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Like sound, light waves moving away from the observer are stretched making the wavelength longer and when light comes toward us it appears to become compressed.

Since the bottom end of the spectrum is red and the top blue, an object which radiates light appears to be red shifted when it moves away from us as the light wave is stretched. It has been observed that all stars are red shifted, therefore the conclusion is that all stars are moving away from us in space.

This effect is called Doppler shift and is the reason a car engines note sounds higher as the car approaches and lower as it moves away from the listener.

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Each star shines with its own light, and every star is different. But there are certain things that are constant, such as the spectrum lines for elements like hydrogen, helium, carbon and oxygen, and other heavier elements.

There is a phenomenon called the "Doppler efflect", named by Christian Doppler, an Austrian mathematician and physicist. (See the link below.) In the 1920's, spectral analysis of the light of distant galaxies revealed that the light spectra was shifted, and that the Doppler effect allowed astronomers to calculate the speed at which those galaxies were moving toward or away from us. With few exceptions, those galaxies are moving away, and the further away they are, the higher their velocities are.

Edwin Hubble suggested that the uniform motion away from Earth might suggest that rather than the Earth being unique in having a galactic case of terrible body odor, the universe was expanding. This took the uniqueness away from Earth or the Milky Way galaxy; hypothetical observers in ANY galaxy would perceive that everything was moving away from THEM as well. (An interesting sidenote; the Andromeda galaxy is actually getting CLOSER to the Milky Way, and will probably collide with us in about 3 billion years. Fasten your seat belts! )

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Q: How do you determine how quickly a distant galaxy is moving away from the earth?
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When a star or galaxy moves quickly away it is called what?

We can measure fairly accurately the radial speed of a star or galaxy by measuring the Doppler shift of the emitted light from the star. Stars emit specific frequencies of light, and we can measure the frequencies to determine what elements are contained within the star. But since we know exactly what the frequencies are, we can measure the precise frequencies that we measure from the star. A star moving toward us will have its light "blue-shifted", or compressed a tiny bit in frequency. The amount of the compression tells us the radial velocity. A star whose light is red-shifted is moving away from us. Radial velocity is the part of the velocity that is directly toward or away from us; Doppler shifts don't tell us anything about a star's side-to-side motion. One of the astonishing discoveries of Edwin Hubble is that most galaxies are moving away from us, and the farther away they are, the faster they seem to be receding. Some nearby galaxies are moving closer, but the more distant the galaxy, the faster it is moving moving away. He determined this by the "red shift" of the light from distant galaxies.


What galaxy did hubble discover?

-- Once you get past our "local group", every galaxy is moving away from us. -- The farther any galaxy is from us, the faster it's moving away from us.


Why are the blueshift and redshift useful in the study of the universe?

Redshift and blueshift are manifestations of the Doppler effect. This lets us determine whether a star, or a galaxy, is moving towards us, or away from us.


How do you use spectral lines to determine if a galaxy is moving towards earth or away from earth?

The spectral lines move towards one direction, or towards the other direction, depending on the relative speed.


Spectrographs help astronomers determine a star's what?

The star's chemical composition; the star's rotation; pulsations of the star; planets or other invisible objects moving around the star; how quickly the star is moving towards us or away from us.

Related questions

How does light from distant galaxy . galaxy out side of 32000000 light years support the big bang theory?

The light from distant galaxies is redshifted. The only reasonable explanation for that is that the galaxies are moving away from us.


How does imaging determine how fast a distant galaxy is moving away from Earth.?

The star's spectrum is analyzed; certain lines in the spectrum, which have a fixed position, will change their position when the object moves away from us or towards us.


What is the pattern between how far away galaxies are and how quickly they are moving?

The farther a galaxy, the faster it moves away from us.


How the spectrum shift of the dark line supports theory that universe began from a very small point?

1.the observed wavelength of the dark line from the distant galaxy has increased 2.therefore the distant galaxy must be moving away from the Earth suggesting the Universe is 3.expanding outwards from a small initial point


When a star or galaxy moves quickly away it is called what?

We can measure fairly accurately the radial speed of a star or galaxy by measuring the Doppler shift of the emitted light from the star. Stars emit specific frequencies of light, and we can measure the frequencies to determine what elements are contained within the star. But since we know exactly what the frequencies are, we can measure the precise frequencies that we measure from the star. A star moving toward us will have its light "blue-shifted", or compressed a tiny bit in frequency. The amount of the compression tells us the radial velocity. A star whose light is red-shifted is moving away from us. Radial velocity is the part of the velocity that is directly toward or away from us; Doppler shifts don't tell us anything about a star's side-to-side motion. One of the astonishing discoveries of Edwin Hubble is that most galaxies are moving away from us, and the farther away they are, the faster they seem to be receding. Some nearby galaxies are moving closer, but the more distant the galaxy, the faster it is moving moving away. He determined this by the "red shift" of the light from distant galaxies.


How is the cosmological motion of a distant galaxy fundamentally different from the motion of an object speeding through space?

The object - planet, meteoroid, comet, spaceship - is traveling THROUGH space; the galaxy is moving away WITH space. That is, the space itself is expanding.


Which has a higher frequency a star moving away from earth or towards earth?

I would think that current evidence suggests that the stars moving away from earth, some of them in far distant galaxies moving at unimaginably high speeds, are going much faster than stars moving toward us. The entire Andromeda galaxy is moving toward us and will collide with us in roughly 5 billion years, and it is not moving anywhere near as fast as the distant retreating galaxies.


How can the Doppler effect determine if things are moving towards a distant galaxy or away from one?

Light had properties of frequency that related to colour. It is apparently contract in the direction moving toward the observer (higher frequency-short wavelength) and apparently elongated in the direction moving away from observer (lower frequency-high wavelength). What moving toward us is tend to be look more blue than usual (blue shift) and what away from us is redder than usual (red shift).


What if no distant galaxies showed any redshift or blueshift?

It would mean that the universe was radially static. That is, no galaxy was moving towards or away from the earth. This could happen if everything in the whole universe were moving in the same direction at the same [linear or rotational] velocity.


How does the Doppler shift determine the distance of Sirius?

It doesn't. The Doppler shift can tell you how fast something is moving towards us or away from us; not how far it is. Only in the case of distant galaxies can this be used to estimate the galaxy's distance, because of the expansion of the Universe (galaxies that move away from us faster are generally farther away).


Does the colour of a galaxy reflect its distance away from the earth?

No, however, we can determine whether a galaxy is moving towards or away from us, by looking at the shift in its spectrographic analysis. There are "red shifts" and "blue shifts" in spectrographic results. "Blue shifts" indicate that a galaxy is moving towards us, because the wavelength of the light emitted by the galaxy is compressed, causing it to shift to the blue end of the colour spectrum. "Red shifts" indicate that a galaxy is moving away from us, because the wavelength of the light emitted by the galaxy is being stretched towards the red end of the colour spectrum.


How fast is the milky way galaxy moving away from us?

We are part of the milky way galaxy, so we are moving with it.