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The Shape of Spacetime. |
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| Jun26-12, 11:50 AM | #137 |
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The Shape of Spacetime. |
| Jun26-12, 12:27 PM | #138 |
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Did you read the problem of the ants on a rubber rope <http://en.wikipedia.org/wiki/Ant_on_a_rubber_rope> |
| Jun26-12, 02:07 PM | #139 |
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What you are not understanding is that nothing is traveling FTL in the same reference frame. The universe is expanding. The recession rate has nothing to do with c. |
| Jun26-12, 02:43 PM | #140 |
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| Jun26-12, 03:02 PM | #141 |
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I know that v=H*D. If the Hubble constant was constant, this would lead to an exponential recession.
I understood how H is determined (through the variations of redshifts as fonction of distance). I also see how distances can be determined. But I dont know how recession velocities are measured? do you knwo? |
| Jun26-12, 03:03 PM | #142 |
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There are no galaxies residing beyond the surface of last scattering whose photons have not yet reached us. Nothing but hot plasma exists beyond z~1100 [source of the cmb].
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| Jul2-12, 11:31 AM | #143 |
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Recession velocities are measured via redshift. Research the Doppler Effect to understand why Redshift comes about. We can determine which spectral emission lines we can expect to see in stars of certain materials (I can't remember how,) and see how redshifted the stars are. Plug into our easily derivable formula for the relativistic doppler effect, and we're done.
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