What is the general relationship between a galaxy's distance from earth and its speed?
Hubble law explains the recessional velocity and distance.
The current value of the Hubble constant is 73 kilometres per second or megaparsecs. Put another way, the further away a galaxy is, the faster its recessional speed is. V= Ho x D where V= recessional ve; velocity Ho=Hubble constant
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Hubble's law, which is expressed as v = H0 * d, where v is the velocity, d is the distance, and H0 is the Hubble constant, describes the general relationship between a galaxy's speed and its distance from Earth. It states that the velocity at which a galaxy is moving away from us is directly proportional to its distance from Earth.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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