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#21 |
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Join Date: Feb 2005
Location: Berkeley, CA
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It's when current generation stars form. First generation stars formed at higher temperatures, but you're not going to get planetary systems around first generation stars.
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#22 |
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Join Date: Aug 2007
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In addition, planets around first generation stars would be hydrogen and helium only.
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Fred Brackin |
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#23 | |
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Join Date: Jun 2005
Location: Lawrence, KS
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Quote:
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Bill Stoddard I don't think we're in Oz any more. |
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#24 |
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Join Date: Jun 2005
Location: Lawrence, KS
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So, okay, on one hand, mean energy per unit volume varies as L^(-4). On the other hand, minimum mass for gravitational collapse to form a solar system varies as T^(3/2). To link the two, we need a conversion between energy and temperature.
* In basic thermo, temperature was defined as mean molecular kinetic energy, which would suggest that T is proportional to E, probably using Boltzmann's constant or the ideal gas constant. * In blackbody radiation, energy radiated per unit time is proportional to T^4. * However, the universe doesn't seem to be radiating into anything other than itself. I believe the proportionality for energy *content* in a medium is that internal radiation is proportional to T^3. Which of these gives the right scaling relationship?
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Bill Stoddard I don't think we're in Oz any more. |
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#25 |
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Join Date: Jan 2005
Location: Gothenburg, Sweden
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The first stars formed when the universe was about 200 million years after the Big Bang. How hot would the CMB be then.
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“When you arise in the morning think of what a privilege it is to be alive, to think, to enjoy, to love ...” Marcus Aurelius Author of Winged Folk. The GURPS Discord. Drop by and say hi! |
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| Tags |
| cmbr, space, spaceships, worldbuilding |
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