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 focuses on distinguishing between gravitational redshift from supermassive black holes and cosmological redshift in galaxies. Gravitational redshift varies across a galaxy, particularly influenced by the black hole at its core, while cosmological redshift remains uniform throughout. Observers can only infer redshift from measured wavelengths and other factors, such as the hydrogen spectrum. The intrinsic gravity of a galaxy, combined with its distance from Earth, plays a crucial role in interpreting redshift data.
PREREQUISITESAstronomers, astrophysicists, and students studying cosmology and galaxy dynamics will benefit from this discussion.
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?