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  7. Exploring the Enigma of Black Holes | National Geographic

Exploring the Enigma of Black Holes | National Geographic

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Delve into the mysterious world of black holes, where gravity reigns supreme, light cannot escape, and the laws of physics cease to exist. Learn about the event horizon and singularity that make these cosmic objects among the most captivating in the universe.
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0:00
(mysterious music)
0:03
- [Woman] Black holes are among
0:04
the most fascinating objects in our universe,
0:07
and also the most mysterious.
0:14
A black hole is a region in space
0:16
where the force of gravity is so strong,
0:18
not even light, the fastest known entity
0:20
in our universe, can escape.
0:23
The boundary of a black hole is called the event horizon,
0:27
a point of no return, beyond which we truly cannot see.
0:32
When something crosses the event horizon,
0:34
it collapses into the black hole's singularity,
0:37
an infinitely small, infinitely dense point
0:40
where space, time, and the laws of physics no longer apply.
0:46
Scientists have theorized several different types
0:48
of black holes, with stellar and supermassive black holes
0:52
being the most common.
0:54
Stellar black holes form when massive stars
0:57
die and collapse.
0:59
They're roughly 10 to 20 times the mass of our sun,
1:02
and scattered throughout the universe.
1:05
There could be millions of these stellar black holes
1:07
in the Milky Way alone.
1:10
Supermassive black holes are giants by comparison,
1:14
measuring millions, even billions of times,
1:17
more massive than our sun.
1:19
Scientists can only guess how they form,
1:21
but we do know they exist at the center
1:24
of just about every large galaxy, including our own.
1:29
Sagittarius A, the supermassive black hole
1:32
at the center of the Milky Way,
1:33
has a mass of roughly four million suns,
1:36
and has a diameter about the distance
1:38
between the earth and our sun.
1:42
Because black holes are invisible,
1:44
the only way for scientists to detect
1:46
and study them is to observe their effect
1:48
on nearby matter.
1:50
This includes accretion disks,
1:52
a disk of particles that form when gases and dust
1:55
fall toward a black hole, and quasars,
1:58
jets of particles that blast out
2:00
of supermassive black holes.
2:04
Black holes remained largely unknown until the 20th century.
2:09
In 1916, using Einstein's general theory of relativity,
2:13
a German physicist named Karl Schwartzschild
2:16
calculated that any mass can become a black hole
2:19
if it were compressed tightly enough.
2:22
But it wasn't until 1971 when theory became reality.
2:27
Astronomers studying the constellation Cygnus
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