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If the information we see in space is very old, and the universe "seems" to be expanding, how can we know that it is still expanding?
The discussion centers on the implications of observing ancient light from space and its relation to the universe's expansion. Participants emphasize that while the universe's expansion is inferred from the Hubble constant, which has shown consistent scaling over time, there is no definitive proof that this expansion has not halted at some point in the recent past. The analogy of gravity is used to illustrate the uncertainty in predicting cosmic behavior, yet the consensus is that the long-term trend of expansion is unlikely to reverse suddenly.
PREREQUISITESAstronomers, astrophysicists, and students of cosmology who are interested in the dynamics of the universe and the implications of observational data on cosmic theories.