Name: What If You Fall into a Black Hole?
Uploaded: 2022-03-22T13:35:01.000Z
Duration: 12 min 15 s
Description: VoiceTubeの動画で発音を聞きながら英語表現を覚えよう！学べる英語：

Black holes are the most powerful and extreme things in the universe and they are wildly

weird and complicated. What would happen if you fell inside one and what are they really?

First we need to talk about space and time: Space and time are the grand stage where the

play of the universe unfolds. But space isn’t a fixed stage and time doesn’t tick the

same for everyone everywhere. In short, they are relative. Matter bends space and bent

space tells matter how to move. Put some stars and planets on the stage, and it sags underneath

them. That misshapen stage, with all its little warps and dips, gives us gravity. Black holes

do not just bend the stage, they are like trap doors. Places with so much mass that

the universe formed a ‘no-go’ zone where the rules change.

Most black holes form when very massive stars die. We explained this process in detail in

our neutron star video – all you need to know, that in the final moments of really

massive stars, their insides implode, at nearly a quarter of the speed of light. This packs

so much mass, so close together that it creates something so dense that it sort of breaks

the stage of the universe. A black hole with ten times the mass of the sun would be barely

If you look directly at a black hole it looks like... nothing. The space under their control

is blocked by an invisible, one-way border called the event horizon. The event horizon

forms a shell around a region of space that, once entered, is shielded from the rest of

the universe forever. Because the black hole trap door deforms space so much, not even

light can escape it. And with nothing escaping to transfer information from the inside, it’s

impossible to tell what it really looks like.

We still can observe black holes because of their effect on matter. Things can orbit black

holes just as they can orbit the sun or a planet. Many black holes have discs of matter

orbiting outside the event horizon. This matter can become incredibly hot as close orbits

can speed this matter up to half the speed of light, and tiny amounts of friction and

collisions between particles heat them to a billion degrees, making the space around

these black holes, ironically, incredibly bright.

What would happen if you would try to get close, or even inside a black hole? First

of all, you would see the strangest funhouse mirror in the universe. Matter isn’t the

only thing orbiting a black hole: gravity is so strong near them that light can orbit

too. If you hovered just outside the event horizon, at the photon sphere, in any direction

you’d just see… yourself! Straight ahead would be the back of your own head, as light

from your back travels around the black hole to your eyes. Gravity also alters the passage

of time itself. The stronger the gravity, the slower time passes. While you watch the

universe above you speed up, those far away will watch you in slow motion. If you chose

to fly away from the black hole, you might find that eons have passed for the rest of

the universe, a freakish one-way time-travel trip to the future where your loved ones are

But getting close to a black hole can be incredibly dangerous. A painful death by ‘spaghettification’

awaits you. Because your feet are closer to the black hole than your head they feel a

stronger pull of gravity, enough to pull you apart. As you descend it gets worse, the pulling

gets stronger, your body squeezed thinner and straighter until you’ve been reduced

to a thin stream of hot plasma, gobbled up in one final slurp, never to be seen again.

Spaghettification is only a risk with smaller black holes, since they have much smaller

radii. If you go to the center of a galaxy and find a supermassive black hole, you might

be able to experience crossing the event horizon.

As you approach the event horizon, a distant observer would think they never saw you enter

it, seeing you stop and fade. The last light you emit trickling up and out, away from the

event horizon. Meanwhile, from your perspective the void of the black hole rises up to meet

you, as light from fewer directions can reach you. The blackness envelopes you until your

only view of the universe you left is a tiny spot of light.

Here, inside the event horizon, space and time are so horribly broken that real time

travel is possible, so it’s probably a good thing that nothing gets out. If anything could

escape it could create all sorts of time travel paradoxes and issues that break the universe.

As scary as the event horizon is, it keeps us safe from that drama.

Whether you have survived this long doesn’t really matter, as now there is only the certainty

of crushing death in your near future. Inside the event horizon space time itself is so

bent and warped, that whatever direction you move here, every “forward” you go, leads

only towards the center of the black hole. Trying to go any direction only brings you

to the center faster. To survive the longest, you must do: nothing.

In the center of the black hole, we find the singularity. A single point with all the matter

that has ever crossed the event horizon, all crushed to a point infinitely small. There

is no memory of the things that made it as stuff disappears down the black hole trapdoor

forever. The singularity makes all things equal. This actually breaks the universe in

really cool ways. We made a whole video about this problem if you want to learn more. But

in a nutshell, everything that comes too close becomes black hole matter, concentrated at

This lack of a memory of its past, means that a black hole has only three properties: their

mass, spin, and electric charge. Everything else is lost. They’re a lot like fundamental

particles in that respect. This actually means that every single black hole in the universe

is the same. Sure, their mass is different and some spin faster than others. But If we

were to put all the singularities into a magical physics museum, they would be identical, like

But just like fundamental particles, the properties of singularities are the best ways we can

describe them on paper, rather than an accurate representation of reality. Our current theories

about the Universe, namely general relativity, are just not able to describe or explain them.

The curvature of space becomes infinite, density becomes infinite, and our rules just don’t

make sense. The singularity has no surface or size, something like a divide-by-zero error

in the universe. So singularities might not even exist or be completely different things.

But this is all we know right now, from the best prediction we have, from our best current

Also, basically everything you’ve ever heard about black holes, even in this video, is

about theoretical black holes that aren’t spinning, because their math is so much easier.

But since black holes were born from dying stars that were spinning extremely quickly

in their last moments, as far as we know, all black holes in the universe should be

spinning right now. At incredible speeds too, up to 90 % the speed of light. This means

in reality, black holes are even more screwed up than they usually get credit for.

The singularities of rotating black holes are even wilder. The rotation causes them

to swell outwards into a sort of ringularity. This rotation is so powerful, that space itself

is dragged along. This creates another region around spinning black holes, called the Ergosphere

where it’s impossible to stay still, no matter how hard you try. Like a rushing whirlpool

of spacetime, the tide is irresistible and black hole makes you orbit it whether you

Ok. So what will happen with black holes as the universe ages and dies around them? Again,

we don’t know but have some ideas based on our current understanding of physics: Hawking

radiation. In quantum field theory the vacuum of space is boiling with quantum fluctuations.

These fluctuations are creating matter and antimatter pairs of particles from nothing

which only exist for a very short time before annihilating. When this happens near the event

horizon of a black hole, one of these particles can fall in, stopping them from annihilating.

The escaping particle is Hawking radiation. Ultimately, the mass of this particle must