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  • Black holes are captivating, both in a literal sense and as a topic of discussion.

  • Everything about them is bizarre and extreme and were always discovering something new.

  • But even the most basic facts about black holes are pretty incredible, and it’s possible

  • youve never had a primer on them.

  • So today were going back to basics and talking about what black holes are, how they

  • form, and how they die.

  • So let’s start at square one and define exactly what a black hole is.

  • A black hole is a region in space where the gravitational pull is so strong, anything that

  • enters cannot escape again.

  • That includes the fastest thing in the universe, light, and since light can’t come back out

  • once it crosses that point of no return known as the event horizon, observers like us on

  • the outside can’t see black holes.

  • They are completely invisible.

  • So you may be wondering how we know theyre there.

  • Weve even taken pictures of them, it was in the news and everything.

  • The black hole itself may be invisible, but we can still find them because of the effect

  • they have on nearby matter and on light passing close-but-not-too-close.

  • Weve spotted the radiation given off by superheated matter swirling around them, forming

  • what’s called an accretion disk.

  • It basically looks like space’s version of the Eye of Sauron.

  • We can even see the back side of the accretion disk that would be hidden behind the black

  • hole’s shadow if it weren’t for the wild way black holes can alter the path light takes.

  • According to Einstein’s theory of General Relativity, black holes warp space and time to the extreme

  • because they pack an enormous amount of mass into an incredibly small space at the black

  • hole’s center.

  • Just how much mass the black hole has determines how far away the event horizon is from the

  • center, a distance called the Schwarzschild radius, and the radius can grow if more matter

  • falls into the black hole.

  • The Schwarszchild radius is important in another way: it’s also the minimum size an object

  • will have to be squeezed down to for gravity to take over and turn it into a black hole.

  • Everything has a Schwarzschild radius, you me, the earth, the sun.

  • To make a star with the mass of the sun into a black hole, you would need to compress it

  • down to a sphere with a radius of less than 3 kilometers.

  • If that were to suddenly happen somehow, let’s say via some alien superweapon or something,

  • the earth and all the planets wouldn’t be sucked in and compressed into oblivion.

  • Remember objects have to be within that Schwarzschild radius for a black hole to devour them, and

  • as long as we stayed more than 3 kilometers away from our black hole sun that wouldn’t

  • be our fate.

  • In fact if the sun were to be replaced with a black hole of 1 solar mass, the orbits of

  • the planets in our solar system wouldn’t change at all.

  • The sudden onset of eternal night would be catastrophic though, so we’d still be doomed,

  • just not in the way you might first assume.

  • Ruling out alien superweapons, how do black holes form?

  • Well it depends on what kind of black hole were talking about.

  • Stellar mass black holes with masses between 3 to dozens of times that of our sun dot the

  • galaxies.

  • Most often they form when a star of at least 20 solar masses goes supernova, leaving behind

  • a core that collapses below its Schwarzchild radius under its own weight.

  • Supermassive black holes are anywhere from 100,000 to billions of solar masses and we

  • think theyre found at the center of most large galaxies, if not all of them.

  • The famous photo of a black hole is a supermassive black hole in the galaxy Messier 87.

  • How they form is still a mystery but we think they get their start around when their galaxies

  • are just beginning.

  • Obviously there’s a huge gap in size between stellar mass and supermassive black holes,

  • so scientists have long predicted the existence of intermediate black holes and weve just

  • started to spot our first candidates recently.

  • There’s also the possibility that black holes smaller than stellar masses were created

  • by the early universe.

  • Some speculative theories even suggest black holes could be as tiny as the subatomic scale,

  • and could be smashed into existence

  • from collisions inside particle accelerators.

  • We haven’t seen any evidence of those yet, but if we did, don't fret.

  • Remember again that just because something’s a black hole doesn’t automatically turn

  • it into an unstoppable planet-crushing vacuum cleaner.

  • It would need to get close enough to you for it to be a threat, and because of how black

  • holes die, microscopic black holes will never get the chance to expand to a dangerous size.

  • We think black holes decay by giving off something called Hawking radiation.

  • The oversimplified explanation goes that virtual particles are constantly popping into existence

  • in the vacuum of space and usually they come together and cancel each other out, but if

  • a pair forms straddling an event horizon, one will escape while the other will fall

  • in and the process shrinks the black hole until it is no more.

  • Physicist Stephen Hawking predicted the existence of this radiation and also showed that the

  • smaller a black hole is, the faster its rate of decay.

  • That means a microscopic one made from particle collisions would have an unfathomably short

  • lifespan of around 10 to the -27 seconds.

  • Much too short to balloon to a dangerous size.

  • That’s a bit of a relief, but by the same token, this also means that supermassive black

  • holes will be around for a very long time, many orders of magnitude longer than

  • the current age of the universe.

  • Still it’s not like well come dangerously close to one of those in our lifetimes.

  • So really the only thing about black holes you won’t be able to escape is us talking about

  • them on this channel, and since youve watched this video, youll be up to speed when we

  • do.

  • If you can't wait to learn more, we've got a whole playlist ready for you.

  • Get ithole..

  • You can go get sucked into that.

  • And also let us know if this video gave you some new insight or

  • if your mind was already crammed full of black-hole knowledge, because

  • we'd like to do more back-to-basics explainers.

  • Tell us in the comments, don’t forget to subscribe, and thanks for watching Seeker!

Black holes are captivating, both in a literal sense and as a topic of discussion.

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The Life of a Black Hole

  • 9 1
    Summer 發佈於 2022 年 04 月 20 日
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