What proportionality did Hubble establish in 1929 concerning a galaxy's recessional velocity and its distance from Earth?
Answer
The recessional velocity of a galaxy was directly proportional to its distance from Earth.
The breakthrough observation published by Hubble in 1929 was not merely that galaxies were moving away, but the systematic manner in which they were receding. He demonstrated a direct proportionality: the farther away a galaxy is located from our position, the faster it is observed to be moving away from us. This relationship implies a large-scale, systematic motion affecting all observed galaxies. This finding crystallized into Hubble's Law, forming the observational backbone for understanding the large-scale structure and dynamics of the cosmos.

Related Questions
What did Edwin Hubble prove about the "spiral nebulae" observed across the night sky in the 1920s?Which specific standard candles did Hubble utilize to accurately calculate the distances to remote nebulae like the Andromeda Nebula?What proportionality did Hubble establish in 1929 concerning a galaxy's recessional velocity and its distance from Earth?What physical phenomenon causes the light from distant galaxies to be shifted toward the red end of the spectrum during spectroscopic analysis?What is the mathematical expression used to represent the proportionality described by Hubble's Law?What crucial insight did Hubble's data provide regarding the nature of the cosmic expansion, as opposed to a simple explosion scenario?According to the implications of Hubble's findings, what geometric property describes the expansion as being the same in all directions and everywhere in space?Whose theoretical work, rooted in Einstein’s General Relativity, proposed a model for an expanding universe that Hubble's observational data later substantiated?After Hubble confirmed that spiral nebulae were external galaxies, how drastically did the perceived size of the known universe change?What task, undertaken alongside Milton Humason, was required after establishing galaxy distances to determine their movement?