How big do we need for comsological principle?

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When we say the universe is homogenous and isotropic . How many Mega PArsecs are we talking about? Preusmably we all agree its not homogenous or isotropic on small scales. So where is the border and how when was it established? Is the current estimate, whatever it is, as recent as Sloan Digital Sky survey or much older than that?
 
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How many Mega PArsecs are we talking about?
There's a diagram on Ned Wright's site. It's a gradual transition - the larger the scale, the more homogeneous.
 
skydivephil said:
When we say the universe is homogenous and isotropic . How many Mega PArsecs are we talking about? Preusmably we all agree its not homogenous or isotropic on small scales. So where is the border and how when was it established? Is the current estimate, whatever it is, as recent as Sloan Digital Sky survey or much older than that?
Roughly 80Mpc or so.
 
Agh thanks for that, wanted it for my cosmology exams which was yesterday ,think I aced it and you guys have been enormous help in general, Physics forums rock
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
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