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Old 04-28-2006, 04:23 PM   #29
Sternwallow
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Quote:
logarithm wrote
Quote:
Sternwallow wrote
Quote:
logarithm wrote
Your general solar evolution allows production of elements up to iron by fusion. After that, things go haywire, and a reasonable rate is impossible. That's generically where the death starts to occur. As Choobus says, then all the heavier stuff gets formed, eventually, when the star goes "ker-flooey" and snots all over the place.
Do you have available the contribution to intergalactic recession velocity caused by cosmic snot?
:lol::lol::lol::lol:
Yes, but you are going to have to give me a snootful of unobtanium for the answer.
Oh dear, what is the current rate of exchange between unobtanium and gold-presslatinum?

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