the drake equation - high point university
TRANSCRIPT
The Drake Equation
~5%-15% of Sun-like stars are directlyobserved to have exoplanets.
Term #2
But is 0.05-0.15 a reasonable estimate?(No, because detection methods have known shortcomings).
The Drake Equation
Number of exoplanets per planet-hosting star that could potentially support life.
(# of Earth-like exoplanets per planet-hosting star)
Term #3
Let’s look at our Solar System firstsince it’s the only place where life definitely exists.
sizes to scale, distances not to scale!
Some Basic Requirements for Life?• Stable source of energy (long−lived, low−mass stars best)
• Raw materials for complex chemistry
• Location for life to emerge (solid surfaces, atmosphere)
• Benign environmental conditions (low UV radiation, etc.)
• Water?
• Magnetic field?
The Solar System’s Habitable Zone
Habitable Zone:Region around a star in which it is possible for a
planet to have liquid water
Inside the zone, it’s too hot.
Outside the zone, it’s too cold.
The extent of the habitable zone depends on the star’s luminosity.It also changes as a star evolves.
Image is to scale
Habitable Zone Simulator
http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html
Eccentric (non-circular) orbits can be a problem
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http://astro.unl.edu/classaction/animations/renaissance/kepler.html
Start animation on Kepler’s first law below. Increase eccentricity and think about why high e value might be bad.
The Galactic Habitable Zone
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http://astro.unl.edu/naap/habitablezones/animations/milkyWayHabitability.html