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The Universe is observed to be expanding, with galaxies moving away from each other.
Description
Expansion of the Universe
The distance to a galaxy can be calculated using the equation d = v/H₀, where 'd' is the distance, 'v' is the velocity of the galaxy, and 'H₀' is the Hubble constant.
- a[1]
State the significance of the equation d = v/H₀ in cosmology.
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