Explore
For Enterprise
Join for Free
Log In

artes y humanidades
Negocios
Ciencias de la Computación
Ciencia de Datos
Tecnología de información
salud
Matemáticas y Lógica
Desarrollo Personal
Ciencias Físicas e Ingeniería
Ciencias sociales
Aprendizaje de un idioma
Grados
Certificados

Explorar todo lo que Coursera tiene para ofrecer

Explorar
Buscar
For Enterprise
Inicia Sesión
Únete de forma gratuita

1-5 Beginning of the Universe Look Far into the Past I

Loading...

From the Big Bang to Dark Energy

Universidad de Tokio

4.8 (1,531 calificaciones) | 40K estudiantes inscritos

We have learned a lot recently about how the Universe evolved in 13.7 billion years since the Big Bang. More than 80% of matter in the Universe is mysterious Dark Matter, which made stars and galaxies to form. The newly discovered Higgs-boson became frozen into the Universe a trillionth of a second after the Big Bang and brought order to the Universe. Yet we still do not know how ordinary matter (atoms) survived against total annihilation by Anti-Matter. The expansion of the Universe started acceleration about 7 billion years ago and the Universe is being ripped apart. The culprit is Dark Energy, a mysterious energy multiplying in vacuum. I will present evidence behind these startling discoveries and discuss what we may learn in the near future. This course is offered in English.

Revisiones

4.8 (1,531 calificaciones)

5 stars
1,284 ratings
4 stars
217 ratings
3 stars
24 ratings
1 star
6 ratings

LF

Feb 29, 2016

This was an excellent course! It was very interesting, well-explained, and easy to follow (even for someone like me, who isn't necessarily up-to-date on mathematics). Can't recommend enough!

VK

Jan 02, 2017

Maybe the best course I have taken so far. Very interesting subject great professor and perfect distribution of content. Would like to see another course by professor Murayama in the future.

De la lección

From Daily Life to the Big Bang

Understanding the Universe in which we live and how to probe it can begin with simple daily life experiences such as night and day and the four seasons. Starting from these observations, we will take a journey from our local Earth at the present time all the way to the edge of the universe and back to its birth, learning the techniques and findings in modern physics that provide us this understanding.

1-5 Beginning of the Universe Look Far into the Past I13:31

1-6 Beginning of the Universe Look Far into the Past II5:45

1-7 Beginning of the Universe Look Far into the Past III6:41

1-8 Beginning of the Universe Look Far into the Past IV8:54

1-9 Beginning of the Universe Look Far into the Past V10:20

1-10 Cosmic Expansion6:26

Impartido por:

Hitoshi Murayama
MacAdams Professor of Physics, University of California, Berkeley

Transcripción

So now, before getting to this evidence that black holes actually

exist in our universe, we'd like to start our journey from nearby.

And by gradually going away from us, you're

looking in farther and farther away in the universe.

But what that means also, is that you're

looking farther and farther back into the past.

And that's the way we begin our journey back to the big bang.

So let's start that journey.

So, thinking something that is fairly nearby.

So this is a picture of the International Space Station.

Where you can see the astronauts actually even working outside the space station.

And these pictures are very impressive.

Because, now, that shows that humans have

developed to the extent that we can actually

leave the earth, get into outer space and have even a station, outside the earth.

But if you actually look it up, you’ll find

something which may be surprising to you: The International Space Station,

is floating above the earth at the altitude of 275 kilometers.

That's not that much of a difference, distance, right?

If you think of the fact that the diameter of

the earth is 12,000 kilometers, this is actually not very much.

So, if you think of the Earth, planet Earth, as a, let's say, a fruit,

peach, then how much you actually move up...

To the International Space Station.

It's only a skin depth of a peach. So you see, it's actually not very much.

So that also tells you that moving into, farther away

the universe is actually not a very easy thing to do.

You can send probes, though.

And of course, people have managed to even go to the moon, as well.

So, this video clip

is showing the image of a space probe named

Kaguya, which Japan has launched a couple of years ago.

And what this probe has done, is go to

the other side of the moon, and gradually come back.

And while it's coming back, the, you know, the Earth

was in the shadow of the moon, itself, for a while,

but then you start seeing the Earth getting into your

view So, this is the Earth rise instead of Sun rise.

You see, the Earth is such

a beautiful planet. Of course, we have to protect it.

but, you know, this is a really impressive picture because of that.

And now, just by thinking about how far away the moon is.

It's actually 380,000 killometers away. From the Earth.

Much much farther away than the International Space Station.

And because the distances we talked about in the universe

are so big, we typically use, time, rather than the distance

to describe how far away these objects are, using

light, it takes 1.3 seconds to reach the moon.

So we say, the moon, is a distance of 1.3 light seconds away.

As a matter of fact, the Apollo astronauts who have actually been to

the moon, placed a piece of mirror on the surface of the moon.

We can send a laser light from the earth with just the mirror in 1.3

seconds, it gets bounced back to the earth 2.6 seconds later.

So, that's the way we can measure the distance to the moon, extremely precisely.

These days.

Anyway, so this is the picture from this Kaguya probe.

It's just a beautiful picture of our planet Earth.

The object, that is of course very familiar to us,

and very important to us, of course, is the sun.

This is even farther away.

It's takes more than 8 minutes for light to reach.

The sun.

So in terms of kilometers, it's 1.5 times 10 to the 8th kilometers.

You can see this actually pretty far away object.

But we see so much abundant li- sunlight from the sun.

Because sun really radiates incredible amount of energy.

So that's the origin of the warm and heat on

our planet Earth.

And, as we discussed earlier, the solar system consists of

quite a few planets, while revolving around the sun.

And we are actually the third planet, as you see, in this picture.

And that's the solar system.

And again, to get some idea on the distance involved here, Japan has launched

yet another probe Called Hayabusa a couple of

years ago, which managed to reach this asteroid

named Itokawa.

And when this object Hayabusa, that's a, a space probe, eventually landed

on this asteroid Itokawa it was a distance of 20 light minutes away.

From the earth.

So when the command center sends a command to

this probe, it takes 20 minutes to reach it.

And then Hayabusa was trying to land on this

asteroid, it asks for the control, direction and speed,

exact way to land and so on.

And then when it sends back the, the information back

to the command center, that takes another 20 minutes.

And, then sending a signal back would take yet another 20 minutes.

That's not the way to do it, obviously.

So this probe had to have this own control own artificial intelligence on board,

that it could decide if it was going with the right speed, the right angle.

To the right distance, to the right location

on its own.

So, it takes that much time to send back and forth

the communication signals to a distance even within our solar system.

And if you think about even the farther away outer planet, like

Neptune, it takes 4 hours for the light signal to get there.

So, our solar system, as you can see, is really, pretty big.

And do you know what is the human

made object that moved away from us the farthest possible, so far?

That is a space probe launched by NASA, in

the United States, about like, 30 years ago named Voyager.

And it passed by planets like Jupiter and Saturn on their

way And, and sent us very beautiful pictures of those planets.

And, and, they're still moving away from the solar system.

Only this year,

we were, we learned that the Voyager has basically left the solar system.

And went even farther into deep-, farther deeper into the universe.

So where Voyager is now is 16 light-hours away.

If you go to NASA website, you can see the

precise location of Voyager, we're still communicating with the probe.

And the numbers of the distance just keeps ticking

up as you watch, so it's still in communication

with us.

And on this space probe Voyager that we have put in, say, a

metal plate that has the etching of the human drawings, human letters, some

of the

pictures, even CD recordings music and so on, hoping that

maybe one day an alien might be able to actually

find it, and send us a signal back that, we

found your stuff, And we are still waiting for that.

But, do you know how much that might actually take in the end?

So here's the picture of the closest star, where we might possibly

hope that the aliens might be able to pick up this space probe.

Voyager, that's

hi-res

. And name of the star is Proxima Centauri

and the distance to this star is actually a long distance even for light

It takes more than 4 years, 4.2 lightyears away.

And the Voyager took 30 years to get to this distance of 16 light-hours away.

In order to get there, it will still take tens

of thousands of years.

So maybe we can wait for the signal from alien that soon, unfortunately.

But anyway.

So this is the closest star, we can

find around us that's already several light years away.

And we have many of these stars in our own Milky Way galaxy.

And the Milky Way is named by the fact that

the stars all line, all lined up in a way that

it might look like a milk flowing. That's a milky way.

And the reason why the stars look like this is because we're

embedded into a disk of this Milky Way galaxy And you might

be, actually, surprised to hear is that we are not at the

center of this milky way galaxy, but actually in a suburb, out here.

And in this galaxy, there are something like a hundred billion stars and

we are actually located 28,000 light years away from the center of the galaxy.

So that's you know, a pretty far away suburb, that's where we live in.

And the shape of this galaxy is actually like this, if you look at it from sideways.

It's fairly thin - it's only 1,500 light years thick.

And we are way, like I said, 28,000 light years away from the center.

And because of

the shape of this disc.

We are here looking towards the center of the galaxy, everything's inside the disc.

And that's why the stars look like flowing along a river.

And that's why we observe the milky way.

So that's the structure and shape of our own galaxy.

But, because we're actually off centered, it's like the Earth...

Off centered from the sun.

Our solar system is revolving around the center of galaxy over many, many years.

And this is actually going at even incredible speed.

It's actually that our solar system is moving

at a speed of 220 kilometers Per second.

That's an incredible speed.

But then you should ask the following question, right?

If the

solar system is moving so fast, why is it still kept inside our Milky Way?

What is pulling us inside? What is the source of that strong gravity?

Well, then you might ask the following question.

Maybe there's are objects like Black Hole at the center of galaxy

that's pulling us, that's why we can stay inside the Milky Way galaxy.

So let's now take a look into the center of the galaxy.

So, this is the video showing zooming in

towards the center of galaxy by using powerful telescopes.

You see a lot of this black stuff, they're actually dust.

And dust is not really black.

It's just that it creates a shadow, we can't see the stars beyond them.

But using something called infrared light, we can

go around that dust, and see what's beyond it.

And we can observe the motion of stars at the center of galaxies.

And just

watch this star. It goes like, you know, quook!

Quick, right?

It's being pulled towards something, gets accelerated, and then once its actually

get close, very close to the center of, of the object here.

Goes like,

this one here. Quick.

So it's clear that something very heavy is pulling this star.

It's accelerated.

And

after it passes through

passes through, goes back also very quickly.

So, this is the cleaned up image by using computer processing.

So, what we have to do is watch the motion of these stars over, like, 20 years.

You know, it takes that long years.

For these stars to orbit around this very heavy object.

And by studying the motion of these stars,

you can even determine how massive the object is.

Just like we could determine the mass

of the sun by using the force of gravity that's

keeping us around, in the elliptical orbits around the sun.

And the answer turned out to be staggering.

This object is 4 million times heavier than our sun,

and nothing can be that heavy, except for a black hole.

There is a black hole, a super-massive black

hole, at the center of our Milky Way galaxy.

So, there's a black hole. And, that was discovered by many people.

And this is one of my, my colleagues,

[UNKNOWN]

working at Berkeley.

And, and so they determined the mass of the black hole is,

like I said, is 4 million times the mass of the sun.

And if you observe other galaxies beyond our Milky Way Galaxy, some of them have

even heavier super massive black holes, as heavy

as billion times the mass of the sun.

And as we talked about before, black holes can

swallow things, but nothing can come out of it because

even the speed of light is not enough to

escape the force of gravity from the black hole.

So, if a blackhole swallows things around it, it

falls into it and it would never come out.

Even light does not come out from it.

You can never see it anymore, but just before gas

might enter the blackhole, it gives us the last word.

It likes a scream!

[NOISE]!

It lights up! And you can actually observe that!

So if you observe this video here, then if

you look closely at the location of the black

hole, sometimes it just brightens up a little bit,

and like 30 minutes later, it fades back down.

So that's the last word we hear... From the gas falling into the black hole.

Well now that we have learned that this black hole is

4 million times heavier than the Sun, that's an incredible mass.

But we also learn that our solar system could not be bound to the, our Milky

Way galaxy by the force of gravity of hundred billion stars, right?

So even the black hole as heavy as 4 million times

the sun wouldn't be able to keep us inside the Milky Way.

We still need more mass to be kept inside our solar system.

What do you think that

could be?

So that's the subject of the next discussion.

Explora nuestro catálogo

Inscríbete de manera gratuita y obtén recomendaciones personalizadas, actualizaciones y ofertas.

Coursera brinda acceso universal a la mejor educación del mundo, al asociarse con las mejores universidades y organizaciones, para ofrecer cursos en línea.

© 2019 Coursera Inc. Todos los derechos reservados.

Descargar en la App Store

Consíguelo en Google Play

Coursera
Acerca de
Liderazgo
Empleo
Catálogo
Certificados
Certificados MasterTrack™
Grados
For Enterprise
For Government

Comunidad
Learners
Partners
Developers
Beta Testers
Translators

Conectar
Blog
Facebook
LinkedIn
Twitter
Instagram
Youtube
Blog de Tecnología

Más
Términos
Privacidad
Ayuda
Accesibilidad
Prensa
Contacto
Directorio
Afiliados