How would you calculate the habitable surface area on Gliese 667 Cc?
How could I calculate the habitable bounds, in relation to temperature, near the twilight zone of Gliese 667 Cc? Assuming an Earth-like atmosphere and no tidal working.
Here are the numbers that I have been using:
- Parent star Temperature =
- Distance from star =
- Radius =
- Surface area =
I have little experience in astrophysics, or basic physics for that matter, so my understanding of heat dissipation through space is poor at best. In my mind, since I have the temperature of a heat source, a distance to the center of the planet, and the planet's farthest points from the center (25.4 million km ± 9,800 km), it wouldn't be difficult to calculate if you understood radiant flux and such.
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