How can astronomers determine that the universe is expanding?
By measuring the Doppler shift.
Both light and sound waves gets elongated if the source is getting away from us.On the other hand if an object is coming towards us the waves gets compressed.The elongation waves in light is called red shift. In 1920 Edwin Hubble studied spectrum of several Galaxies and found the red shift.He found tht the far away galaxies move fastest.
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The redshift of distant galaxies—which shows that these objects are moving away from us and that their apparent speed increases with distance—is the primary indicator used by astronomers to determine that the universe is expanding. This phenomenon is consistent with the universe expanding uniformly in all directions.
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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.
- If the Hubble Space Telescope proved that Hubble's constant is actually half as large as it is currently believed to be, what would the implied age of the universe be in comparison to the current accepted value?
- What is our nearest star to earth?
- What does gravity mean in flight?
- How strong is the force of gravity on earth?
- What is the diameter of the Celestial Sphere?
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