sqljunkey
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How can someone tell the difference between a super massive galaxy's redshift and a galaxy that is accelerating away?
The discussion revolves around distinguishing between the redshifts of supermassive galaxies and those of galaxies that are accelerating away from the observer. It explores concepts related to gravitational and cosmological redshift, as well as the implications of distance and intrinsic gravity.
Participants express differing views on the terminology and concepts involved, indicating that there is no consensus on how to interpret the differences in redshift between the two types of galaxies.
There are limitations in the discussion regarding the definitions of terms like "super massive galaxy" and the assumptions about gravitational versus cosmological redshift. The implications of distance and intrinsic gravity are also not fully resolved.
If you detect light you have one parameter: the measured wavelength. Any "redshift" is inferred from other factors, such as that you are observing a shifted hydrogen spectrum. There is, therefore, nothing inherent in the measured wavelength that tells you anything other than the measured wavelength.sqljunkey said:How can someone tell the difference between a super massive galaxy's redshift and a galaxy that is accelerating away?