Planetary habitability
Planetary habitability is the measure of a planet's or a natural satellite's potential to develop and maintain environments that are hospitable to life.[1]
Planetary Habitability Media
A visualization showing a simple model of Earth's magnetic field.
The Atacama Desert in South America provides an analog to Mars and an ideal environment to study the boundary between sterility and habitability.
Relative star sizes and photospheric temperatures. Any planet around a red dwarf such as the one shown here (Gliese 229A) would have to huddle close to achieve Earth-like temperatures, probably inducing tidal locking. See Aurelia. Credit: MPIA/V. Joergens.
An artist's impression of GJ 667 Cc, a potentially habitable planet orbiting a red dwarf constituent in a trinary star system.
References
- ↑ Dyches, Preston; Chou, Felcia (7 April 2015). "The Solar System and Beyond is Awash in Water". NASA. Retrieved 8 April 2015.