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Why don't stars explode? What holds them together? |
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| Nov11-05, 10:32 PM | #18 |
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Why don't stars explode? What holds them together? |
| Nov11-05, 10:39 PM | #19 |
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| Nov11-05, 11:32 PM | #20 |
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| Nov11-05, 11:50 PM | #21 |
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| Nov12-05, 12:53 PM | #22 |
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Thanks, Tiger. I knew that there was something wrong with my post. Those sequential thingies always mess me up.
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| Nov12-05, 06:42 PM | #23 |
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Some Lithium could be produced within about three minutes of the big bang, but most is the cosmic ray-to carbon collisions after carbon is formed many years after the big bang from reactions in the cores of stars.
From: UCLA we get that: So, if that's the case and order of formation, when do we consider the "big bang" to be in process? One second, one minute, three minutes (as in the book name) ? This is just a general (and pickey) question that I haven't seen brought up before; how much time after zero is the BB still considered to be in process?.. Anyone answer.
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| Nov12-05, 07:38 PM | #24 |
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| Nov12-05, 07:48 PM | #25 |
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The pressure comes from the intense heat/temperature which comes from the fusion reactions. Fusion reactions produce energy on the order of 1 MeV and at 11605 K/ev, that's about 11 billion K. However, only a fraction of mass is fusing at a given time, so that kinetic energy of the fusion reactants is dissipated quickly to the various atoms and electrons nearby. Temperature of the sun's core is estimated to be ~13.6 MK, and the corona temperature is about 5 MK, while the photosphere 'surface' temperature is about 5800 K. For information on pp and CNO chain reactions see - http://csep10.phys.utk.edu/astr162/l...gy/cno-pp.html http://burro.astr.cwru.edu/Academics...s/ppchain.html http://www.shef.ac.uk/physics/people...3_fusion3.html ----------------------------------------------- Re: Li production (is it necessary that most(?) Li was formed around time of BB as opposed to stars later on or novae?) p + 9Be -> 4He + 6Li d + 4He -> 6Li t + 6Li -> 7Li + d (or p +n) There is a paper "Influence of Gravity Waves on the Internal Rotation and Li Abundance of Solar-Type Stars" by Corinne Charbonnel and Suzanne Talon in Science mag, but I can't access it since I am not a member. Anyone read this? Ann Merchant Boesgaard. (http://www.ifa.hawaii.edu/~boes/) is looking at Li abundance in stars. |
| Nov12-05, 08:59 PM | #26 |
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| Nov12-05, 09:04 PM | #27 |
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| Nov12-05, 09:17 PM | #28 |
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| Nov12-05, 09:36 PM | #29 |
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![]() (slow night) |
| Dec27-05, 05:30 PM | #30 |
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stars are in a state of hydrostatic equallibrium. outward radiative pressure from photons and nuetrinos emitted in he core are balanced by the inward force of gravity.
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| Dec27-05, 07:25 PM | #31 |
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| Dec27-05, 10:13 PM | #32 |
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| Jan12-06, 02:50 PM | #33 |
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While this is technically true, as SpaceTiger pointed out, radiation pressure is insignificant in the case of the sun. I whipped this up in Matlab real quick to demonstrate. The graph is on a log scale, so the [tex]10^#[/tex] you see on the y axis is the same as that part in scientific notation. it had to be log scale for the gas pressure to even be noticeable on the graph. A difference of 10^4 is a factor of 10,000 difference between the two. |
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