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Can somebody please explain Olbers' paradox to me? |
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| Jan16-11, 05:53 PM | #1 |
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Can somebody please explain Olbers' paradox to me?
In general terms, but not too general.
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| Jan16-11, 06:10 PM | #2 |
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If the universe were of infinite age and size, every line of sight would end on the surface of a star and it would be very bright:
http://en.wikipedia.org/wiki/Olbers'_paradox |
| Jan17-11, 07:25 AM | #3 |
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It goes further. Imagine for a minute a large box with perfectly reflective interior walls. Make the box large enough to contain stars, planets, and interstellar gas. Since there is no way for heat or light to escape, the contents of the box will heat up, eventually reaching and surpassing the (original) temperature in the interior of the stars.
A long-lived universe that does not expand is equivalent to a set of such boxes, or if you prefer, to just one. In either case, Earth, and humans could not survive in such a universe. In effect, Olber's paradox says we must live in an expanding universe, since we could not exist in a static or shrinking universe, unless it was extremely young. And very young universes have other problems. |
| Jan17-11, 09:45 AM | #4 |
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Can somebody please explain Olbers' paradox to me?Olber's paradox also doesn't address the issue of the age of the stars which is not infinite despite the infinite age of the universe. At some point all the hydrogen in a region would be depleted and no new stars could form. In fact if the universe were infinitely old, would that not mean that there could be no shining stars at all - a truly dark sky. |
| Jan17-11, 11:51 AM | #5 |
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Neither would all the light reach us since the expansion rate would outrun the light's ability to traverse it.
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| Jan17-11, 12:36 PM | #6 |
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I don't think Olber's paradox considers an expanding universe. The universe is considered to be infinitely large and infinitely old. There would be nowhere to expand.
"Eternity is a long time, especially towards the end." - Woody Allen |
| Jan17-11, 01:06 PM | #7 |
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So the probability of not hitting a star in the first D light years could be (1-p). Not hitting a star in a distance of 2D would have probability (1-p)2. Not hitting a star ever would have probability [tex]\lim_{n\to\infty}(1-p)^{n} = 0 \ \forall p>0[/tex] This assumes the universe has some regular structure for a big enough scale of distance. There are big fluctuations in density over even the scale of light years, because of galaxies compared to intergalactic space, but if there is ever a scale over which the distribution of stars is well approximated as homogeneous and isotropic, then this logic would hold. Of course, there are some assumptions in this argument. If the stars preferentially aligned themselves behind one another from the earth's perspective, this would not work. But that would make the earth a very special place in the universe. The universe could be infinite, but with the density of stars diminishing towards 0 quickly as you head outward. This is why you need the assumption of homogeneity. |
| Jan17-11, 04:36 PM | #8 |
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LeonhardEuler,
I concede your point, however I don't believe your example is quite correct, though, even when corrected, it doesn't change the result. It still doesn't address the problem of in a universe of infinite age, all the hydrogen and other fusionable elements would have long disappeared. |
| Jan17-11, 04:55 PM | #9 |
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In any case, you're still not thinking about it properly. This is isn't like a lottery where once a number (printed on a ball) is used, it can't be used again. Any individual vector has the same finite odds of hitting a star by a particular distance and the fact that some vectors hit more than one star (and some certainly will!) doesn't change that. No one is suggesting that each vector would hit only one star! |
| Jan17-11, 08:46 PM | #10 |
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| Jan17-11, 08:57 PM | #11 |
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The idea of Olber's paradox is that if a ray ends on the surface of a star, then what you see coming from that direction is the surface of a star. So if every ray terminates on the surface of a star, then everywhere you look in the sky should seem like the surface of a star.
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| Jan17-11, 09:33 PM | #12 |
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That point is no longer in dispute, just that if the universe were infinitely old, the surface of those stars would certainly be dark.
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| Jan18-11, 01:50 AM | #13 |
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I agree with russ, the universe cannot be both spatially and temporally infinite. Expansion does not resolve this paradox. The photons from distant stars would still have an infinite amount of time to reach us.
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| Jan18-11, 04:46 PM | #14 |
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When considering Olber, it helps to remember that you are not at the center of the universe.
If there is a decreasing density the further you move from your origin, Olber's seems silly, if there is roughly the same density (thus that term "homogenous" being used) every which way you go, then you will not be able to look any direction without seeing a photon. |
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