| |
| | SPACE.com -- SETI"s Planetary Instruction Kit: Venus and Mars |
 | | By dissolving carbon dioxide and re-releasing it into the atmosphere, the oceans can be thought of as controlling the temperature of our planet (this process is, of course, much more complex). |
 | | When water vapor reached the upper atmosphere, the ultraviolet light from the Sun would break it into its components -- oxygen and hydrogen -- the latter of which escaped into space. |
 | | As Venus oceans were evaporating, their carbon dioxide was released into the atmosphere, which caused increasing heat, which, in turn, caused increasing evaporation, and so on. |
| www.space.com /searchforlife/seti_solarsystem_three_010216.html (843 words) |
|