Inhalt / Plan
- Introduction
- Subject of this course
- Relation to other courses
- Prerequisites
- Literature
- Logistics
- Historical overview
- From antiquity to Copernicus
- From Descartes to Laplace
- Theories of the 20th century
- Observational revolution of 1990s
- Present state of the theory
- From clouds to disks
- GMCs and star-forming regions
- The Jeans criterion
- From clouds to cores
- Angular momentum problem
- From cores to disks
- Timescales
- Protoplanetary disks - hydrodynamics
- Hydrodynamics
- Viscosity and angular momentum
- Equations of viscous accretion
- Protoplanetary disks - physics and structure
- Shakura-Sunyaev model
- Viscosity and turbulences
- Disk structure
- Disk observations
- Protoplanetary disks - lifetimes and masses
- Disk lifetimes
- Disk masses
- Disk stability
- Two scenarios of planet formation
- Dust-gas interactions
- Condensation of solids
- Forces on dust grains
- Vertical motion: sedimentation
- Stopping time and settling time
- Vertical motion: settling-mixing
- Radial motion: drift
- Dust in the midplane
- From dust to planetesimals
- Observations, experiments, modeling
- Sticking or Goldreich-Ward instability?
- Dust morphology
- From 1 micron to 1 mm
- From 1 mm to 1 m
- From 1m to 1km
- From planetesimals to planetary embryos
- Kinematics of a planetesimal swarm
- Runaway growth
- Oligarchic growth
- Isolation of oligarchs
- From embryos to planets
- Formation of Juipter and Saturn
- Formation of Uranus and Neptune
- Endgame for terrestrial planets
- Hot Jupiters and migration
- Demographics of extrasolar planets
- Disk-planet interactions
- Type I migration
- Type II migration
- Type III migration
- Discussion of migration
- Other exoplanet populations
- Super-Earths
- Resonant systems
- Eccentric planets
- Inclined planets
- Massive distant planets
- Left-over planetesimals
- Asteroid belt, EKB, and Oort cloud
- Basic features of the Kuiper belt
- Dynamical evolution of the Kuiper belt
- Late heavy bombardment
- Debris disks
- What are debris disks?
- Observations: Vega phenomenon, resolved examples, statistics
- Internal physics of debris disks
- Debris disks and gas
- Debris disks and small bodies
- Debris disks and planets
Die Inhaltsangabe ist nicht verbindlich und kann entsprechend der Gegebenheiten abgeändert werden
The contents is subject to change
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