Discussion Overview
The discussion revolves around the scale at which the universe can be considered homogeneous and isotropic, specifically in terms of Mega Parsecs (Mpc). Participants explore the boundaries of this principle, its establishment, and the relevance of recent surveys like the Sloan Digital Sky Survey.
Discussion Character
- Exploratory, Technical explanation, Conceptual clarification
Main Points Raised
- Some participants question the specific Mega Parsecs scale at which the universe is considered homogeneous and isotropic, noting that it is not the case on smaller scales.
- One participant references a diagram from Ned Wright's site, suggesting a gradual transition to homogeneity as the scale increases.
- Another participant estimates that the relevant scale is roughly 80 Mpc.
- A later reply expresses gratitude for the information, indicating its usefulness for a recent cosmology exam.
Areas of Agreement / Disagreement
Participants generally agree that the universe is not homogeneous or isotropic on small scales, but there is no consensus on the exact Mega Parsecs scale or the historical context of its establishment.
Contextual Notes
The discussion does not clarify the assumptions behind the estimates or the specific definitions of homogeneity and isotropy being used, nor does it resolve the historical timeline of when these estimates were established.