ugalpha said:
So i read the answer of Marcus in the thread "Where is the Center of the Universe" where there was a brief mention of the "Un-Copernican" view of the Cosmos. Now i do not think that we are at the center of the Universe but this got me thinking.
"IF" the homogeneity of the Cosmos really was only the consequence of us being in the center of the Universe, How far away from our planet would we have to observe the universe to start seeing the heterogeneity of the Cosmos?
10,100,1000 billion miles?
I'd be happy to hears how some other people would reply to that. I think it would depend on how ABRUPT you imagine the inhomogeneity to be.
We see a fairly homogenous U out to a presentday radius of about 45 Gly.
At that distance (45 billion ly) we see the emission of the ancient light from nearly uniform density glowing hot hydrogen gas. The unevenness in density of the gas is about 1/1000 of one percent.
Suppose we lived in the center of a 46 Gly radius bubble and outside that there was a much denser layer. This idea has been explored by cosmologist David W. as a way to explain the very gradual acceleration of expansion. Could it be the "pull" of a denser surroundings that we cannot see?
Then the U that we can see would be, in effect, a comparatively low density "void".
Well depending on how abrupt the transition was we would probably not be able to tell. People in a galaxy 1 Gly to the east of us would be closer to the denser shell and would be able to see it as an anomalous spot in their CMB sky.
Any spot that is not due to our own motion doppler and which is substantially hotter/colder than the normal temperature fluctuations which are 1/1000 of one percent, would be a giveaway that there is some inhomogeneity.
But the conditions imagined in order to "fool us" are finetuned and far-fetched. It is like fairies having put fake dinosaur fossils in the rocks so as to make us believe dinosaurs.
We are contriving an inhomogeneity and then contriving to put Earth right in the center of a void so that we do not see it.
