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[QUOTE]Originally posted by E. Cartman: [QB] M-class planet density depends on the number of main sequence stars in the same spectral class as our Sun. Earth-like worlds can only exist (as far as we know) around stars that exhibit a very narrow band of characteristics - ruling out all types except F8, G0 through G10, and K1. Together, these account for approximately 0.05[b]%[/b] of the total galactic composition, so decade-spanning terraforming projects would likely remain a necessity... most stars don't even have any orbiting companions. :) [/QB][/QUOTE]
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