Measurement of Galaxy Rotation: How Long Does it Take?

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Galaxy rotation is measured over many years using spectroscopy, which analyzes the redshift of stars in different arms of the galaxy. While individual stars have varying velocities, most stars in a galaxy's arms generally move at similar speeds, which can be quantified. The term "fast" is relative, often compared to the Sun's orbit at approximately 251 km/s. Observations indicate that stars in the arms are moving faster than general relativity predicts, leading to the hypothesis of dark matter's existence. This discrepancy in expected versus observed speeds is a key focus in understanding galaxy dynamics.
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it takes many years to see the change of arms of a galaxy. so how was the rotation of arms measured?
 
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Spectroscopy. You check the red shift of stars in the various arms of a galaxy.
 
but it is said that stars in the arms are moving at fast rate. the arms are nothing but collection of stars. so, how can arms have a different speed and if so, how can it be measured?
 
jayaramas said:
but it is said that stars in the arms are moving at fast rate.

Define fast. Compared to what? The Sun orbits the galaxy at about 251 km/s.

the arms are nothing but collection of stars. so, how can arms have a different speed and if so, how can it be measured?

While each individual star will have it's own specific velocity at any point in time, in general most stars will have roughly the same velocity as they move around the galaxy. This is measurable through spectroscopy like Chronos said.
 
jayaramas said:
but it is said that stars in the arms are moving at fast rate.
They are indeed going faster than general relativity predicts, hence the assumption that there is hidden (dark) matter.
 
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