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Originally posted by nightbringr
Originally posted by CLPrime
reply to post by nightbringr
That's essentially right, except it is the radius of the universe that we view expanding from the apparent center, not half the radius. We view 13.7 billion light-years expanding in every direction.
No. If the radius is 15 billion light years, and we are in the middle looking towards the "edge", we only are viewing half of the 15 billions, thus 7.5 billion.
Originally posted by CLPrime
It's also misleading to say "edge" or "center". Galaxies at what we see as the "edge" see exactly the same sort of stuff that we see, and, to them, we appear to be at the edge while they appear to be at the center. It's all a matter of perspective.
Perhaps you can explain this more? This would only work in the "wrap around universe" theory. Since we are discussion the "expansion" theory, this is i believe incorrect. The would be a distinct "edge". After all, the galaxy closest to the edge would see nothing looking towards the edge, however would view 15 billions light years of universe looking towards the center.
Originally posted by fenceSitter
I was trying to figure out exactly what the km/s/megaParsec speed meant. I guess it is related to Hubble's Law which states that the further an object is away from us, the faster it goes.
So according to this new measurement, anything 3 million light years away is travelling at 74.3 km/s (+/-). That would mean something 10 times farther away is travelling 10 time faster - 743 km/s. If the estimated size of the observable universe is around 93 billion light years, the universe's farthest edge (from the 'center') would be 46.5 billion light years. That would mean the edge is travelling 15,500 x 74.3 km/s = 1,151,650 km/s!
If my math is right - that is hard speed to fathom. Thanks OP - I learned something today
The second statement might be true though you really need to go further out, the first almost certainly isn't though your calculation would fall on the line of Hubble's law. The problem with your first statement is that distance is within our galactic cluster, where the galaxies are moving toward rather than away from each other. For example Andromeda is 2 million light years away and it's moving toward us rather than away from us.
Originally posted by fenceSitter
So according to this new measurement, anything 3 million light years away is travelling at 74.3 km/s (+/-). That would mean something 10 times farther away is travelling 10 time faster - 743 km/s.
a galaxy at 1 million parsecs will not be observed to recede from us (unless possibly it is located in a direction from us opposite the direction to Andromeda), because the diameter of the Local Group of galaxies is about 3 million parsecs, and within the Local Group, galaxies are not observed to recede.
It's interesting that not all of the uncertainties overlap, but there are no huge disagreements.
A recent 2011 estimate of the Hubble constant, which used a new infrared camera on the Hubble Space Telescope (HST) to measure the distance and redshift for a collection of astronomical objects, gives a value of H0 = 73.8 ± 2.4 (km/s)/Mpc.[9][10] An alternate approach using data from galactic clusters gave a value of H0 = 67.0 ± 3.2 (km/s)/Mpc.[11][12]
As of 3rd Oct 2012 the Hubble constant, as measured by NASA's Spitzer Telescope and reported in Science Daily, is 74.3 ± 2.1 (km/s)/Mpc
An observational determination of the Hubble constant obtained in 2010 based on measurements of gravitational lensing by using the HST yielded a value of H0 = 72.6 ± 3.1 (km/s)/Mpc.[13] WMAP seven-year results, also from 2010, gave an estimate of H0 = 71.0 ± 2.5 (km/s)/Mpc based on WMAP data alone, and an estimate of H0 = 70.4 +1.3
−1.4 (km/s)/Mpc based on WMAP data with Gaussian priors based on earlier estimates from other studies.[14] In 2009 also using the Hubble Space Telescope the measure was 74.2 ± 3.6 (km/s)/Mpc.[15] The results agree closely with an earlier measurement, based on observations by the HST of Cepheid variable stars, of H0 = 72 ± 8 km/s/Mpc obtained in 2001.
I just finished re-watching a video course in cosmology, so the fact that I watched it once before, and the 2nd time was just within the last few weeks makes this stuff pretty fresh in my head. The TTC site is down right now, but here's a spam-type link (I have no affiliation with this "download provider" scam, and don't recommend it) so disregard any download links, but you can see a description of the course:
Originally posted by watchitburn
reply to post by Arbitrageur
Do you just know all this stuff, or do you have to go dig it up?
01 From Dawn To Dusk
02 Exploring The Night Sky
03 Recent Discoveries in Our Solar System
04 Other Worlds Galore
05 The Formation and Evolution of Stars
06 Supernovae - Catastrophic Stellar Explosions
07 Gamma Ray Bursts and the Birth of Black Holes
08 Observational Evidence For Black Holes
09 Einstein's Relativity
10 Cosmology And Cosmic Expansion
11 The Birth And Evolution Of Galaxies
12 The Accelerating Expansion of the Universe
13 The Stuff of the Cosmos
14 Energy-May The Force Be With You
15 Theories of Everything and Hidden Dimensions
16 Our Universe One Of Many