Internal Structure of Giant and Icy Planets: Importance of Heavy Elements and Mixing
arXiv:1705.09320 · doi:10.1007/978-3-319-55333-7_44
Abstract
In this chapter we summarize current knowledge of the internal structure of giant planets. We concentrate on the importance of heavy elements and their role in determining the planetary composition and internal structure, in planet formation, and during the planetary long-term evolution. We briefly discuss how internal structure models are derived, present the possible structures of the outer planets in the Solar System, and summarise giant planet formation and evolution. Finally, we introduce giant exoplanets and discuss how they can be used to better understand giant planets as a class of planetary objects.
Invited review chapter, accepted for publication in "Handbook of Exoplanets"
References in corpus (21)
- Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core
- Ab initio Equation of State data for hydrogen, helium, and water and the internal structure of Jupiter
- A Massive Core in Jupiter Predicted From First-Principles Simulations
- Heat transport in giant (exo)planets: a new perspective
- Planet formation with envelope enrichment: new insights on planetary diversity
- Saturn Ring Seismology: Evidence for Stable Stratification in the Deep Interior of Saturn
- Phase separation in hydrogen-helium mixtures at Mbar pressures
- Layered convection as the origin of Saturn's luminosity anomaly
- Uranus evolution models with simple thermal boundary layers
- A Preliminary Jupiter Model
- On the Origin of HD149026b
- Jupiter internal structure: the effect of different equations of state
- Jupiter's formation and its primordial internal structure
- The Evolution and Internal Structure of Jupiter and Saturn with Compositional Gradients
- Understanding Jupiter's Interior
- An Exploration of Double Diffusive Convection in Jupiter as a Result of Hydrogen-Helium Phase Separation
- Convection and Mixing in Giant Planet Evolution
- Saturn's fast spin determined from its gravitational field and oblateness
- Measuring Jupiter's water abundance by Juno: the link between interior and formation models
- Bayesian Evolution Models for Jupiter with Helium Rain and Double-diffusive Convection
- On the Radius Anomaly of Hot Jupiters: Reexamination of the Possibility and Impact of Layered Convection
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- How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes
- Uranus and Neptune are key to understand planets with hydrogen atmospheres
- The deep composition of Uranus and Neptune from in situ exploration and thermochemical modeling
- A Possible Mechanism to Explain the Prograde Equatorial Jet of a Jupiter-like Gaseous Giant