How do astronomers know the size of the universe?
They don't actually. What they have now as its age is an educated guess but they admit they could be way off.
Astronomers speculate the size of the universe to be 47 billion light years. One way the do this is by approximating the distance of the cosmic microwave background (the "sound" the big bang made).
This is very problematic because they have fairly well nailed down the age of the universe at 13.7 billion years. If you accept that nothing can go faster than the speed of light, as is considered axiomatical, then that should also be the size of the universe if the most distant objects moved out from the big bang at the speed of light.
The fly in the ointment is that in the fist few billionths of a second the universe was in its "expansion" phase. During the initial expansion it became half the size it is today. That means energy moved at speeds well in excess of the speed of light.
Then the expansion slowed way down and objects were created out of energy. As astronomers have studied thousand of galaxies they have found one constant, every galaxy appears to be moving away from every other galaxy and the rate of separation is accelerating. They are at a loss to explain this phenomena.
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Astronomers use various methods to estimate the size of the universe, including measuring the observable universe's radius, using the cosmic microwave background radiation, and studying the distribution and movement of galaxies. These methods provide estimates of the universe's size, but since the universe may extend beyond the observable universe, its exact size remains uncertain.
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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.
- How did the Big Bang begin?
- What is Hubble's Law? What is it used for?
- What is it expanding into? Will it ever stop? Will we ever be able to go outside the zone it is expanding into?
- How many parsecs are in an AU?
- Does the Hubble Law imply that the universe is expanding uniformly from Earth or somewhere near it?
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