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Monster BLACK HOLE | Full Documentary

  • Monster BLACK HOLE | Full Documentary

    50:01

    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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  • Biggest Black Holes and Cosmic Monsters - Space Documentary 2015

    1:23:28

    Biggest Black Holes and Cosmic Monsters - Space Documentary 2015
    Astronomers have identified a mammoth black hole weighing as much as 12 billion suns.


    It's not the biggest black hole ever found, but it's astonishingly young. The giant appears to have swelled to its enormous size only 875 million years after the big bang, when the universe was just 6 percent of its current age. That's a surprise, astronomers report Wednesday in the journal Nature, because giant black holes are thought to grow relatively slowly by vacuuming up gas and even stars that venture too close.

    How do you build such a big black hole in such a short time? asks Xue-Bing Wu of China's Peking University, lead author of the study.

  • Monster Black Hole - How the Universe Works

    43:02

    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

  • Monster Black Holes - New NOVA Space Documentary 2015 HD

    1:6:24

    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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  • Black Holes National Geographic Documentary HD

    50:33

    Black Holes National Geographic Documentary HD
    Documentaries Documentary HD BBC National Geography History Animal Planet
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  • The Most Dangerous Supermassive Giant Black Hole in the Universe Documentary HD 1080p

    49:31

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

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  • Nova Documentary - Black holes - Space Documentary 2020

    55:27

    Nova Documentary - Black holes - Space Documentary 2020


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  • Biggest Black Hole in the center of Galaxy HD documentary

    1:14:16

    Astronomers are closing in on the proof they've sought for years that one of the most destructive objects in the universe -- a super massive black hole -- lurks at the center of our own galaxy..

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    Astronomers are closing in on the proof they've sought for years that one of the most destructive objects in the universe -- a super massive black hole -- lurks at the center of our own galaxy...
    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 ...

    National Geographic Documentary | Black Holes & Monsters of Universe | Science Documentary Full HD Black holes of stellar ...

    A supermassive black hole (SMBH) is the largest type of black hole, on the order of hundreds of thousands to billions of solar masses (M☉), and is found in the ...

    Supermassive Black Hole at the Center of the Galaxy - Space Documentary 2016 A supermassive black hole (SMBH) is the largest type of black hole, on the ...

    Astronomers are closing in on the proof they've sought for years that one of the most destructive objects in the universe -- a super massive black hole -- lurks at ...

  • MONSTER BLACK HOLE WITH MASS OF 66,000,000,000 SUNS... TON 618

    10:55

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  • Black Holes

    50:33

    Subscribe to Naked Science -

    Every other Wednesday we present a new video, so join us to see the truth laid bare...

    Somewhere in our galaxy, at some time in the future, a spacecraft from Earth will encounter the most dangerous object in the Universe. A stunning visual journey into black holes, their structure and their creation.

    A black hole is a geometrically defined region of spacetime exhibiting such strong gravitational effects that nothing, including particles and electromagnetic radiation such as light, can escape from inside it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.

  • National Geographic: The Largest Black Hole In the Universe Documentary HD

    24:59

    Astronomers have discovered the largest and most luminous black hole ever seen — an ancient monster with a mass about 12 billion times that of the sun — that dates back to when the universe was less than 1 billion years old.

    It remains a mystery how black holes could have grown so huge in such a relatively brief time after the dawn of the universe, researchers say.

    Supermassive black holes are thought to lurk in the hearts of most, if not all, large galaxies. The largest black holes found so far in the nearby universe have masses more than 10 billion times that of the sun. In comparison, the black hole at the center of the Milky Way is thought to have a mass only 4 million to 5 million times that of the sun.

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  • Monster Black Hole With Mass of 40,000,000,000 Suns

    10:36

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  • Monster of the Universe Black Hole Documentary

    58:56

    A black hole is a region of spacetime from which gravity prevents anything, including light, from escaping. The theory of general relativity predicts that a sufficiently compact mass will deform.

    Monster Black Holes in the Universe - Documentary 2017 A supermassive black hole found only a billion years after the Big Bang adds to growing questions about how such black holes grew so quickly..

    Astronomers have discovered the largest and most luminous black hole ever seen — an ancient monster with a mass about 12 billion times that of the sun — that dates back to when the universe.

  • BBC Documentary - How To See A Black Hole 1080i HDTV

    59:01

    A BBC documentary about one of the greatest discoveries of humans by a team of top scientific minds from different parts of the world known as the Event Horizon Telescope project team guided by Dr Sheperd Doeleman of the Smithsonian Astrophysical Observatory, on a mission to capture the first ever picture of a black hole with a mega virtual telescope the size of the earth, by combining radio observatories and telescope facilities from all over the world to make up this earth-size virtual telescope.

    All the videos, songs, images, and graphics used in the video belong to their respective owners and I or this channel does not claim any right over them.

    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 favour of fair use.
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  • Secret Monster Black Holes and Time - New BBC Documentary 2015 HD

    1:11:09

    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 Monster Black Holes & Space Documentary

    50:03

    Thanks for watching Please Like, Share, Comment and Subscribe A black hole is a mathematically defined region of spacetime exhibiting such a strong gravitational pull that no particle or electromag.

    Black Holes and other Cosmic Monsters - Full Space Documentary Subscribe for more videos: Read more: . Welcome To Space & Science Channel.be entertain,learn . Black Holes, Parallel Universes,.

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    Monster of the Milky Way : Black Holes Astronomers are closing in on the proof they've sought for years that one of the most destructive objects in the.

  • The Largest Black Holes in the Universe

    24:59

    For more 4K space, and more great History and Science than you'll ever watch, check out our sister network...

    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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  • Unintentional Asmr Monster Blackhole Documentary guarantee deep sleep

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  • Documentary 2015 - Black Holes and Cosmic Monsters Space FULL HD

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  • Black Holes 101 | National Geographic

    3:11

    At the center of our galaxy, a supermassive black hole churns. Learn about the types of black holes, how they form, and how scientists discovered these invisible, yet extraordinary objects in our universe.
    ➡ Subscribe:

    #NationalGeographic #BlackHoles #Educational

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    National Geographic is the world's premium destination for science, exploration, and adventure. Through their world-class scientists, photographers, journalists, and filmmakers, Nat Geo gets you closer to the stories that matter and past the edge of what's possible.

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  • BBC Space Documentary Monster Black Holes and Time Science Documentary 2014 HD

    45:58

    BBC Space Documentary Monster Black Holes and Time Science Documentary 2014 HD

  • Supermassive black hole The Unknown Universe Documentary - Space Discovery Documentary

    35:03

    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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  • Whats Inside A Black Hole? | Unveiled

    9:16

    What's Inside A Black Hole?
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    Black holes are mysterious and bizarre objects in the universe that really have no explanation. In fact, we hardly know anything about what lies inside of a black hole. We know and understand what we see on the outside of a black hole, but we have no way of going inside one to take a look at what is really happening. Even if we sent a probe inside a black hole, it would not survive the journey, and there would be no way that the probe could transmit a signal outside once it had been sucked inside. This is because a black hole is the product of mass being squeezed together so densely, and so tightly, that it creates a gravitational pull that is so strong, that not even light can escape its grasp.

    Supermassive black holes with masses millions to billions of times that of the sun are thought to lurk at the hearts of all galaxies in the universe. You may notice that when you see a photo of a spiral galaxy, such as the Milky Way, in the center of the galaxy is a giant mass of light, which many people would think looks like a massive sun.

    But this is not light coming from the black hole itself. Remember, that light cannot escape the heavy gravitational pull. Instead, the light we see comes from the magnetic fields near a spinning black hole that propel electrons outward in a jet along the rotation axis. The electrons produce bright radio waves. Quasars are believed to produce their energy from massive black holes in the center of the galaxies in which the quasars are located. Because quasars are so bright, they drown out the light from all the other stars in the same galaxy.

    You’re probably asking, ‘well, what’s a quasar?’ A Quasar is the short name for ‘quasi-stellar object’ and is a very highly energetic object surrounding an actively feeding Supermassive Black Hole. In more basic terms, the Supermassive Black Hole in the middle of a galaxy feeds intermittently. As it feeds, gas swirls around it at incredible speeds and forms an insanely bright hot orbiting disk. And if the black hole is swallowing a large amount of material, this feeding is accompanied by gigantic jets of gas. These are called Quasar. They are essentially fueled by the Black Holes they orbit.

  • Doomsday: 10 Ways the World Will End: PLANET DESTROYING BLACK HOLE | History

    10:29

    Scientists believe millions of Black Holes exist in our galaxy and have the capability to destroy everything in its path. What would happen if a black hole sucked Earth into its deadly vortex? Find out in this clip from Season 1, Black Hole. #Doomsday
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  • Journey to a Black Hole - Uncovering a Mystery | SPACETIME - SCIENCE SHOW

    47:29

    We are surrounded by an intangible infinity: a universe in which the Earth is merely a grain of sand on the shore of an ocean. But we are unravelling more and more of the secrets of the universe which surrounds us. And that includes black holes, bottomless pits like the jaws of hell which devour all material that comes too close to them. Even light has no chance of escaping from them. But how does a Black Hole form? Are there any near us? And can they pose a threat to us? A look at the universe presents us with pictures of fascinating and confusing beauty: landscapes of light and gas and stardust, formed by cosmic wind and radiation. Our telescopes are discovering more and more wonders of the universe. They are looking far out into space and thus far back into the past. The centre of our galaxy is marked by a super-heavy Black Hole: an astronomical object with an inconceivable gravitational pull. Nothing can escape from it. The black hole at the centre of our galaxy is known as Sagittarius A-star. Of enormous size, it devours everything while remaining totally invisible.

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  • What to Expect if Earth Ever Falls Into a Black Hole?

    10:03

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  • What Happens If 1 mm Black Hole Appears On Earth?

    9:00

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  • How do we know theres a black hole in every galaxy centre? | History of Supermassive Black Holes

    25:49

    At the centre of every galaxy, there is a supermassive black hole (a million to a billion times bigger than the Sun). But how do we even know that? There are so many scientific results that have jigsaw-pieced together throughout the past century that allow us to know that now, so join me, as I go through decade by decade and explain the significance of all the results that have built up the big picture.

    00:00 - Introduction
    00:53 - 1900s
    03:58 - 1910s
    05:50 - 1920s
    06:58 -1930s
    09:04 - 1940s
    11:00 -1950s
    12:09 -1960s
    17:14 - 1970s
    18:38 - 1980s
    19:40 - 1990s
    22:12 - 2000s
    23:28 - 2010s

    Here are links to all the papers I mentioned throughout the video, again listed by decade (note that et al. is Latin for and others):

    Michell (1784) -

    Fath (1909) -
    Einstein (1915) -
    Schwarzschild (1916) -

    Lemaître (1927) -
    Hubble (1929) -

    Einstein (1931; cosmological constant introduced) -
    Chandrasekhar (1931) -
    Tolman (1939) -
    Oppenheimer & Volkoff (1939)

    Seyfert (1943) -
    Bolton, Stanley & Slee (1949) -

    Baade & Minkowski (1954) -
    Burbidge (1959) -

    Minkowski (1960) -
    Giacconi (1962) -
    Hoyle & Fowler (1963) -
    Schmidt (1963) -
    Kerr (1963) -
    Salpeter (1964) -
    Zel’dovich (1964) -
    Schmidt & Matthews (1964) -
    Schmidt (1965) -
    Penrose (1965) -
    Hawking (1967) -
    Hewish, Bell et al. (1968) -
    Lynden-Bell (1969) -

    Lyden Bell & Rees (71) -
    Wolfe & Burbidge (1974) -
    Bardeen, Carter & Hawking (1973) -
    Bekenstein (1973) -
    Balick & Brown (1974) -
    Sargent et al. (1978) -

    Dressler (84) -
    Kormendy (88) -

    Harms et al. (1994) -
    Miyoshi et al. (1995) -
    Urry & Padovani (1995) -
    Faber et al. (1997) -
    Magorrian et al. (1998) -

    Ferrarse & Merritt (2000) -
    Gebhardt et al. (2000) -

    Hopkins et al. (2006) -
    Simmons, Smethurst & Lintott (2017) -
    Martin et al. (2018) -

    ---

    ???? My book: Space at the Speed of Light is now available in the USA & Canada!

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    ????????‍???? Dr Becky Smethurst is an astrophysicist researching galaxies and supermassive black holes at Christ Church at the University of Oxford.

  • Inside the black hole image that made history | Sheperd Doeleman

    11:30

    At the center of a galaxy more than 55 million light-years away, there's a supermassive black hole with the mass of several billion suns. And now, for the first time ever, we can see it. Astrophysicist Sheperd Doeleman, head of the Event Horizon Telescope collaboration, speaks with TED's Chris Anderson about the iconic, first-ever image of a black hole -- and the epic, worldwide effort involved in capturing it.

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  • Supermassive Black Hole in the Milky Way Galaxy

    20:09

    See the updated, expanded version of this video:


    From a distance, our galaxy would look like a flat spiral, some 100,000 light years across, with pockets of gas, clouds of dust, and about 400 billion stars rotating around the galaxys center. Thick dust and blinding starlight have long obscured our vision into the mysterious inner regions of the galactic center. And yet, the clues have been piling up, that something important, something strange is going on in there. Astronomers tracking stars in the center of the galaxy have found the best proof to date that black holes exist. Now, they are shooting for the first direct image of a black hole.

    From a distance, our galaxy would look something like this.

    A flat spiral, some 100,000 light years across, with pockets of gas, clouds of dust, and about 400 billion stars rotating around the galaxy's center.

    That center -- bulging up and out of the galactic disk -- is tightly packed with stars.

    Thick dust and blinding starlight have long obscured our vision into the mysterious inner regions of this so-called bulge.

    And yet, the clues have been piling up, that something important...something strange... is going on in there.

    The first to take notice was the physicist Karl Jansky back in the 1930s.

    He was asked by his employer, Bell Telephone Labs, to investigate sources of static that might interfere with what it saw as the killer app of its time... radio voice transmissions.

    Using this ungainly radio receiver... Jansky methodically scanned the airwaves. He documented thunderstorms, near and far... and another signal he could not explain.

    It sounded like steam -- a hiss of radio noise. Jansky narrowed it to a spot in the constellation of Sagittarius, in the direction of the center of the galaxy.

    Located within a larger pattern of radio emissions... ... Jansky's sighting would become known as Sagittarius A*.

    The word of Jansky's finding got out. He assured the public that it was not aliens seeking contact.

    But that's just about all anyone could say... for over three decades.

    Then Erik Becklin got on the case.

    Becklin is one of those rare researchers whose curiosity and determination push our understanding to a whole new level.

    It was the 1960's and astronomy, like society, was in a period of ferment. Startling new observations were being made... and new interpretations were in the air.

    Quasars had just been discovered... extremely bright beacons of light from deep space. Were they coming from the centers of distant galaxies? And what powerful objects were generating them?

    To study an event at the center of a galaxy, you have locate it. Young Becklin first took aim at our neighboring galaxy, Andromeda.

    In ultraviolet light, you can see a dense glow in the middle. Becklin found the point where the light reaches peak intensity... and marked it as the Center.

    From our orientation in space, all of the Andromeda galaxy is in full view.

    But our galaxy is a different story. We live inside it, of course. Becklin had to find a way to see through all the dust and gas that obscure our line of sight into the center. So he went to a military contractor...

    ...and obtained a device that reads infrared light... whose wavelengths are similar to the distances between particles in a dust cloud, allowing them to move right through.

    Becklin began measuring the brightness of the light as it rose to a peak... marking the location of the galactic center.

    Pinpointing this site would now allow astronomers to begin probing for details with a new generation of powerful telescopes... to peer into the bright lights... the forbidden zones... deep in the heart of the Milky Way.

    Becklin wasn't the only astronomer interested in the galactic center.

    Reinhardt Genzel, and a team based at the Max Planck Institute for Extraterrestrial Physics in Germany, began a similar campaign in 1990... from the New Technology Telescope in the mountains of Chile.

    A few years later, in 1993, high atop Hawaii's Mauna Kea volcano...

    Eric Becklin and colleagues, including Andrea Ghez, began using the newly christened Keck Telescope. The American and German groups shared the same goal... to pinpoint the precise location of Sagittarius A*, and find out what it is.

    Because the object is too small to see... at 26,000 light years away... they would study it by tracking the orbits of stars around it.

    Even seeing them would take the sensitivity of Keck's wide aperture; an instrument powerful enough to detect a single candle flame at the distance of the moon...

    Meanwhile, using a similar technique, astronomers had focused the new Hubble Space Telescope on a different galaxy... a giant elliptical cloud of nearly a billion stars, lying some 50 million light years away called M87.

  • What If a Black Hole Ate the Sun?

    5:26

    It's almost as old as the Universe, and as massive as 34 billion Suns. It eats stars for breakfast. And now it's about to consume our own. Behold, the great and powerful black hole with the catchy name J2157. If it came close enough to our Solar System, how fast would it destroy us? How would it all go sideways for our Sun? And how exactly would this monstrous black hole end all life on Earth?

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  • What If Two Black Holes Collided?

    5:08

    Black holes are the gravitational monsters of the Universe. They are so powerful that nothing, even light, can escape their grasp. One black hole is bad enough. But if you took two black holes and smashed them into each other, they'd be capable of changing the shape of space itself. How epic would that explosion be? And could it somehow reach the Earth?

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  • Black Hole Size Comparison 2019

    6:01

    Signup for your FREE trial to The Great Courses Plus here:

    In this video we take a look at the size of black holes in our Universe, from stellar mass black holes formed from a collapsing star to the Ultramassive ones that hold galaxies together. Enjoy!

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  • Black Hole Collision With An Unexplained Massive Object

    11:08

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  • Black Holes Explained – From Birth to Death

    5:56

    Black holes. Lets talk about them.


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  • Black Holes Explained | Cinematic Short Space Documentary

    8:15

    Part of the Universe Project. A seven episode mini series about the universe.
    This video is purely for entertainment purposes.
    All video, photo and music licenses are available.

    Please enjoy the episode about black holes. Maybe one of the biggest mysteries in our known universe. A part of space that bends time & space. But also the minds of the smartest scientists. Its a short space documentary. Maybe this helps you learn more about how the universe works.

    Also we discuss the event horizon. Can you believe the mass of black holes?

    In the next episode we discuss our moon nasa visited in 1969. The question is: why do have a moon?

    cosmology and astrophysics

  • What Actually Happens When You Drop Something into a Real Black Hole?

    14:32

    Get your Action Lab Box Now!

    In this video I show you what it actually looks like to drop different things into a black hole! I talk about gravitational lensing, gravitational time dilation and gravitational red shifting. All of this to show you what it would actually look like to watch something fall into a black hole.

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    For more awesome videos checkout:What Happens If You Fly a Drone In An Elevator? Real Experiment!


    The New World's Blackest Paint (Black 3.0) vs the Brightest Flashlight!


    What Happens if You Focus a 5W Laser With a Giant Magnifying Glass? Negative Kelvin Temperature!


    Darker Than Vantablack—Absorbs 99.9923% of Light


    Amazing experiment actually makes black fire


    What Does a 4D Ball Look Like in Real Life? Amazing Experiment Shows Spherical Version of Tesseract


    How I Made an Ant Think It Was Dead—The Zombie Ant Experiment


    Can Light be Black? Mind-Blowing Dark Light Experiments!


    Mirror-Polished Japanese Foil Ball Challenge Crushed in a Hydraulic Press-What's Inside?


    Mixing the World's Blackest Paint With the World's Brightest Paint (Black 2.0 vs LIT)


    What if You Try To Lift a Negative Mass? Mind-Blowing Physical Impossibility!


    What Does a Giant Monster Neodymium Magnet do to a Mouse?


    The Worlds Blackest Black vs The Worlds Brightest Flashlight (32,000 lumen)—Which Will Win?


    How Much Weight Can a Fly Actually Lift? Experiment—I Lassoed a Fly!


    DISCLAIMER: Any experiment you try is at your own risk

  • Soundgarden - Black Hole Sun

    5:21

    REMASTERED IN HD!

    Music video by Soundgarden performing Black Hole Sun. (C) 1994 A&M Records

    #Soundgarden #BlackHoleSun #Remastered #Vevo

  • National Geographic Documentary 2015 Monster Black Holes Full Documentary 2015 HD

    46:50

  • Physicist Brian Cox Explains Black Holes in Plain English | Joe Rogan

    5:39

    Taken from Joe Rogan Experience #1233 w/Brian Cox:

  • The Death of a Black Hole | space and astronomy

    10:04

    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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  • What If a Black Hole Opened at CERN?

    5:04

    Let's roll back a few days. This is CERN, the Nuclear Research laboratory on the border of France and Switzerland. It features the most powerful particle accelerator on Earth, the Large Hadron Collider, or LHC. What does it do? It accelerates and collides particles at 99.99% of the speed of light. And maybe, it could produce the very first lab-grown black hole. How big would that black hole be? What precautions would you need to take not to get sucked in it? And how long would it take it to destroy the entire planet?

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  • Fascination Black Holes Pt. 1 | Special Episode

    10:41

    Black holes are the universe at its most extreme: matter and energy crunched so small they literally exit the known universe. Scientists are beginning to suspect that these monsters have a powerful impact on galaxies, solar systems and space-time itself. And now, researchers are finally getting a grip on these black holes with a new generation of high-tech laser systems and advanced telescopes in space.
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  • What If All Black Holes in the Universe Collided?

    10:39

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    Subscribe to Ridddle channel. We will make this universe smarter together!
    Okay, okay. I got to go..... See You Soooooooooooooooon dudes ;)

  • Monster Black Holes - New BBC Documentary 2015 HD

    42:08

    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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  • Supermassive Black Hole Documentary - Part 2

    5:18

    What are Supermassive Black Holes? This is part 2 of the black hole documentary series. In this part, we will explore supermassive black holes and even ultra massive black holes. Subscribe and ring the bell to be notified about similar videos.

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  • National Geographic 2014 Monster Black Holes Full Documentary HD

    1:54:51

    National Geographic 2014 Monster Black Holes Full Documentary HD

  • Unlocking the Secrets of Cosmos Super Massive Black Holes - Full Documentary

    54:20

    Unlocking the Secrets of Cosmos Super Massive Black Holes
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    43:54

    Monster black hole - How the universe works in hindi

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