Lecture notes on the formation and early evolution of planetary systems
arXiv:astro-ph/0701485
Abstract
These notes provide an introduction to the theory of the formation and early evolution of planetary systems. Topics covered include the structure, evolution and dispersal of protoplanetary disks; the formation of planetesimals, terrestrial and gas giant planets; and orbital evolution due to gas disk migration, planetesimal scattering, planet-planet interactions, and tides.
Based on lectures given at the University of Colorado, Boulder. Last revised February 2017. Published, in modified form, as "Astrophysics of Planet Formation" (Cambridge University Press)
References in corpus (5)
- Tidal dissipation in stars and giant planets
- Dynamics of Solids in the Midplane of Protoplanetary Disks: Implications for Planetesimal Formation
- Formation of Jupiter using opacities based on detailed grain physics
- Secular Effects of Tidal Damping in Compact Planetary Systems
- Magnetohydrodynamics of Protostellar Disks
Cited by in corpus (17)
- The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
- Solar structure and evolution
- Planet formation in Alpha Centauri A revisited: not so accretion-friendly after all
- Relative velocities of inertial particles in turbulent aerosols
- Hydrogen Axion Star: Metallic Hydrogen Bound to a QCD Axion BEC
- Circumstellar disks and planets. Science cases for next-generation optical/infrared long-baseline interferometers
- Super-Earths: A New Class of Planetary Bodies
- Second generation planets
- Planetary Migration in Protoplanetary Disks
- AGN flares as counterparts to LIGO/Virgo mergers: No confident causal connection in spatial correlation analysis
- Clump formation due to the gravitational instability of a multiphase medium in a massive protoplanetary disc
- Statistical model for collisions and recollisions of inertial particles in mixing flows
- Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit
- The structure of young embedded protostellar discs
- An upper limit for the growth of inner planets?
- Gravitational Radiation Driven Supermassive Black Hole Binary Inspirals as Periodically Variable Electromagnetic Sources
- Impact of Gas Giant Instabilities on Habitable Planets