12.472
Building Earth-like Planets: From Nebular Gas to Ocean Worlds
Fall 2008
Topics
- Introduction
- Dust clouds, star formation
- What is a good question?
- Stars and disks
- Dust accretion
- Accretion signatures, T-Tauri disks, lifetimes, compositions
- Orderly and runaway growth
- Integrated model of the planetary disk
- Efforts to model accretion
- Differentiation I
- Differentiation II
- Planetesimals
- Planetesimals: compositions and distributions
- Effects of the star
- Moons
- Melting from the outside and the inside
- Magma ocean processes
- Exoplanet systems
- Volatiles
- Planetary crusts
- Venus, Mercury, Earth, Mars — surfaces
- Venus, Mercury, Earth, Mars — interiors
- Habitability and biosignatures
- Ocean worlds
- Desert worlds
Readings
- Safronov, V. S. Evolution of the Protoplanetry Cloud and Formation of the Earth and the Planets . Jerusalem, Israel: Israel Program for Scientific Translations, 1972. ISBN: 9780706512250.
- Albarède Francis, and Janne Blichert-Toft. “The Split Fate of the Early Earth, Mars, Venus, and Moon.” C. R. Geoscience 339, nos. 14-15 (2007): 917-927.
Sources
- Course catalogue ↗Historical OpenCourseWare
- MIT OCW syllabus ↗
- MIT OCW readings ↗
- MIT OCW calendar ↗
- Historical MIT OpenCourseWare offering. Named reading entries and schedule topics are automatically extracted from the linked source pages.