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Table of contents

0:33
13.800 millones de años atrás
1:30
13.400 millones de años atrás
2:18
13.000 millones de años atrás
4:01
12.500 millones de años atrás
5:30
9.000 millones de años atrás
6:09
4.600 millones de años atrás
7:59
3.500 millones de años atrás
8:45
600 millones de años atrás
9:16
200 millones de años atrás
9:45
Tiempos modernos
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00:00:00
Our universe was born
00:00:02
billions of years ago and since then it has
00:00:04
given rise to millions of galaxies.
00:00:07
Our solar system and who knows what
00:00:10
else has been evolving for 13.8 billion
00:00:14
years,
00:00:15
so exactly how
00:00:18
did we get here? Well, fasten your
00:00:22
seat belt because Today
00:00:25
we will go back in time to go through
00:00:28
the history of the universe in just 10
00:00:33
minutes in the beginning there was
00:00:38
nothing suddenly the Big B happened and created
00:00:42
our
00:00:45
universe you are right maybe it was
00:00:48
something more complicated than that but the
00:00:50
beginning of such a cosmic event is still
00:00:53
a
00:00:54
mystery The truth is that once
00:00:57
it started it never stopped in a matter of
00:01:01
milliseconds particles such as
00:01:04
quarks and photons were formed some of the
00:01:06
basic components of the world that
00:01:08
surrounds us today within 2 minutes
00:01:13
other elements appeared I am referring to
00:01:15
protons and neutrons They came together
00:01:17
to form elements like helium and
00:01:21
deuterium. Then the universe spent 400
00:01:24
million years expanding rapidly.
00:01:31
After hundreds of millions of years of
00:01:34
chaotic expansion, things
00:01:36
slowed down with the appearance of
00:01:39
the first structures of the universe
00:01:41
that we know. Imagine them as the
00:01:44
ingredients that formed stars and
00:01:46
galaxies, even planets like Earth. This is
00:01:49
where we witness the formation
00:01:52
of primordial gas clouds made of
00:01:55
helium and hydrogen, two of the elements
00:01:58
that were created previously. These
00:02:01
clouds have been compacted for
00:02:03
millions of years thanks to gravity and
00:02:06
once created they slowly began to
00:02:09
gain more and more density
00:02:12
HM perhaps it would be better for us to accelerate a
00:02:18
little as the gas clouds
00:02:20
approached each other and became
00:02:22
denser, they became hotter
00:02:25
when the center of some reached
00:02:27
10 millions of degrees Kelvin
00:02:29
caught fire, causing the process
00:02:32
you know as nuclear fusion. The
00:02:35
hydrogen atoms combined to form
00:02:37
helium, releasing a lot of energy. From one
00:02:41
moment to the next, the first star
00:02:44
in our universe was born and it was not the only one,
00:02:47
of course, among all those
00:02:49
thousands of cosmic clouds. Millions of stars
00:02:52
appeared, but they were not
00:02:54
simple bright balls made of light,
00:02:57
but indispensable protagonists in the
00:03:00
formation of our universe. The
00:03:02
stars were not all the same at birth.
00:03:05
They assumed different shapes and sizes.
00:03:08
Some were massive
00:03:11
blue giants, others were tiny with red wings.
00:03:15
However, they were not. They only differed according to
00:03:17
size but also by their life cycles,
00:03:20
some glowed for tens of
00:03:23
millions of years and others for
00:03:25
billions and now that we are
00:03:28
observing them we see that something fascinating is
00:03:30
beginning to happen. It seems that they do not
00:03:33
like to spend time alone and that is why
00:03:35
the You see
00:03:37
them group together and it seems that when they join
00:03:40
together and add other particles
00:03:42
such as gas, dark matter and dust, plus the
00:03:45
gravitational forces that make them
00:03:47
attract each other, they form the
00:03:51
Galaxies, thus the Milky Way and Andromeda will be born,
00:03:54
although there are still a couple
00:03:57
of thousand missing. millions of years for it to
00:04:02
happen, hundreds of millions of
00:04:05
years passed and the universe continued to expand,
00:04:08
more galaxies appeared and now they
00:04:10
evolve in
00:04:12
fantastic ways, as we have already explored
00:04:15
in previous episodes, they began
00:04:17
to gravitate towards each other. You see how
00:04:20
important gravity is.
00:04:23
As they come together, they form clusters of
00:04:26
galaxies, that is, the
00:04:28
largest gravitational structures that
00:04:30
we know of. At this point, we also see
00:04:33
some of the stars that
00:04:35
formed at the beginning of the
00:04:37
universe die. How do they do it? Well, they explode and
00:04:41
become supernovas, but don't
00:04:43
feel sorry. for his death because that
00:04:46
sacrifice is necessary to provide
00:04:48
the universe with the essential elements
00:04:50
to later create not only planets but
00:04:53
also life itself regarding
00:04:56
essential elements I must mention
00:04:59
again or dark matter, this
00:05:02
Mysterious substance does not emit or absorb
00:05:04
any light but plays a primordial role in
00:05:06
the
00:05:09
universal fabric although we cannot
00:05:11
see it we know that dark matter
00:05:13
has an enormous force that has
00:05:15
contributed to shaping everything we
00:05:18
know dark matter is more or
00:05:21
less the hidden framework on which they
00:05:25
have gone generating the clusters of
00:05:27
galaxies and other elements of the universe
00:05:29
[Music]
00:05:33
at this point everything becomes more
00:05:36
familiar after the grouping of several
00:05:38
small galaxies the milky way begins
00:05:41
to form and our sister galaxy
00:05:43
andromeda is also at its moment of
00:05:46
origin Meanwhile in
00:05:49
similar galaxies are appearing
00:05:51
solar systems gigantic clouds of gas and dust
00:05:55
collapse under the force of their own
00:05:57
gravities they come together and create young
00:05:59
planets and
00:06:02
star systems get ready because from
00:06:05
here on this whole story becomes more
00:06:10
interesting Well we are away for a few
00:06:13
billion of years and
00:06:14
meanwhile the universe has not stopped
00:06:17
expanding. Now there are many more
00:06:20
solar systems and galaxies and the number
00:06:22
of stars is much greater. Speaking of
00:06:25
stars, the one that is undoubtedly the most
00:06:27
important of all has just
00:06:30
made our
00:06:32
sun after its formation. You can see
00:06:35
that gases and a lot of dust surround it. Over
00:06:38
time, those particles accumulated and
00:06:41
created
00:06:42
planetesimals. The origin of what we today
00:06:44
call the planets of the
00:06:46
solar system. Over time, the planetesimals
00:06:50
became larger and larger
00:06:51
due to countless collisions and
00:06:55
gravitational attractions. One of those
00:06:57
emerging protoplanets is the Earth and
00:07:01
its development. It is marked by a
00:07:03
crucial event. An object the size of Mars
00:07:06
known as Tea collided with our
00:07:08
planetesimal and created what we know today
00:07:11
as the Earth and its moon. Collisions like this
00:07:15
created other
00:07:17
rocky planets. like Mercury, Venus and Mars, in
00:07:20
colder regions of space far from the
00:07:23
sun, giants like Jupiter and Saturn
00:07:25
began to form. Of course,
00:07:28
returning to the rocky planets, if
00:07:30
we look at them closely, they do not
00:07:33
look anything like those that exist
00:07:35
today for some reason. They look much
00:07:38
smoother, just wait a couple of million
00:07:41
years for what is known as
00:07:44
the late intense bombardment to occur, the
00:07:47
cosmic event in which rocky planets
00:07:50
were hit by
00:07:52
gigantic asteroids, said event practically
00:07:55
defined their current appearance.
00:08:01
Well, after thousands After millions of years,
00:08:04
life finally begins to emerge in
00:08:06
the universe, but don't get
00:08:09
too excited because I am referring to
00:08:11
simple, single-celled organisms called
00:08:14
prokaryotes. These lack most
00:08:17
of the essential functions for
00:08:19
current life, but they still represented an
00:08:22
important step in our development. Evolution At
00:08:24
this very moment, billions of them
00:08:27
inhabit your body. It was not long
00:08:30
before oxygen appeared on
00:08:32
Earth and with it
00:08:35
multicellular organisms. The Earth's climate
00:08:37
takes shape and the ozone layer is generated
00:08:39
that protects nascent life. of
00:08:46
space radiation I already know that we keep skipping
00:08:49
billions of years and that a lot has
00:08:51
happened, for example,
00:08:53
microscopic organisms evolved
00:08:56
to become
00:08:58
vertebrate creatures all together and the antecedent
00:09:01
of all vertebrate life forms
00:09:03
on Earth included You, in addition, many
00:09:07
other changes happened during this
00:09:09
period, the plants evolved and the
00:09:11
continents
00:09:16
moved. We have already reached the era of
00:09:18
Pangea and the reptiles, with all their
00:09:21
drawbacks, a mass extinction event
00:09:24
wiped out a large part of the
00:09:26
species that had been patiently
00:09:28
evolving
00:09:30
and created the perfect scenario for
00:09:32
dinosaurs and
00:09:34
mammals to emerge and yes we are approaching the end of
00:09:37
this era Pangea fragmented and laid the
00:09:41
foundations of our
00:09:45
current continents and just like that we have returned
00:09:49
for hundreds of millions of years humans
00:09:53
evolved modern civilization was born
00:09:56
and now we seek to take one step further
00:10:00
what awaits us
00:10:02
space travel climate change
00:10:06
futuristic technologies perhaps to find out we will have to
00:10:08
travel a billion years in the
00:10:10
future but that sounds like a story
00:10:13
for another episode of what would happen
00:10:19
if you liked this video Like and
00:10:23
don't forget to subscribe to our channel
00:10:24
to receive the best throughout the week.

Description:

Solo necesitas estos 10 minutos para ver la historia de TODO nuestro universo. 00:33 13.800 millones de años atrás 01:30 13.400 millones de años atrás 02:18 13.000 millones de años atrás 04:01 12.500 millones de años atrás 05:30 9.000 millones de años atrás 06:09 4.600 millones de años atrás 07:59 3.500 millones de años atrás 08:45 600 millones de años atrás 09:16 200 millones de años atrás 09:45 Tiempos modernos Producido por: https://underknown.com/ Sobre What If en Español: Escenarios de especulación y las posibilidades más remotas que alguna vez te has preguntado, con respuestas científicas entretenidas: eso es What If. Atrévete a preguntarte “¿Qué pasaría si…? y descubre un universo de posibilidades. Síguenos también en Facebook: https://www.facebook.com/unsupportedbrowser https://www.facebook.com/unsupportedbrowser Y en Instagram: https://www.facebook.com/unsupportedbrowser

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