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01-01-2002, 11:40 AM | #51 | ||
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Just some nitpicking.
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01-01-2002, 03:04 PM | #52 |
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oh... i know why david is confused and i really didn't answer the question.. when the sun 'burns' it's fuel, it is fusion of hydrogen into helium. the actual mass fraction lost to energy by the conversion of hydrogen to helium is very small (not fast enough to noticeably change the radius of the sun) and remember that the byproducts remain in the sun as helium and possibly other elements. david, a little advice, learn about a subject that you are going make thses type of comments about.
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01-01-2002, 03:21 PM | #53 |
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Whooee, it can get boring on a holiday afternoon! I was forced to figure this one out. The Sun converts 4.2 million metric tons of matter into energy each second. (It processes 140 times this mass of hydrogen into helium to do this.) That's a lot of mass going away - equivalent in weight to a billion gallons of water per second. Also, however, it is only a 0.0000000001% decrease in the mass of the Sun per century. Like Opticsguy said: you won't see it.
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01-02-2002, 06:54 PM | #54 |
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From a non scientific newbie...
Regarding earlier post... Wouldn't death be an evolutionary advantadge in that species that die allow younger and stronger examples of thier biological species to fill a certain niche and therefore pass on more DNA??? Just curious Bubba |
01-02-2002, 07:47 PM | #55 |
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Not exactly. I assume that by "death" you mean "death due to aging", since death itself doesn't really require an evolutionary explanation. The problem with your explanation is that it doesn't explain why being younger should mean being stronger - why not simply be healthy and vigorous until death due to external causes? The explanation seems to be that eventually everything is going to die of an external cause, and that any genes that have deleterious effects or interactions which take place aftera certain age will be less selected against or not selected against at all. Look at salmon - they have essentially no chance of spawning again so they essentially fall apart (catastrophic senescence) after spawning.
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01-02-2002, 09:52 PM | #56 | |
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Thanx heaps, Grady |
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01-03-2002, 10:32 AM | #57 |
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Grady - It's pretty simple, really, and I actually found results like mine here" target="_blank">http://www.seds.org/billa/tnp/sol.html]here[/URL]</a> a couple of minutes ago.
Start with the energy output of the sun, 3.83 x 10^33 ergs per second, from the link above or an astronomy text. Then remember what ol' Al Einstein said: E equals emcee squared, or E=mc^2. The appropriare value for c, the speed of light, is 3 x 10^10 centimeters per second. So now we have 3.83 x 10^33 = (3 x 10^10)^2 x m , so m, the mass converted to energy per second, is 4.26 x 10^12 grams/second. That converts to 4,250,000 metric tons. The "140 times this much hydrogen" is from the fact that four hydrogen atoms weigh 0.029 atomic mass units more than one helium atom - this lost mass is about 1/140th of the 4 amu the hydrogen weighed. The loss per century is arrived at by multiplying the loss per second out to 100 years' worth and dividing by the mass of the sun. Another fun way to express some of this is that the water equivalent of the mass-per-second is also 3450 acre-feet of water, or a 100-acre lake 34.5 feet deep. And you can put this all in perspective, sort of, if you consider that the Hiroshima A-bomb converted about one gram of matter into energy. |
01-03-2002, 03:39 PM | #58 | |
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01-03-2002, 03:46 PM | #59 | |
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01-03-2002, 06:20 PM | #60 |
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Well, they can be expressed all along, as long as the debilitating effects only become significant later.
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