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The Most Dangerous Supermassive Giant Black Hole in the Universe Documentary HD 1080p

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The Most Dangerous Supermassive Giant Black Hole in the Universe Documentary HD 1080p

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Universe - How The Super Black Hole Was Created | Discovery Documentary 1080p.

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Full Documentary Films: SUPERMASSIVE BLACK HOLES Space Exploration Documentary. A super massive black hole is thought to form from the joining of .
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The Most Dangerous Supermassive Giant Black Hole in the Universe Documentary HD 1080p

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On our channel a lot of interesting documentaries on such themes: to destroy the Land, kill the Earth, end of Earth, the death Land, death Land, doomsday, Armageddon, Apocalypse, space, about space, star, stars, universe, galaxy, big Bang the big Bang theory, constellation, planet, solar system, satellite, UFO, aliens, Earth, planet Earth, Moon, Mars, Jupiter, Venus, Saturn, Uranus, Neptune, Pluto, mercury, astronaut, rocket, meteor, comet, astronomy, matter, quasar, telescope, meteor, Infinity, planets, Sun, Hubble, asteroid, documentary, black hole, quasar, national geographic documentary, full documentary, discovery documentary, history documentary, bbc documentary, national geographic, the universe, discovery channel, stephen hawking, brian greene, Neil deGrasse Tyson,
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Monster BLACK HOLE | Full Documentary

Monster Black Hole traces the life cycle of a black hole, from its violent beginnings in the early universe, to its growth to supermassive proportions at the center of a galaxy, and its death in deep time.

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The Largest Black Holes in the Universe

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Our Milky Way may harbor millions of black holes... the ultra dense remnants of dead stars. But now, in the universe far beyond our galaxy, there's evidence of something far more ominous. A breed of black holes that has reached incomprehensible size and destructive power. Just how large, and violent, and strange can they get?

A new era in astronomy has revealed a universe long hidden to us. High-tech instruments sent into space have been tuned to sense high-energy forms of light -- x-rays and gamma rays -- that are invisible to our eyes and do not penetrate our atmosphere. On the ground, precision telescopes are equipped with technologies that allow them to cancel out the blurring effects of the atmosphere. They are peering into the far reaches of the universe, and into distant caldrons of light and energy. In some distant galaxies, astronomers are now finding evidence that space and time are being shattered by eruptions so vast they boggle the mind.

We are just beginning to understand the impact these outbursts have had on the universe: On the shapes of galaxies, the spread of elements that make up stars and planets, and ultimately the very existence of Earth. The discovery of what causes these eruptions has led to a new understanding of cosmic history. Back in 1995, the Hubble space telescope was enlisted to begin filling in the details of that history. Astronomers selected tiny regions in the sky, between the stars. For days at a time, they focused Hubble's gaze on remote regions of the universe.

These hubble Deep Field images offered incredibly clear views of the cosmos in its infancy. What drew astronomers' attention were the tiniest galaxies, covering only a few pixels on Hubble's detector. Most of them do not have the grand spiral or elliptical shapes of large galaxies we see close to us today.

Instead, they are irregular, scrappy collections of stars. The Hubble Deep Field confirmed a long-standing idea that the universe must have evolved in a series of building blocks, with small galaxies gradually merging and assembling into larger ones.

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Supermassive black holes: Most Powerful Objects in the Universe - Space Discovery Documentary

A supermassive black hole (SMBH or sometimes SBH) is the largest type of black hole, containing a mass of the order of hundreds of thousands to billions of times the mass of the Sun (M☉). Black holes are a class of astronomical object that have undergone gravitational collapse, leaving behind spheroidal regions of space from which nothing can escape, not even light. Observational evidence indicates that nearly all large galaxies contain a supermassive black hole, located at the galaxy's center.[3][4] In the case of the Milky Way, the supermassive black hole corresponds to the location of Sagittarius A* at the Galactic Core.[5][6] Accretion of interstellar gas onto supermassive black holes is the process responsible for powering quasars and other types of active galactic nuclei.

Supermassive black hole The Unknown Universe Documentary - Space Discovery Documentary

The star's outer layers spew out into space, but the inside implodes, becoming denser and denser, until there is too much matter in too little space. The core succumbs to its own gravitational pull and collapses into itself, in extreme cases forming a black hole

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Monster Black Hole - How the Universe Works (S04E03)

How the Universe Works - Monster Black Hole (Season 4/Episode 3).
Black holes are the least understood places in the universe, where the rules of physics collapse. We go inside the super-massive black hole in the center of the Milky Way.

Archived for educational purposes only. No copyright infringement intended. All rights belong to Discovery.

#HowTheUniverseWorks #MonsterBlackHole #Documentary

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Quasars: the Brightest Black Holes - Professor Carolin Crawford

Quasars are among the most dramatic objects anywhere in the cosmos. They emit prodigious amounts of energy, all due to a supermassive black hole at the heart of a galaxy. Visible far across the Universe, quasars can be used to trace both the early life of galaxies, and the properties of the intervening space.

The transcript and downloadable versions of the lecture are available from the Gresham College website:

Gresham College has been giving free public lectures since 1597. This tradition continues today with all of our five or so public lectures a week being made available for free download from our website. There are currently over 1,500 lectures free to access or download from the website.
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The Most Dangerous Supermassive Giant Black Hole in the Universe Documentary HD 1080p

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Universe | The Most Dangerous Supermassive Giant Black Hole in the Universe

The idea of a body so massive that even light could not escape was briefly proposed by astronomical pioneer and English clergyman John Michell in a letter published in November 1784. Michell's simplistic calculations assumed that such a body might have the same density as the Sun, and concluded that such a body would form when a star's diameter exceeds the Sun's by a factor of 500, and the surface escape velocity exceeds the usual speed of light. Michell correctly noted that such supermassive but non-radiating bodies might be detectable through their gravitational effects on nearby visible bodies. Scholars of the time were initially excited by the proposal that giant but invisible stars might be hiding in plain view, but enthusiasm dampened when the wavelike nature of light became apparent in the early nineteenth century.[13] If light were a wave rather than a corpuscle, it became unclear what, if any, influence gravity would have on escaping light waves. Modern relativity factually dispels Michell's notion of a light ray shooting directly from the surface of a supermassive star, being slowed down by the star's gravity, stopping, and then free-falling back to the star's surface.

Full Space Documentary - Monster Black Holes

Astronomers have discovered the oldest supermassive black hole ever found — a behemoth that grew to 800 million times the mass of the sun when the universe was just 5 percent of its current age, a new study finds.

This newfound giant black hole, which formed just 690 million years after the Big Bang, could one day help shed light on a number of cosmic mysteries, such as how black holes could have reached gargantuan sizes quickly after the Big Bang and how the universe got cleared of the murky fog that once filled the entire cosmos, the researchers said in the new study.

Supermassive black holes with masses millions to billions of times that of the sun are thought to lurk at the hearts of most, if not all, galaxies. Previous research suggested these giants release extraordinarily large amounts of light when they rip apart stars and devour matter, and likely are the driving force behind quasars, which are among the brightest objects in the universe. [The Strangest Black Holes in the Universe]

Astronomers can detect quasars from the farthest corners of the cosmos, making quasars among the most distant objects known. The farthest quasars are also the earliest known quasars — the more distant one is, the more time its light took to reach Earth.

The previous record for the earliest, most distant quasar was set by ULAS J1120+0641. That quasar is located 13.04 billion light-years from Earth and existed about 750 million years after the Big Bang. The newfound quasar (and its black hole), named ULAS J1342+0928, is 13.1 billion light-years away.

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Biggest Black Holes and Cosmic Monsters Documentary 2015

A combination of ground-based and spacecraft observations has
uncovered two black holes of 10 billion solar masses in the nearby
Universe. The finding sheds light on how these cosmic monsters
co-evolve with galaxies.
Giant black holes, with masses of a few billion times that of the
Sun, have fascinated scientists, science-fiction writers and the general
public alike since they were first proposed1
four decades ago. These
supermassive black holes, which lurk in the centre of galaxies, are not
just theoretical curiosities. Their existence was convincingly demon-
strated 15 years ago, and soon astrophysicists realized that such black
holes can have profound effects on how galaxies form2
. This realiza-
tion spurred a flurry of studies aiming to understand the joint evolution
of galaxies and black holes. On page 215 of this issue, McConnell
et al.3
present the detection of the two most massive black holes ever
found. They argue that their finding provides a key missing piece of
evidence to our understanding of how galaxies and black holes form.
The existence of monster black holes was originally invoked to ex-
plain the intense energy released by active galaxies known as quasars.
These galaxies are especially numerous at very large distances from
Earth, corresponding to a time when the Universe was less than half its
current age. Their tremendous brightness is thought to be the last flash
from gas accelerated to extreme speed before being accreted by a giant
black hole in the galaxys nucleus. There is now less gas in the nearby
Universe than there was at early epochs, because most of it was used
to make stars. For this reason, no quasar exists in our cosmic back-
yard. However, if supermassive black holes are responsible for quasars
power production, they should still lie dormant in the centre of the most
massive nearby galaxies.
Indeed, systematic searches for supermassive black holes have
found them at the centre of all massive galaxies for which reliable de-
terminations of the black-hole mass exist (see McConnell et al.3
for
an up-to-date list). But such black holes are not massive enough to
power the brightest quasars. The ideal candidate galaxies for hosting
these largest black holes are the massive elliptical galaxies found at
the centre of galaxy clusters. Like giant spiders at the centre of a web,
these galaxies lie at the bottom of a clusters gravitational potential well,
feeding their black hole by accreting gas and stars from neighbouring
galaxies. However, the nearest big galaxy cluster to Earth is about 100
megaparsecs away, and this large distance makes determining the mass
of their putative black holes a challenge.
McConnell et al.3
targeted the central elliptical galaxy of two mas-
sive clusters, using two of the worlds largest telescopes and observa-
tions from the Hubble Space Telescope. They found two black holes,
each with a mass of more than 10 billion solar masses, in the nuclei
of the two galaxies. These objects probably represent the missing dor-
mant relics of the giant black holes that powered the brightest quasars
in the early Universe.
The mass of the supermassive black holes studied so far is closely
related to the amount of random motion — the velocity dispersion —
of the stars in the central parts of the host galaxies4,5

Documentary 2015 - Black Holes and Cosmic Monsters Space FULL HD

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Deep Space | Inside a Black Hole - Documentary HD 2017

Deep Space | Inside a Black Hole - Documentary HD 2017Black Holes Space Documentary

Monster Black Holes - New NOVA Space Documentary 2015 HD

A black hole is a mathematically defined region of spacetime exhibiting such a strong gravitational pull that no particle or electromagnetic radiation can escape from it. The theory of
general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.[2][3] The boundary of the region from which no escape is possible is called the event
horizon. Although crossing the event horizon has enormous effect on the fate of the object crossing it, it appears to have no locally detectable features. In many ways a black hole acts like
an ideal black body, as it reflects no light. Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black
body of a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for black holes of stellar mass, making it essentially impossible to observe.

Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general
relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although its interpretation as a region of space from which nothing can escape was first published by
David Finkelstein in 1958. Long considered a mathematical curiosity, it was during the 1960s that theoretical work showed black holes were a generic prediction of general relativity. The discovery
of neutron stars sparked interest in gravitationally collapsed compact objects as a possible astrophysical reality.

Black holes of stellar mass are expected to form when very massive stars collapse at the end of their life cycle. After a black hole has formed, it can continue to grow by absorbing mass from its
surroundings. By absorbing other stars and merging with other black holes, supermassive black holes of millions of solar masses (M☉) may form. There is general consensus that supermassive black
holes exist in the centers of most galaxies.

Despite its invisible interior, the presence of a black hole can be inferred through its interaction with other matter and with electromagnetic radiation such as visible light. Matter falling
onto a black hole can form an accretion disk heated by friction, forming some of the brightest objects in the universe. If there are other stars orbiting a black hole, their orbit can be used
to determine its mass and location. Such observations can be used to exclude possible alternatives (such as neutron stars). In this way, astronomers have identified numerous stellar black hole
candidates in binary systems, and established that the radio source known as Sgr A*, at the core of our own Milky Way galaxy, contains a supermassive black hole of about 4.3 million M☉.


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Best Documentary 2017 The Universe S01E12 THE MOST DANGEROUS PLACE IN THE UNIVERSE BluRay 1080p

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Scientist describe the current understanding of exotic stars; magnetars, black holes and quasars with an obsession about how they would kill you. Galaxy .

Supermassive Black Holes (Science Documentary 2017)

A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it.[1] The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.[2][3] The boundary of the region from which no escape is possible is called the event horizon. Although the event horizon has an enormous effect on the fate and circumstances of an object crossing it, no locally detectable features appear to be observed. In many ways a black hole acts like an ideal black body, as it reflects no light.[4][5] Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for black holes of stellar mass, making it essentially impossible to observe.

Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although its interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were long considered a mathematical curiosity; it was during the 1960s that theoretical work showed they were a generic prediction of general relativity. The discovery of neutron stars sparked interest in gravitationally collapsed compact objects as a possible astrophysical reality.

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