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B1 Intermediário Inglês 10:45 Educational

Travel INSIDE a Black Hole

Vsauce · 33,637,027 visualizações · Adicionado há 3 semanas

Estatísticas de aprendizado

B1

Nível CEFR

5/10

Dificuldade

Legendas (128 segmentos)

00:00

Hey, Vsauce. Michael here. And today we are going to go inside a black hole. It's not

00:07

going to be comfortable, but it will be pretty fun. Now, first thing's first: mathematically

00:13

speaking, anything could become a black hole, if you were to compress it into a small enough

00:19

space. That's right, you, me, this camera - everything in the unvierse has what is known

00:24

as a "Schwarzschild radius." A tiny, tiny amount of space that, were you to collapse the entire

00:31

mass of the object into, its density would be so great that its gravitational pull would

00:38

be so great that not even light could escape from it. You would have a black hole.

00:45

If you were to compress Mount Everest into something smaller than a nanometer, you would

00:50

have a black hole. And if you were to compress the entire Earth down to the size of a peanut,

00:56

you would have a black hole.

00:57

But, fortunately for us, there is no known way to compress Everest or Earth in that fashion.

01:03

But a star, many, many, many times larger than our own Sun, has a much larger Schwartzchild

01:09

radius, and when it runs out of fuel and can no longer keep itself hot enough, it collapses

01:15

to a single, infinitesimally-small point known as a "singularity."

01:20

Its density will be infinite and so its gravitational pull will be so strong that

01:25

nothing can escape, not even light.

01:29

But enough about ways black holes form, let's jump into one. First question: what would

01:34

it look like from the outside? Well, we know that gravitational fields bend space and time.

01:41

Stars behind our Sun will actually appear to be in slightly different locations from

01:46

Earth, because the Sun's gravitational field bends the light coming from those stars.

01:52

When it comes to the gravitational fields of larger objects, like entire galaxies or,

01:57

for that matter, a black hole, the effect is even nuttier. Light coming from object's

02:02

behind them is significantly distorted, producing smears and smudges.

02:07

As seen from Earth, the blue galaxy behind this red galaxy is completely distorted, like

02:13

a fun house mirror. So, rather than appearing as it really should, it looks to us like a ring -

02:19

a smudge all the way around the red galaxy.

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