Cosmological redshift refers to the phenomenon where light from distant galaxies shifts to longer wavelengths, appearing "redder" as those galaxies move away from us, a concept rooted in the Doppler effect. This shift is significant in the context of an expanding universe, as demonstrated by Hubble's observations linking distance and redshift. General relativity explains that light traveling through gravitational fields can also experience redshift, known as gravitational redshift, but this is distinct from cosmological redshift. The relationship between redshift and galaxy distance supports the idea that space itself is expanding, a key tenet of modern cosmology. Understanding these shifts is crucial for interpreting astronomical observations and the dynamics of the universe.