk
Calculations of the accretion and evolution of giant planets: The effects of solid cores
Oligarchic planetesimal accretion and giant planet formation
Aims. In the context of the core instability model, we present calculations of in situ giant planet formation. The oligarchic growth regime of solid protoplanets is the model adopted for the growth…
Models of Jupiter's growth incorporating thermal and hydrodynamic constraints
Accretion of the gaseous envelope of Jupiter around a 5–10 Earth-mass core
Models of the in Situ Formation of Detected Extrasolar Giant Planets
Abstract We present numerical simulations of the formation of the planetary companions to 47 UMa, ρ CrB, and 51 Peg. They are assumed to have formed in situ according to the basic model that a core…
...
...