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00:00:00
have already heard the news, the Voyager 2 probe, the most distant from
00:00:04
earth, which
00:00:05
has been traveling through interstellar
00:00:07
space for more than 45 years, suddenly began
00:00:10
sending strange encrypted signals to earth.
00:00:12
And the most interesting thing is that there are
00:00:15
no signs that the probe is broken
00:00:18
or that there is something wrong with it, except for a
00:00:20
mysterious buzzing, they reported at NASA, what
00:00:24
could have happened to him, you
00:00:27
will find the answer in the nightspace telegram channel,
00:00:29
quickly subscribe link in the description
00:00:33
enjoy watching
00:00:35
[music]
00:00:51
[music] the
00:00:59
legendary telescope that opened our
00:01:02
eyes to the secrets of the universe
00:01:04
[music]
00:01:14
and introduced us to the grandiose forces of
00:01:17
whose existence we didn't even
00:01:19
suspect
00:01:25
this is the amazing Hubble Universe
00:01:32
[music] the
00:01:39
extreme limit of the Hubble telescope
00:01:44
the most famous telescope on earth
00:01:47
never touches its surface the
00:01:49
Hubble space telescope moves in
00:01:51
orbit at an altitude of almost 650 km from the earth
00:01:54
it circles the globe every 97 minutes
00:02:01
[music]
00:02:04
its powerful the mirror sees everything
00:02:12
majestic Star factories where
00:02:14
new worlds are born
00:02:18
destructive explosions of stars
00:02:22
and black holes appearing in a new light
00:02:26
Hubble is the key that has revealed some of the
00:02:28
greatest secrets of the universe
00:02:36
but now there is a threat of
00:02:38
losing the telescope forever the
00:02:43
most important instruments have failed the
00:02:47
main camera and a light-splitting
00:02:50
device called a spectrograph
00:02:52
Exited building
00:02:54
gyroscopes that ensure the
00:02:56
correct orientation of the hubble in
00:02:58
space will soon stop working
00:03:00
but the worst thing is that the hubble is falling a
00:03:05
12-ton telescope the size of a school
00:03:08
bus is slowly approaching the
00:03:10
surface of the earth
00:03:12
The only chance for the hubble to survive is us
00:03:14
but the mission to save the telescope could
00:03:17
be very dangerous
00:03:20
I don’t know I could I would ask an astronaut
00:03:24
to risk his life to fly and
00:03:26
fix who it is. Difficult choice that
00:03:29
Everyone makes for himself but if you ask the
00:03:31
astronauts they agree without
00:03:34
hesitation
00:03:38
space shuttle expedition for
00:03:41
maintenance of the hubble which starts
00:03:42
in October 2008
00:03:48
three two one start the
00:03:53
hubble expedition it is calculated
00:03:56
space flight In any case, there is a
00:03:58
risk involved. I made a decision with
00:04:00
my family that this is worth
00:04:02
risking my life for.
00:04:04
Why is it worth taking this risk for an aging telescope that has
00:04:07
almost reached the end of its 20-year life
00:04:09
because Hubble
00:04:12
continues to amaze us with amazing
00:04:14
facts about our universe and it
00:04:17
has not stopped doing this since its launch
00:04:19
in 1990,
00:04:22
astronomers have long wanted to know where
00:04:24
stars like our Sun come from
00:04:30
from the University of Arizona knows that
00:04:33
stars are formed from clouds of gas and dust,
00:04:35
he hopes to find out how these clouds
00:04:38
give birth to stars,
00:04:41
astronomers suspected that the key to the
00:04:43
solution may be in the
00:04:45
Eagle Nebula But even the most powerful ground-based
00:04:47
telescopes could not give it a clear
00:04:49
image in the
00:04:52
spring of 1995, Hester points the
00:04:55
Hubble Space Telescope at the Eagle Nebula
00:04:59
by downloading an image from Hubble Hester
00:05:02
cannot believe his eyes
00:05:03
[music]
00:05:08
Here is the first photograph of the Eagle Nebula,
00:05:11
which is located 6 .5 thousand light
00:05:14
years taken by Hubble, three
00:05:17
giant pillars consisting of gas and
00:05:19
dust are visible; the column on the left has a height of about 4
00:05:22
light years
00:05:29
[music]
00:05:36
They owe their shape to the fact that nearby there are
00:05:39
several very massive very
00:05:41
bright and very hot stars
00:05:43
that give a huge amount
00:05:47
ultraviolet radiation,
00:05:52
this radiation creates such a relief
00:05:56
Never before have these Celestial columns
00:05:59
been presented in such stunning
00:06:00
detail
00:06:07
[music]
00:06:10
for the first time scientists see that each column
00:06:13
is strewn with small clumps of gas,
00:06:15
perhaps these clumps are the missing link in the
00:06:19
process of star formation
00:06:24
[music]
00:06:26
Kester calls these clumps
00:06:28
evaporating gases globules,
00:06:31
or abbreviated as and gg,
00:06:36
the image shows that inside
00:06:39
some Global there are
00:06:41
nascent stars.
00:06:43
This image depicts a very
00:06:46
dynamic process.
00:06:48
This is a photograph of an object in the process of
00:06:51
changing,
00:06:53
during these changes a New
00:06:56
generation of stars appears. Here, for example, you can see a
00:06:59
small red dot, in fact
00:07:01
it is a star
00:07:05
at the top
00:07:12
in the photograph Glo seemed
00:07:14
small, but inside one of them
00:07:17
our entire solar system could easily fit
00:07:19
these clumps of hot gas are the first
00:07:23
stage of star formation and the columns on
00:07:26
which they hang are rightly called the
00:07:28
pillars of creation the
00:07:30
image of the Eagle Nebula obtained by
00:07:33
Hubble shows us the early stage of
00:07:35
star formation
00:07:38
But the next stage is not visible on it How
00:07:41
stars are formed from Global The
00:07:45
answer to this question was given by photographs
00:07:48
taken by Hubble in 1994,
00:07:52
approximately one and a half thousand light years
00:07:55
from the earth, the Orion Nebula is located, like the
00:07:58
Eagle Nebula Orion is the
00:08:00
birthplace of stars
00:08:02
when scientists looked closely at this
00:08:05
image they discovered tiny
00:08:07
dark spots
00:08:17
are flattened disks of gas and patches of
00:08:20
dust left over from the Global from which
00:08:22
stars have recently emerged these spots are
00:08:25
called protoplanetary disks or
00:08:27
abbreviated as plates
00:08:30
warm orange clump in the center
00:08:32
attracts free matter from the
00:08:34
surrounding disk due to this the matter
00:08:37
in the center of the clump is compressed pressure
00:08:39
grows the clump heats up
00:08:44
As a result, it becomes so hot
00:08:46
that nuclear fusion begins in it, so
00:08:49
a star is born,
00:08:51
heat and radiation from nuclear fusion
00:08:54
gives rise to a stellar wind that carries away
00:08:56
most of the free matter of the disk,
00:09:03
but part of this free matter remains
00:09:05
in the orbit of the newborn star,
00:09:10
over time the fragments gather together and
00:09:13
also form nodes and the clumps that
00:09:15
grow and turn into planets,
00:09:21
if you were transported four and
00:09:23
a half billion years ago during the
00:09:25
formation of the sun and the solar system,
00:09:28
then you would see a similar environment.
00:09:33
Hubble showed us how a new
00:09:36
solar system arises and answered the long-standing
00:09:39
question of how ours arose
00:09:41
the sun's own star and our Earth
00:09:52
behind the Eagle and Orion nebulae in the
00:09:54
plane of the Milky Way there are even
00:09:56
larger star-forming regions,
00:09:59
scientists want to know whether stars in
00:10:02
these distant regions go through the same
00:10:03
life cycle
00:10:07
in March 2005, Hubble began transmitting an
00:10:10
image of a new object,
00:10:15
this is the Carina Nebula one of largest
00:10:18
star forming regions in the sky but the
00:10:21
raw data that
00:10:23
Hubble transmits looks nothing like this
00:10:25
picture
00:10:30
creating images that help
00:10:32
scientists solve Mysteries with this
00:10:35
data the task of an expert in
00:10:37
gold image processing Liliya I am partial
00:10:40
to this image not only because of its
00:10:42
aesthetic value but because -due to the fact
00:10:46
that Hubble has been working on it for so long,
00:10:49
it transmits graphical data in the form of a
00:10:52
black and white image, Livi
00:10:54
colors these images in
00:10:56
accordance with the chemical elements
00:10:57
detected by Hubble instruments
00:10:59
[music]
00:11:02
blue indicates oxygen,
00:11:05
red indicates sulfur
00:11:09
and green indicates a whirlpool to assemble the entire
00:11:13
mosaic of 48 individual photographs
00:11:15
take about a year;
00:11:19
photographs of kiwi taken by Hubble
00:11:21
show an area 50
00:11:24
light years long [music]
00:11:27
Here, too, are a globule that will
00:11:30
one day turn into stars surrounded by
00:11:32
planets
00:11:36
among thousands of newborn stars, a
00:11:38
surprise lurks
00:11:41
among the majestic clouds of the carina Hubble
00:11:44
spots a huge star in agony
00:11:49
for scientists dying the star is a chance
00:11:52
to look into the future of our solar
00:11:54
system
00:11:59
what you see in these
00:12:01
Hubble images is a shell of gas that
00:12:03
serves as
00:12:06
their tombstones Peaceful beauty is deceptive
00:12:13
These colored walls the outer layers of a star are
00:12:16
similar to our Sun when a star
00:12:19
runs out of fuel these layers
00:12:21
expand until until the gravity of
00:12:23
the star can no longer hold them, in the
00:12:26
end they fly into space
00:12:33
in 2004, Hubble takes a picture that
00:12:36
allows us to take a look at what
00:12:38
our inevitable death of the
00:12:40
helix nebula will look like after the expansion of the
00:12:43
outer layers of the star, inside there remains a
00:12:45
hot ball of solidified oxygen
00:12:48
carbon, which astronomers call
00:12:49
white dwarf
00:12:58
one day the same thing will happen to
00:13:01
our sun it will run out of fuel and
00:13:04
the sun will turn into a giant red
00:13:06
star
00:13:14
[music]
00:13:16
this is bad news for our world
00:13:18
the temperature on the surface of the planet
00:13:21
will exceed 1000 degrees
00:13:28
all life on earth will die a
00:13:31
wall of hot gas will pass over the earth
00:13:34
will reach the limits of the solar system and
00:13:36
fly into space,
00:13:41
it will incinerate all the planets and moons on
00:13:44
its way, all that remains of our
00:13:47
Sun is a colored spot that will be
00:13:49
visible for thousands of light years,
00:13:55
such as this,
00:13:59
humanity received a warning
00:14:02
in 5 billion years, we need to
00:14:04
move But even the death of our The Sun
00:14:07
cannot be compared with the much more disastrous
00:14:09
destruction
00:14:11
some stars have a mass 100
00:14:13
times more than our Sun the larger
00:14:16
the star the shorter its life and the more
00:14:19
destructive its death
00:14:24
such stars explode in the form of a huge
00:14:27
fireball which is called a
00:14:29
supernova
00:14:32
not all stars can explode in the form a
00:14:35
supernova, for example, the Sun cannot; it
00:14:38
simply does not have enough mass for processes to begin in the core
00:14:40
that lead to the
00:14:43
explosion of the star, but there are many stars in the galaxy
00:14:45
that are definitely capable of this.
00:14:51
Any star is in a state of
00:14:54
fragile balance between gravity,
00:14:56
which pulls inward, and heat pressure,
00:14:58
which is generated due to nuclear
00:15:01
synthesis and is directed outward when
00:15:03
the fuel runs out, the
00:15:05
pressure that ensures equilibrium disappears;
00:15:10
now only gravity acts; the
00:15:14
star collapses inward and explodes.
00:15:19
The fury of a supernova destroys both the
00:15:21
star itself and everything that surrounds it;
00:15:26
if such a star were
00:15:28
close enough to the earth, then a
00:15:30
wave of deadly
00:15:33
x-ray gamma would be sent to us radiation, it would
00:15:35
disable our communications satellites and lead
00:15:37
to global power outages,
00:15:41
in fact, one such giant
00:15:43
star has already exploded in our Galaxy, the
00:15:48
Hubble Space Telescope recorded
00:15:50
the consequences of this explosion
00:16:01
[music]
00:16:02
the blood nebula is the flying
00:16:05
debris of a supernova that
00:16:07
appeared in 1054
00:16:11
[ music] the
00:16:15
supernova explosion was recorded by
00:16:18
Chinese astronomers so we
00:16:20
know exactly when it happened the
00:16:25
flying debris of this supernova
00:16:27
star that exploded A thousand years ago is
00:16:30
still moving at a speed of about 5
00:16:32
million kilometers per hour
00:16:35
But this image is more than
00:16:38
just a photograph of ancient history
00:16:43
interconnected threads like a network
00:16:46
give scientists a clue to the essence of life itself; the
00:16:50
basic elements necessary for the
00:16:52
origin of life are formed in the heart of a
00:16:54
star
00:16:56
when stars explode; these fundamental
00:16:58
elements spread throughout the Universe;
00:17:00
from them, distant clouds of the
00:17:03
nebula arise where new planets
00:17:05
and New life are born
00:17:11
[music]
00:17:16
When you bleed You see that it is
00:17:19
red is hemoglobium its red color
00:17:22
is associated with oxygen and iron that arose in a
00:17:25
supernova the gold from which
00:17:28
your wedding ring is made arose
00:17:30
in a supernova calcium in your bones a
00:17:33
supernova occurred When stars die we
00:17:36
learn a lot about the Universe as a whole
00:17:42
Hubble gives scientists unique knowledge
00:17:44
by tracking one specific a star is a
00:17:48
carina in the carina nebula
00:17:59
[music]
00:18:03
this is a mysterious star; its mass is a hundred times
00:18:06
greater than the mass of the Sun; this is the upper limit; the
00:18:09
greater the mass of a star, the hotter it is; the
00:18:12
surface of this star is so
00:18:14
hot that it cannot hold the gas it
00:18:16
consists of; a
00:18:19
stream of Gas constantly comes out of it.
00:18:21
For more than 10 years, Hubble has been serially
00:18:24
photographing this carina.
00:18:28
In the photo, two huge petals of
00:18:30
super-hot gas are visible that are escaping from
00:18:32
the surface,
00:18:34
although this carina is a young star due to its
00:18:37
enormous mass, it is unstable. This
00:18:39
star will not live long.
00:18:45
Carinae is one of the few stars
00:18:48
that we can point to. finger and
00:18:50
say
00:18:52
when this Killer explodes it will become
00:18:55
one of the most destructive supernovae
00:18:57
in the entire history of observations
00:19:00
when the light of the explosion reaches us it
00:19:03
will be an amazing sight
00:19:05
it will be almost as bright as the full
00:19:08
moon the light will concentrate at one point in
00:19:11
the sky and at night it will cast shadows the
00:19:17
fireworks will begin When the Star
00:19:19
runs out of fuel, the giant star
00:19:21
will collapse in just a few seconds, the
00:19:37
entire brunt of the disaster will fall on the cores of the
00:19:40
exploding star,
00:19:42
when this happens in the place of the star, a
00:19:45
cosmic phenomenon will remain that has
00:19:47
long occupied the imagination of astronomers
00:19:50
[music]
00:19:53
black hole
00:20:09
Mysterious Black hole is the result of a
00:20:12
powerful destructive supernova explosion
00:20:16
at least At least in theory,
00:20:18
before the launch of Hubble, scientists did not
00:20:21
have any strong evidence of
00:20:22
the existence of black holes. The modern
00:20:25
concept of a black hole is based on
00:20:28
Einstein’s general theory of relativity. If you
00:20:30
make matter massive enough and
00:20:33
dense enough, then Gravity will be
00:20:36
so strong that there will be a region of
00:20:38
space where light cannot
00:20:40
escape.
00:20:43
space into which you can get But
00:20:45
from where you can’t get out something like a
00:20:47
cosmic lobster trap
00:20:53
[music]
00:20:55
according to Einstein’s theory a black hole
00:20:58
Arises from a very large star
00:21:02
it must be at least four
00:21:04
times larger than our Sun a black hole
00:21:07
is just a piece of matter that
00:21:09
somehow decreased So its
00:21:12
gravitational field is so strong that
00:21:15
the Trace cannot leave it even if
00:21:18
radiation occurs then photons return
00:21:22
back
00:21:30
during a supernova explosion the inner
00:21:33
core of the star is compressed into one point
00:21:35
smaller than the head of a pin
00:21:39
astronomers call this point the
00:21:41
singularity
00:21:48
singularity is an object not having
00:21:50
lengths of width and height but it has
00:21:54
most of the gravity of the star from
00:21:56
which it emerged
00:21:58
one of the main goals of the hubble was to prove once and
00:22:01
for all that black holes
00:22:02
actually exist or do not
00:22:05
exist
00:22:11
but how to look for an invisible point
00:22:14
astronomers decide to point the hubble at the
00:22:16
exact centers of galaxies
00:22:22
this is the solution justifies itself They
00:22:25
discover that stars close to the center of
00:22:27
the Galaxy move in a circle at a very
00:22:29
high speed
00:22:32
for stars this is abnormal behavior
00:22:34
most stars move at a
00:22:37
relatively low speed
00:22:39
but in the center of galaxies the stars are accelerated by
00:22:42
the gravity of some very massive but
00:22:44
at the same time ultra-compact object such an
00:22:48
effect can have only one
00:22:50
object, the
00:22:51
legendary black hole,
00:23:00
another proof of the existence of
00:23:03
black holes are photographs of a mysterious
00:23:06
jet about 5000 light years long
00:23:08
transmitted by Hubble; the jet passes through the
00:23:11
center of the giant elliptical
00:23:12
galaxy M87; the
00:23:15
jet in the M87 galaxy is formed due to the
00:23:19
fact that the black hole attracts a
00:23:21
huge amount of gas and dust;
00:23:27
the substance is so many things create a
00:23:29
jam gas and dust accumulate form a
00:23:33
disk some of this matter escapes and
00:23:36
forms a jet
00:23:40
[music]
00:23:45
The black hole reveals itself as a
00:23:48
light show
00:24:03
[music]
00:24:09
The Universe
00:24:11
is more than just a sea of ​​stars
00:24:18
[music]
00:24:24
it is a symphony of science
00:24:30
from the point of view of science more
00:24:36
[music]
00:24:40
anyone can understand the tactics using
00:24:43
which I won,
00:24:52
but hidden from all eyes is
00:24:55
the strategy by which I
00:24:57
organized victory The Art of War
00:25:01
Ground War On Thursdays at 21:00 on
00:25:04
the channel I found Jack graph HD
00:25:07
3 2 1
00:25:12
earthquake
00:25:15
Tornado
00:25:18
avalanches how these disasters affect
00:25:21
people Tim Samaras is trying to measure something
00:25:24
that has never been measured, everything is correct, he
00:25:28
risks his life,
00:25:30
knowledge comes to us when something
00:25:32
happens masters of disaster on the
00:25:35
Nat geo HD channel
00:25:37
[music] the
00:25:44
connection between the galaxy and the black hole at
00:25:47
its center is not yet fully understood but
00:25:50
astronomers it is believed that black holes play a
00:25:52
role in the formation of galaxies,
00:26:01
as far as we know,
00:26:04
there is a black hole in the center of any large Galaxy.
00:26:06
We don’t know how exactly this happens.
00:26:08
This is probably due to the fact that as they
00:26:11
evolved
00:26:36
before the advent of Hubble, black holes were
00:26:39
just theories, an unverified
00:26:41
astronomical guess, a
00:26:42
space telescope Hubble changed this forever the
00:26:53
destructive forces that create
00:26:55
stars in deep space form our
00:26:58
own solar system
00:27:00
[music] in
00:27:04
the summer of 1992, Shoemaker's comet Levi 9,
00:27:09
abbreviated shl-9, passes too close
00:27:13
to Jupiter, a
00:27:15
comet with a diameter of 1.8 km falls into the
00:27:20
gravitational field of a giant planet
00:27:22
then sh -9 falls apart
00:27:25
fragments stretch into a long line
00:27:28
the image taken by Hubble is
00:27:30
called the string of pearls
00:27:35
calculations show that these pearls will
00:27:37
soon collide with Jupiter
00:27:41
so astronomer Heidi Hamel, who
00:27:44
specializes in the study of planets,
00:27:46
makes a proposal to NASA for many
00:27:49
decades we have known that collisions
00:27:51
play an incredibly important role in the evolution of the
00:27:54
solar system,
00:27:56
craters on the moon show that
00:27:58
collisions are important even on earth as we
00:28:01
have known for many years collisions played a
00:28:03
big role but we never had
00:28:06
the opportunity to see the collision
00:28:12
comet shoemaker livi 9 would show that
00:28:15
such collisions are possible not only in
00:28:18
the past but also in present and even in
00:28:20
the future,
00:28:26
one of the difficulties in observing
00:28:29
Shoemaker's Comet Pleve-9 is
00:28:31
that Hubble tracks the event in
00:28:34
real time, usually the telescope
00:28:36
is aimed at events that
00:28:37
unfold over millions of years
00:28:39
and the death of the comet will occur quickly
00:28:46
in July 1994, the team meets in
00:28:50
Scientific Institute of the Space Telescope
00:28:52
in Baltimore to observe the
00:28:54
collision of a comet with a planet,
00:28:59
we did not know what would happen when the
00:29:01
Shoemaker Levi-9 crashed into Jupiter
00:29:04
It is quite possible that nothing would have happened
00:29:07
at all, the
00:29:10
first image of the
00:29:12
Shoemaker Swan comet was received, there were no
00:29:15
traces of the collision,
00:29:25
but then new ones came
00:29:28
look
00:29:32
at the pictures Lord Look at this look
00:29:39
The planet rotated enough so that
00:29:42
the trace of the collision became visible on its disks
00:29:48
the group watched the collision of the comet with the
00:29:51
planet in real time before their eyes
00:29:54
Cosmic history was being made reporters
00:29:57
and cameras were ready in the audience
00:29:59
above
00:30:00
At the same time the press was going on on the screen
00:30:03
-conference and Gene Shoemaker
00:30:05
said If only we could
00:30:07
Look at this and we sat on the ground
00:30:10
floor and shouted Wow, look, it’s
00:30:12
amazing we need to show this, we ca
00:30:14
n’t have him sitting at a
00:30:16
press conference and saying that we don’t
00:30:18
know,
00:30:20
I was standing in letters a they were sitting at a
00:30:22
small table,
00:30:24
I think that we have fresh information for a
00:30:48
whole week, according
00:31:45
to our calculations, the pillars from the explosions on
00:31:49
Jupiter rose to a height of 3000
00:31:51
kilometers above its atmosphere,
00:31:53
this is a colossal planetary scale,
00:31:57
the explosions turned out to have a strong thermal
00:32:00
effect on the clouds within a radius of many
00:32:02
thousands of kilometers,
00:32:04
the clouds heated up to temperatures of
00:32:07
tens of thousands of degrees
00:32:10
if such an object as Shl-9 crashed into the
00:32:14
earth It would be a bad day.
00:32:19
Pictures of the collision with the Comet
00:32:21
taken by Hubble prove that the
00:32:23
destructive processes that formed
00:32:25
our planet billions of years ago do not
00:32:27
stop and today
00:32:32
Shoemaker's comet Levi 9 deals a
00:32:34
devastating blow to Jupiter,
00:32:36
located not far from us But when
00:32:38
Hubble points at an empty patch of the distant
00:32:41
sky, its discovery shocks the scientific
00:32:44
community in the
00:32:49
winter of 1995, a series of commands are transmitted to the on-board computer of the
00:32:53
Hubble that
00:32:55
turns the orbital telescope
00:32:58
towards a seemingly empty patch of sky
00:33:07
[music] the
00:33:09
powerful optics of the Hubble monitor the
00:33:12
same In the same region of Space, over the course of 10
00:33:14
days,
00:33:15
the telescope takes a series of photographs which are
00:33:18
called the Hubble Deep Field
00:33:24
project. The Hubble Deep Field project was a great idea
00:33:27
to point the space telescope at one
00:33:29
area of ​​​​the sky and leave it in this
00:33:31
position, take exposure after
00:33:34
exposure over and over again, then
00:33:36
connect them together and as a result
00:33:38
look very deep into the universe,
00:33:41
this is the essence of the Hubble Defield project, we
00:33:44
looked very far into the universe,
00:33:45
we saw Galaxies, thousands of thousands of galaxies
00:33:49
filled with stars, fields that look
00:33:52
like a photograph of fireflies taken at night,
00:33:55
and yet this part of the sky
00:33:58
is considered empty
00:34:03
[music]
00:34:05
every spot of light in this photograph
00:34:07
Hubble is a Galaxy consisting of
00:34:09
billions of stars, these Galaxies
00:34:11
are photographed at different stages of
00:34:13
evolution
00:34:21
from the time shortly after the
00:34:23
birth of the cosmos and ending with the appearance of
00:34:26
spiral galaxies such as our
00:34:28
Milky Way image The Hubble deepfield
00:34:32
is strewn with debris from space,
00:34:33
galaxies that collide and
00:34:36
absorb each other
00:34:47
[music]
00:34:58
[music]
00:35:11
by We estimate that
00:35:14
there are hundreds of billions of galaxies in the Universe,
00:35:16
but you don’t realize it until
00:35:19
you see the Deep Field crab picture and
00:35:22
realize that it’s only a tiny piece of
00:35:24
the sky, but it’s filled to the brim with galaxies,
00:35:27
then you see that the Universe is an
00:35:30
amazing place full of stars, a wonderful place
00:35:34
all history of the evolution of galaxy change
00:35:37
recorded in one image Hubble Deep Field
00:35:43
Perhaps the most important discovery of Hubble
00:35:46
cannot be seen at all. In no way is
00:35:56
it such a powerful force that it
00:35:59
holds the entire Universe together
00:36:03
[music]
00:36:06
For years, astronomers such
00:36:10
as Kim Weaver have been surprised by the behavior of
00:36:13
galaxies,
00:36:16
the objects we have observed such as
00:36:19
Galaxies have puzzled us, for example, with the
00:36:22
way the Galaxy rotates, the
00:36:28
arms of spiral galaxies move
00:36:31
faster than the laws of physics allow,
00:36:34
astronomers have discovered other oddities,
00:36:40
there is a cluster of galaxies that
00:36:43
includes thousands of galaxies, these clusters are
00:36:46
nevertheless connected to each other.
00:36:49
Galaxies after all this time move
00:36:52
in orbits What connects their cluster is
00:37:05
something that we do not see, astronomers
00:37:08
hypothesize that galaxies
00:37:18
They call it dark matter Although
00:37:22
dark matter cannot be seen, one
00:37:24
astronomer found a way to find it
00:37:31
for more than two years We
00:37:34
collected 600 images from the
00:37:36
Hubble Space Telescope like a mosaic, adding them up
00:37:39
together we got a large area of ​​the sky
00:37:41
in which about 2 million
00:37:44
faint galaxies were visible this was the
00:37:47
cosmological study of the
00:37:48
Hubble Space Telescope this was the most
00:37:51
extensive study conducted from
00:37:53
space the study showed that stars
00:37:55
and galaxies are formed from ordinary
00:37:57
matter which is held by gravity
00:37:59
inside the clouds of dark matter
00:38:02
three-dimensional model clouds of dark matter
00:38:05
created by Hubble for the first time in history
00:38:07
shows how Dark Matter forms
00:38:09
the framework of our Universe
00:38:14
shortly after the Big Bang The
00:38:16
gravitational framework of the Dark Universe
00:38:18
formed the basis for evolutionary
00:38:20
changes throughout the cosmos
00:38:29
We owe our very existence to the
00:38:32
framework of dark matter that
00:38:34
formed early in the development of
00:38:36
the Universe Although Dark matter is important for the
00:38:39
very fact of our existence,
00:38:41
astronomers do not yet have any
00:38:42
idea what it is;
00:38:49
this table shows all the elements of
00:38:52
the Universe that we encounter in
00:38:55
everyday life;
00:38:57
all physical matter that we can
00:39:00
see, taste or touch
00:39:02
are in this table
00:39:04
but not Dark matter,
00:39:12
thanks to Hubble, astronomers have found a way to
00:39:15
detect and measure it. They found out
00:39:18
that there is five times more dark matter in the Universe
00:39:20
than physical matter.
00:39:24
But even if we add dark matter
00:39:26
to all the physical matter that
00:39:28
makes up the stars of the planet and people, it
00:39:31
turns out that it’s still not about
00:39:33
two-thirds of the universe is enough
00:39:35
so what is the rest of
00:39:38
the universe made of
00:39:39
scientists are again turning to hubble for
00:39:42
answers the
00:39:48
hubble telescope is changing our understanding of
00:39:50
reality
00:39:55
since the 20s of the 20th century astronomers knew that
00:39:59
the universe was expanding they believed that
00:40:02
one day gravity would slow down the expansion and
00:40:04
even possibly make the universe
00:40:06
stop
00:40:11
I know that the Universe is slowing down
00:40:14
its expansion, the only question is at what
00:40:16
speed the answer to this question should
00:40:18
have put an end to the debate about the age and
00:40:21
fate of the Universe, his search turned
00:40:23
into a race;
00:40:25
there were two groups of scientists who
00:40:28
did not like each other. They tried to
00:40:30
measure the rate of expansion of the Universe in
00:40:33
different periods of the past. and compare it
00:40:35
with the speed at which it is expanding
00:40:37
now
00:40:42
such a check can be carried out by Hubble;
00:40:44
it finds supernova explosions in
00:40:46
distant galaxies and uses the light of
00:40:49
the explosion as a means to measure the
00:40:51
distance from the Earth to the galaxy,
00:40:57
but the data obtained by Hubble does not
00:40:59
fit into the accepted model of the expansion of
00:41:01
the universe of a
00:41:06
Galaxy with supernovae They’re not
00:41:08
just moving away, they’re moving away faster
00:41:30
and faster. Hubble results force astronomers to completely reconsider their views on the Universe. You throw a ball and it slows down and falls back. You don’t expect the ball to fly up faster and faster. It doesn’t happen,
00:41:33
but it happens anyway. according to Hubble,
00:41:36
the Universe is expanding faster and
00:41:39
faster,
00:41:40
the only explanation is just as
00:41:43
simple as it is incredible, something is
00:41:45
causing the Universe to expand faster, an
00:41:48
invisible force called dark
00:41:51
energy,
00:41:54
dark energy is another manifestation of a
00:41:57
force we are familiar with, we are familiar with Gravity,
00:42:00
but we have never seen it like
00:42:02
this before manifested itself, but the darkest
00:42:04
side of this mysterious force is connected with
00:42:07
its future, over time its influence will
00:42:09
increase, this means that one day
00:42:12
dark energy will become stronger than
00:42:14
Gravity, it will overcome even those forces
00:42:17
that hold atoms together,
00:42:20
everything that is connected together will be separated,
00:42:23
including in reality low
00:42:25
Saturday level It seems that the days of our
00:42:29
Universe are numbered One day it will perish in a
00:42:32
cosmic Apocalypse which scientists
00:42:35
call the big rip
00:42:38
[music]
00:42:46
this is a reward For thinking boldly
00:42:50
We went beyond the limits We did not at all
00:42:52
expect such a result this is a
00:42:55
colossal revolution in our understanding of
00:42:57
the Universe Imagine that we don't
00:43:00
know anything about the sea and one day we discover
00:43:02
the ocean to our surprise we find out that
00:43:04
three quarters of the earth is covered by the ocean but we
00:43:07
have no idea what the ocean is and
00:43:10
why it is needed
00:43:11
this is our current knowledge about dark
00:43:14
energy
00:43:24
continuing research into dark energy
00:43:26
this is perhaps the most important reason to
00:43:29
leave Hubble in orbit but how much longer
00:43:32
can we operate?
00:43:43
Almost 20 years have passed since its launch, but the
00:43:46
Hubble Space Telescope continues to
00:43:49
improve
00:43:52
after the completion of the Hubble servicing mission,
00:43:54
from the docking of the Shuttle Atlantis, a
00:43:56
new wide-angle Planetary Camera 3 will begin to operate,
00:43:59
which will expand
00:44:01
the capabilities of Hubble;
00:44:05
another new device is a spectrograph
00:44:08
of origin space will give us new
00:44:10
knowledge about how Dark Matter affects
00:44:12
distant galaxies.
00:44:17
But even after installing the new
00:44:19
equipment, Hubble's days will be numbered
00:44:21
because the astronauts will also install
00:44:24
a device on it that will put an end to
00:44:25
Hubble's long space journey
00:44:34
when the mission is completed and all the
00:44:37
work is done, there will come a time when
00:44:40
we will need to return to the airlock, I'm
00:44:42
absolutely sure that will be the last
00:44:44
time I touch Hubble for the last time,
00:44:46
I will look at it for the last time because I think that will be the
00:44:49
last time people visit the
00:44:51
space telescope.
00:44:54
So many people have put their work into it and I will say goodbye
00:44:57
to mine before let's send him on
00:45:00
a journey to meet a new discovery
00:45:05
it will be a touching farewell
00:45:19
to me It's hard to imagine that the mission of the
00:45:21
space telescope will end
00:45:24
now it is at the peak of
00:45:27
efficiency, that is, it will be at its peak
00:45:29
when we repair it, there is a
00:45:31
great demand for it its capabilities are unique
00:45:34
and will remain unique
00:45:36
when we can no longer using
00:45:38
the hub for observations it will be a huge
00:45:42
loss
00:45:46
on this day the telescope will receive the last
00:45:49
command to turn off and return to
00:45:52
earth the
00:46:04
orbital telescope will burn up upon entering the
00:46:06
earth's atmosphere and will go down in history
00:46:13
[music]
00:46:24
[music]
00:46:26
flight control specialists want the
00:46:29
huge telescope to
00:46:31
fall into the The Pacific Ocean
00:46:42
for those of us who have used hubble
00:46:45
it will be a bittersweet moment the crumble has been the
00:46:48
bright side of our lives has allowed us
00:46:50
to do a wonderful job but at the same
00:46:53
time we are looking to the future the
00:46:57
next generation of space
00:46:59
telescope is called the
00:47:01
james webb space telescope its launch is
00:47:04
scheduled for 2013
00:47:09
the telescope is literally sense, it will go
00:47:12
further than Hubble, it will be located on the far
00:47:15
side of the Moon at the point of fragile
00:47:17
balance of the gravitational fields of the Earth,
00:47:19
the Moon and the Sun
00:47:21
[music] the
00:47:23
James Space Telescope that
00:47:26
will come can get an image of a
00:47:28
planet orbiting another
00:47:30
star, we expect not only to find
00:47:33
planets similar to the Earth, but also to
00:47:35
chemical analysis of their atmosphere
00:47:37
to determine if there are signs of life there
00:47:40
this is not science fiction not dreams we are
00:47:43
very close to achieving this goal
00:47:45
thanks to science going further than
00:47:48
Hubble allowed but Hubble will forever
00:47:50
remain the first
00:47:53
first space telescope and the
00:47:56
number one telescope for everyone
00:48:00
it is used by scientists but photographs
00:48:03
taken this telescope was
00:48:05
accessible to the public like never before in
00:48:08
terms of publicity. It
00:48:10
revolutionized astronomy if you woke up a
00:48:12
randomly selected resident of
00:48:14
this country in the middle of the night and asked him to name
00:48:16
any telescope then Name it.
00:48:33
I hope that in the future we will find a way to
00:48:37
replace it because
00:48:45
[music]
00:48:53
it made thousands of revolutions around the Earth
00:48:59
was Eyes wide open Very
00:49:02
inquisitive creatures he gave us
00:49:05
amazing photographs thanks to which the
00:49:07
human mind went to the beginning
00:49:11
of us to be constantly surprised
00:49:26
[music] the
00:49:40
program was voiced by the ark TV studio the text
00:49:43
was read by Peter Tabelevich

Description:

🪐NIGHT SPACE ПОДПИСАТЬСЯ: https://t.me/+-7S4DX7iUHswODVi «Двери во Вселенную открыты - приглашаем тебя войти и познать все ее тайны!» В видео содержится контент, защищенный авторским правом. Правообладатель разрешил нам использовать видео. Правообладатель "National Geographic" монетизирует это видео. Авторские права соблюдены. Подробная информация тут https://support.google.com/youtube/ -Copyright Disclaimer Under Section 107 of the Copyright Act 1976, allowance is made for "fair use" for purposes such as criticism, comment, news reporting, teaching, scholarship, and research. Fair use is a use permitted by copyright statute that might otherwise be infringing. Non-profit, educational or personal use tips the balance in favor of fair use. No copyright infringement intended. -I Do Not Own Anything.All the Rights in This Content Belong to Their Respective Owner/

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