Planetenentstehung / Planet Formation 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 Initial phase Star-forming regions Collapsing clouds and the Jeans criterion Contraction, accretion, and fragmentation Rotation and angular momentum Flattening of the cloud Timescales Formation and evolution of a gas disk Hydrodynamics Formation of a star and a disk Viscosity and angular momentum Equations of viscous accretion Shakura-Sunyaev model Disk structure and stability Disk dispersal Observations of protoplanetary disks Observation methods Evolutionary classes Disk mass estimates Disk lifetimes Dust-gas interactions Forces on dust grains Vertical motion: sedimentation Stopping time and settling time Vertical motion: settling-mixing Radial motion: drift Goldreich-Ward and shear-induced instabilities 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 Gas damping of velocities Isolation of oligarchs From embryos to planets The timescale problem Critial core mass Growth of gas envelopes Formation of Uranus and Neptune Endgame for terrestrial planets Hot Jupiters and large eccentricities Statistics of extrasolar planets Disk-planet interactions Type I migration Type II migration Type III migration Comparison of migration types Survival strategies for planets Large eccentricity issue Planetary rotation, satellites and rings Planetary rotation Satellites of giant planets Satellites of terrestrial planets Ring systems of giant planets Left-over planetesimals Asteroid belt, EKB, and Oort cloud Disk cleanup and formation of Oort cloud Dynamical sculpturing of the asteroidal belt and EKB Size distribution and total mass of EKB 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 Synthesis and issues not covered A general scheme of the "standard" scenario and its bottle necks An alternative instability scenario (Kuiper-Cameron-Boss) Planets in binary systems Planets around neutron stars Habitability of planets and astrobiology Die Inhaltsangabe ist nicht verbindlich und kann entsprechend der Gegebenheiten abgeändert werden The contents is subject to change