What does the large-scale structure of the universe look like?
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The large-scale structure of the universe consists of galaxy clusters, filaments, and voids, which are interconnected by a cosmic web-like structure. This arrangement forms a foam-like pattern, where galaxies are clustered along filaments and around massive galaxy clusters, with vast empty regions known as voids in between.
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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 fast was the universe expanding during the first second of the big bang?
- How does gravity affect the expansion of the universe?
- How do we know the universe is expanding faster?
- On the 1 to 10 billion scale, about how far is it to the nearest stars besides the Sun?
- Is space expanding within superclusters of galaxies?
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