http://phl.upr.edu/projects/habitable-exoplanets-catalog/dat...
http://phl.upr.edu/projects/habitable-exoplanets-catalog/dat...
water habitable zone
ultraviolet habitable zone
photosynthetic habitable zone
ozone habitable zone
planetary rotation rate habitable zone
planetary obliquity habitable zone
tidal habitable zone
astrosphere habitable zone
I just feel everyone gets excited over nothing solely because its extra-solar. Our own solar system is fairly diverse. If life was common, we'd probably be seeing more of it here.
We'll have a better picture when we study our solar system in more detail. Maybe 100 years? I agree that speculation this early in the game isn't enough to get excited over.
For example, "tidal habitable zone" doesn't mean "we need [ocean] tides to survive," it means "tidal heating effects have an enormous impact on planetary conditions". For example, an Earth analogue in orbit around a tiny red dwarf in a seemingly "habitable zone" would be subject to tidal heating effects which would bake the surface, whereas a similar planet in a similar orbit around a sun-like yellow dwarf would not.
Similarly, "rotation rate habitable zone" doesn't mean "the planet must have a ~24 hour day", it means "all else being equal, a planet's rotation rate can greatly affect habitability," mostly due to weather patterns and air/heat circulation. By including rotation rate in our models, some planets previously thought to be inhabitable may turn out not to be, and vice versa.
http://www.windows2universe.org/glossary/plasmaspheric_gain....