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Planetary Dynamics: Teegarden's Star's Planets' Obliquities
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Classroom Contents
Computational Habitability
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- 1 Intro
- 2 The Atmosphere: Water Photolysis and Hydrogen Escape
- 3 The Interior. The Thermal/Magnetic/Volatile Evolution of Venus
- 4 The Surface: Ice Coverage of Earth-like Exoplanets
- 5 The Planetary System: Orbital Evolution in a Resonance
- 6 The Star: Planets Orbiting Tidally Evolving Binary Stars
- 7 Planetary Dynamics: Teegarden's Star's Planets' Obliquities
- 8 History and Habitability of the LP 890-9 Planetary System
