| http://www.w3.org/ns/prov#value | - by Crucis on Sun 06 Sep 2009 00:06 I was thinking about the Blackbody Temp formula ( Temp = K * (SUM [L / (g * a^2)]) ^ 0.25; where a = radius of the planet's orbit in LM, from the star), when it occurred to me that there is a rather serious problem with the SUM'ing portion of the formula.The SUM'ing portion of this formula exists to merge the effects of the various stars' luminosities in a poly-s
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