Computational Habitability

Computational Habitability

UW Astrobiology via YouTube Direct link

Intro

1 of 8

1 of 8

Intro

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Computational Habitability

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

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