This question came to my mind when I read on NASA's website that an explosion (gamma ray burst, GRB 080913) took place 12.8 billion light years away from us. How do they measure such large distances?
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Possible duplicates: http://physics.stackexchange.com/q/24927/2451 and links therein. – Qmechanic Jul 18 '14 at 18:57
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possible duplicate of How do you measure distance to stars within the galaxy? – John Alexiou Jul 18 '14 at 20:37
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Voting to leave open: certainly not a duplicate of "distances to stars within the galaxy" as the techniques required for this much larger distance are completely different. As to the other possible dup, this measurement uses a technique not mentioned in the answers to that other more general question. Will edit this question a bit to make the distinction more clear. – Kyle Oman Jul 18 '14 at 22:01
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possible duplicate of How is the distance to a $\gamma \mathrm{-ray}$ burst (GRB) measured in just a few days? – Jul 18 '14 at 22:41
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@Kyle but what about the one I linked? Also, if the OP didn't just want GRB's, there's http://physics.stackexchange.com/questions/70400/how-do-we-know-that-these-radio-bursts-are-from-billions-of-light-years-away for radio. – Jul 18 '14 at 22:42
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@ChrisWhite both questions happen to ask about different GRB whose distances were estimated using different techniques (I think the one from this question was from the end of the Ly-$\alpha$ forest, the other one is emission lines from the galaxy). Since they ask about specific objects (though not by name), I'm still leaning not dupe, but your link is certainly arguable. – Kyle Oman Jul 18 '14 at 22:46
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@Kyle then retracted, but perhaps the question should give some hint that photo-z's were involved? Maybe with some quote from the article? – Jul 18 '14 at 22:49
2 Answers
Did you mean 12.8 billion light years away?
If so, in this case the distance was estimated by measuring a rough spectrum for the GRB. The NASA article I've linked says:
In certain colors, the brightness of a distant object shows a characteristic drop caused by intervening gas clouds. The farther away the object is, the longer the wavelength where this fade-out begins.
This technique is used where it's hard to get a detailed spectrum and calculate the red shift.
If you're asking a more general question then this is covered in the question How is distance measured to far away stars and galaxies? and your question would be a duplicate.
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@JohnRennie: yes sir i meant 12.8 billion light years. sorry for omitting billion there. – syed_ali_mousvi Jul 18 '14 at 18:00
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I think that characteristic drop would be the beginning of the "Lyman-$\alpha$ forest". So really this is a lower limit on the distance (which, at 12.8 Gly, still tells you it's pretty darn far away). – Kyle Oman Jul 18 '14 at 18:24
For relatively close objects, the distance can be measured through measurements of parallax (http://en.wikipedia.org/wiki/Parallax ).
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1Note this was a reasonable answer to the question as stated at the time of the answer (I almost downvoted until I noticed). – Kyle Oman Jul 18 '14 at 22:13