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Origins of Giant Planets, Volume 2

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These books will provide a comprehensive overview of giant planet formation, aimed at graduate students and postdocs beginning research on the topic. They will also be a useful reference for obser...
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  • 01 September 2023
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These books will provide a comprehensive overview of giant planet formation, aimed at graduate students and postdocs beginning research on the topic. They will also be a useful reference for observers seeking to interpret their images of young, forming planets or disk features that may be planet indicators. The books will also highlight processes that are not well understood, present new project ideas, and make predictions that can be tested by new models or observations. . This volume begins by explaining how the gravitational fields of the large planetesimals pave the way for the emergence of Mars-sized planetary embryos. Next comes an investigation of gaseous atmosphere accretion, which completes the giant planet formation process. The book concludes by examining the behavior of newly-formed gas giants, including gap opening, migration, and planet survival rate.

Key Features:
  • Provides a comprehensive overview of giant planet formation
  • All theories are compared with observational results
  • Includes discussions of chemistry as well as gravitational dynamics and thermal physics
  • Suggests productive avenues for future research 
  • Well timed to be available to JWST observers
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Price: £99.00
Pages: 200
Publisher: Institute of Physics Publishing
Imprint: Institute of Physics Publishing
Publication Date: 01 September 2023
ISBN: 9780750348188
Format: eBook
BISACs:

SCIENCE / Space Science / Astronomy, Solar system: the Sun and planets

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Chapter 1: Solid core growth • Safronov’s equation • Velocity dispersion and gravitational focusing • Pebble accretion • Runaway vs. oligarchic growth • Isolation mass • Effects of Type I migration • Efficiency of solid accretion Chapter 2: Gas accretion • The Bondi sphere • Ablation, core/envelope mixing, and atmospheric opacity • Quasi-hydrostatic solutions • The role of dynamical heating • Timescale and efficiency of gas accretion • Effects of Type III migration • Crossover mass and transition to runaway growth Chapter 3: The last stages of giant planet growth • Gap opening and the role of disk viscosity • Late-stage planetesimal accretion • Effects of Type II migration • Resonant interactions • What fraction of giant planets survive? • Accretion shutdown and Kelvin-Helmholz contraction