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Whether itβs more troubling to imagine that the Universe goes on forever in every direction, or that it has an edge, beyond which there is nothing, is hard to say.
Astrophysics doesnβt provide any guidance as to which flavour of existential crisis we should be having β while we canβt say with any level of confidence whether the Universe goes on forever or not, we can say that our observable universe has an edge, in the sense that thereβs a distance beyond which, whatever may or may not exist, we absolutely cannot see it.
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Olbersβ ParadoxΒ asks: if the Universe is infinite, and if there are stars (or galaxies) throughout it, why is the sky dark? Surely, if we look in any direction in the sky, that sightline will, eventually, land on a star. Common sense, therefore, tells us that everywhere we look, the sky should be as bright as the Sun, constantly aglow.
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The standard resolution to this paradox invokes the finite age of the cosmos and the speed ofΒ light. Even if the cosmos is endless and full of stars, one might reason, we can only see the ones that are close enough for there to have been enough time (since the beginning of the Universe) for the light to reach us from there. Anything distant enough from the Earth that the light travel time is more than the age of the Universe is invisible to us.
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The stranger physics comes in when you ask, what are those things whose light has travelled for that long? TheΒ Big BangΒ theory says that the Universe 13.8 billion years ago was a hot, dense inferno, in which all of space was filled with glowing-hot plasma, rippling and churning like the surface of the Sun. Because all of space was glowing, when we look into the farthest reaches of the cosmos in any direction, that glow is in fact what we see.ο»Ώ
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The reason the Universe can be glowing all around us but still look dark comes down to the physics of light in an expanding universe. When space expands, and the distance between objects grows, the light passing between those things gets stretched out, shifting the light to lower frequencies on the electromagnetic spectrum.
For visible light, lower frequencies correspond to redder colours, so this effect is called βredshiftβ. You can think of it like a Doppler shift β the same kind of effect thatβs responsible for a siren dropping to a lower tone when an ambulance speeds away from you
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While we may never know if the Universe as a whole is infinite or bounded, we know that theΒ cosmic microwave backgroundΒ β the distant shell of fading fire that surrounds us β is the most distant light we can ever see, at the edge of our observable universe. But just like the darkness of the night sky, this edge is a matter of perspective. Someone living in a galaxy billions of light years away from us sits at the centre of their own observable universe, which may only partly overlap our own.
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