what’s the shape, or “curvature,” of the Universe? our Universe is special— it has a v specific amount of energy allowing it to expand FOREVER as a FLAT Universe. to picture this, imagine shining 2 lasers into space. here, they’ll continue in parallel, never meeting or diverging.
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our Universe didn’t have to be this way. it could’ve had a large enough energy density that space itself would collapse in on itself in the Big Crunch. if you shone lasers in this Universe, the light rays would meet before meeting back where they started—just like a sphere.
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our Universe could’ve been negatively curved if it had a low enough energy density. this open Universe would look like a 4-D saddle, expanding forever.
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in more technical terms, astronomers measure a value called the density Ω. if Ω>1, we’d live in a spherical geometry. if Ω<1, we’d live in a negatively curved, hyperbolic geometry. if Ω=1 (and it VERY nearly does!!), we’d live in a flat universe. And we do. This is home.
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let’s think about this more intuitively. imagine a triangle drawn in space by 3 light beams. if the angles add up to 180deg, we live in a flat Universe. if they’re less than 180deg, space is negatively curved, & if they’re more than 180deg, it’s positively curved.
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so how do astronomers measure the density of the Universe? one way is to use the cosmic microwave background (radiation leftover from the early Universe) temperature variation across space. in flat space, light from hot spots travels along straight lines—and that’s what we see!!
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