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TIMELAPSE OF THE FUTURE: A Journey to the End of Time (4K)

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    Supported By:
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    Supported By:
    Protocol Labs
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    Protocol Labs
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    Protocol Labs
    What does our future hold?
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    Everything has its wonders, even darkness and silence...
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    Everything has its wonders, even darkness and silence...
    - Helen Keller
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    What does the future look like?
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    How will the universe meet its end?
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    We may never be truly certain.
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    But science has begun to paint a stunning picture of how the future might unfold.
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    Let's take a journey to the end of time.
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    We will travel through time exponentially, doubling our speed every 5 seconds.
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    The vision of the future will surely evolve
    as we probe for more clues. But one thing is clear:
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    The universe has only just begun.
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    2019
    [Anthrpocene era]
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    2020
    [Anthrpocene era]
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    2021
    [Anthrpocene era]
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    2021
    The Holocene has ended.
    [Anthrpocene era]
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    2021
    The Holocene has ended.
    [Anthrpocene era]
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    2022
    The Holocene has ended.
    [Anthrpocene era]
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    2023
    The Holocene has ended.
    [Anthrpocene era]
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    2023
    [Anthrpocene era]
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    What we do now,
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    What we do now,
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    What we do now,
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    What we do now,
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    and in the next few years,
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    will profoundly affect
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    the next few thousand years.
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    The only conditions modern humans
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    have ever known so far, are changing.
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    And changing fast.
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    Nothing stays the same on this planet.
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    Everything changes.
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    The Earth is going into one of these jumps
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    The Earth is going into one of these jumps
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    and you don't know what is going
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    to be on the other side of those jumps.
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    The Earth is always jumping.
    [Earth's magnetic field flips]
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    [Earth's magnetic field flips]
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    [Comet Hale-Bopp returns]
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    [Drastic sea level rise]
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    Things move on this planet
    [Drastic sea level rise]
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    Things are not still!
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    Everything is turning.
    [30 meter asteroid impact]
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    [30 meter asteroid impact]
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    [Antares goes supernova]
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    [Sahara becomes tropical]
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    [Constellations begin to wander]
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    [Voyager I passes nearby star]
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    [Interglacial period ends]
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    [Supervolcano eruption]
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    [New Hawaiian island appears]
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    [New island chains]
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    [Apollo footprints fade]
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    [Betelgeuse goes supernova]
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    [Stone monuments erode]
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    [Deadly gamma ray burst]
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    [Mars moon becomes a ring]
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    [Saturn's rings vanish]
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    [Antarctica melts]
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    [Major asteroid impact]
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    [New supercontinent]
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    [Sun increases luminosity]
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    As it begins to run out of fuel,
    [Sun increases luminosity]
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    As it begins to run out of fuel,
    [Photosynthesis ceases]
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    the sun won't simply fade away to nothing.
    [Photosynthesis ceases]
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    the sun won't simply fade away to nothing.
    [All plant life dies]
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    [All plant life dies]
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    [Oceans evaporate]
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    Its core will collapse,
    [Oceans evaporate]
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    [Oceans evaporate]
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    and the extra heat this generates
    [Oceans evaporate]
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    will cause its outer layers to expand.
    [Oceans evaporate]
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    will cause its outer layers to expand.
    [All life dies]
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    [All life dies]
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    [Sun expands]
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    [Sun becomes red giant]
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    [Earth destroyed by the dying Sun]
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    [Sun becomes a White Dwarf]
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    The sun is now dead.
    [Sun becomes a White Dwarf]
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    Its remains slowly cooling
    [Sun becomes a White Dwarf]
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    in the freezing temperatures of deep space.
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    The fate of the sun is the same as for all stars.
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    One day, they must all eventually die,
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    and the cosmos will be plunged
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    into eternal night.
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    All stars eventually will run out of fuel.
    [Stars begin to die off]
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    [Stars begin to die off]
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    The temperature of the universe drops.
    [Stars begin to die off]
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    [Stars begin to die off]
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    Stars, one by one,
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    in the night sky,
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    will turn off.
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    And there will be no more new stars
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    created.
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    And so the universe will end
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    not with a bang,
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    but with the whimper.
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    And not in fire,
    [Last Red Dwarf stars die]
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    [Last Red Dwarf stars die]
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    but in ice.
    [Last Red Dwarf stars die]
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    [Last Red Dwarf stars die]
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    [Degenerate era]
    "With the death of the last sun, the age of starlight comes to an end."
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    [Degenerate era]
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    [Degenerate era]
    "The universe becomes a cosmic boneyard, strewn with remnants of dead stars."
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    "The universe becomes a cosmic boneyard, strewn with remnants of dead stars."
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    "Our Sun becomes a White Dwarf - a hot, dense, shrunken stellar corpse."
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    With no fuel left to burn,
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    a white dwarf's faint glow
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    comes from the last residual heat
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    from its extinguished furnace.
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    Looking at it from where the earth is now,
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    it would only generate the same amount of light
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    as the full moon
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    on a clear night.
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    The faint glow of white dwarfs
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    will provide the only illumination
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    in a dark and empty void
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    littered with dead stars
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    and black holes.
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    In some ways it's kind of a ghost universe
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    it's the corpses,
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    the zombie stars,
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    that will take us into the future.
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    "Over time, gravity ejects dead stars and planets from their galaxies, sending them out into the freezing void."
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    "By chance, some Brown Dwarfs collide and form accidental new stars."
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    "Colliding neutron stars puncture the darkness with ultra bright supernova."
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    [Neutron star collision]
    Colliding neutron stars puncture the darkness with ultra bright supernova."
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    [Neutron star collision]
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    "Any surviving life forms may find refuge around aging White Dwarfs."
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    "But in time, even the White Dwarfs will fade and die."
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    A black dwarf will be the final fate of those last stars
    [Stars become Black Dwarfs]
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    White dwarfs that have become so cold,
    [Stars become Black Dwarfs]
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    that they barely emit any more heat or light.
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    Black dwarfs are dark,
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    dense,
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    decaying balls of degenerate matter.
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    Little more than the ashes of stars,
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    their constituent atoms are so severely crushed
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    that black dwarfs are a million times
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    denser than our sun.
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    Stars take so long to reach this point
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    we believe there are currently
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    no black dwarfs in the universe.
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    "Any matter that fails to escape its galaxy
    is sucked into a supermassive black hole at the center."
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    [Black holes swallow stray matter]
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    [Black holes swallow stray matter]
    "Long dormant black holes flare up in a blaze of glory."
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    [Degenerate era]
    "The rotational energy of black holes becomes the last reliable source of power for any exotic future civilizations."
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    We have a pace of life that's based
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    on the energy available to us now.
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    You could imagine living,
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    conscious systems,
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    which have a very different pace and therefore,
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    can extend out, at least,
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    a lot farther than you'd imagine otherwise.
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    You could have a living system where if,
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    it had a thought every 10 trillion years,
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    that would seem normal.
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    Ever if
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    our life dies out, one could imagine
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    at some time arbitrarily far in the future,
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    a fluctuation occurs which allows intelligent life
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    to exist again, for a little while.
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    So you might have islands in time of intelligence.
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    "As the expansion of the universe accelerates, it
    begins to spread matter apart faster than the speed of light."
    [Expansion of spacetime]
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    [Expansion of spacetime]
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    "By this point, distant galaxies and stars are receding do fast that their light has become undetectable."
    [Expansion of spacetime]
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    "By this point, distant galaxies and stars are receding do fast that their light has become undetectable."
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    "The secrets of the cosmos are locked away forever."
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    "Current theories predict that atoms themselves will begin to decay, destroying all remaining matter in the universe."
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    [Proton decay]
    "Current theories predict that atoms themselves will begin to decay, destroying all remaining matter in the universe."
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    [Proton decay]
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    A proton, one of the fundamental building blocks
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    of atomic matter, what makes us up,
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    can just spontaneously fall apart.
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    Any material that evades the pull of a black hole
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    eventually dies away as its protons disintegrate.
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    "Proton decay is still unproven - and so this chapter of the future could look very different in light of new discoveries."
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    The matter inside black dwarf's,
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    the last matter in the universe,
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    will eventually evaporate away,
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    and be carried off into the void as radiation
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    leaving absolutely nothing behind.
  • 11:35 - 11:42
    [Black hole era]
  • 11:42 - 11:45
    With the black dwarfs gone,
    [Black hole era]
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    there won't be a single atom of matter left.
    [Black hole era]
  • 11:48 - 11:48
    [Black hole era]
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    All that will remain of our once-rich cosmos
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    will be particles of light and black holes.
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    "The Black Hole Era begins."
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    "No planets, no stars, no lingering stellar remnants for life to cling to."
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    "Yet even now, time has only begun to tick."
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    "On the scale of a human lifetime, the universe has just emerged from the womb."
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    "Cold, dark, and empty - this is how the cosmos will spend most of its life."
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    "Our universe gives life only a brief moment to shine - a haven in time, safe from its fiery birth and icy death."
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    The arrow of time creates a bright window
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    in the universe's adolescence
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    during which life is possible.
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    But it's a window that doesn't stay open for long.
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    As a fraction of the lifespan of the universe,
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    as measured from its beginning
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    to the evaporation of the last black hole,
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    life,
  • 13:25 - 13:26
    life, as we know it,
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    life, as we know it, is only possible for
  • 13:27 - 13:28
    one
    (10^(0))
  • 13:28 - 13:29
    one thousandth
    (10^(-3))
  • 13:29 - 13:29
    one thousandth of a
    (10^(-3))
  • 13:29 - 13:30
    one thousandth of a billion
    (10^(-12))
  • 13:30 - 13:30
    one thousandth of a billion billion
    (10^(-21))
  • 13:30 - 13:31
    one thousandth of a billion billion billionth
    (10^(-30))
  • 13:31 - 13:31
    one thousandth of a billion billion billionth,
    billion
    (10^(-39))
  • 13:31 - 13:32
    one thousandth of a billion billion billionth,
    billion billion
    (10^(-48))
  • 13:32 - 13:32
    one thousandth of a billion billion billionth,
    billion billion billionth
    (10^(-57))
  • 13:32 - 13:33
    one thousandth of a billion billion billionth,
    billion billion billionth billion
    (10^(-66))
  • 13:33 - 13:34
    one thousandth of a billion billion billionth,
    billion billion billionth billion billion
    (10^(-75))
  • 13:34 - 13:35
    one thousandth of a billion billion billionth,
    billion billion billion billion billion billionth,
    (10^(-84))
  • 13:35 - 13:36
    one thousandth of a billion billion billionth,
    billion billion billion billion billion billionth, of a percent.
    (10^(-84)%)
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    Black holes become
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    the fundamental building block of the universe.
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    A galaxy will basically be
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    a supermassive black hole in the center,
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    with smaller black holes orbiting it.
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    Zombie galaxies filled with black holes continue to evolve.
  • 14:10 - 14:12
    They'll eat each other, and they'll get bigger,
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    and maybe they'll fall into
  • 14:13 - 14:15
    the supermassive black hole and it'll get bigger.
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    The universe will still be an exciting, dynamic place.
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    it's just that the time scales we're talking about
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    are now trillions of years,
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    instead of thousands or millions of years.
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    [Black home mergers]
    "In this far flung age, black hole mergers become the main event."
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    "Some grow to enormous sizes, possibly trillions of times the mass of our sun."
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    "When they merge, they send out powerful gravity waves that resonate throughout the universe."
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    Black holes can bang on space-time like mallets on a drum.
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    And have a very characteristic song,
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    Imagine two black holes that have lived a long life together
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    At the end of their lives they're going around each other,
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    crossing thousands of kilometers in a fraction of a second.
  • 15:32 - 15:33
    As they do so,
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    they leave behind in their wake a ringing of space
  • 15:37 - 15:39
    an actual wave on space-time.
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    Space squeezes and stretches as it emanates out
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    from these black holes banging on the universe.
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    Those are the gravitational waves
  • 16:05 - 16:08
    and are literally the sounds of space ringing
  • 16:08 - 16:09
    and they will travel out from these black holes
  • 16:09 - 16:14
    at the speed of light as they ring down and coalesce into one,
  • 16:14 - 16:16
    spinning, quiet, black hole.
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    If you were standing near enough,
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    your ear would resonate
  • 16:25 - 16:28
    with the squeezing and stretching of space,
  • 16:28 - 16:30
    you would literally hear the sound.
  • 16:39 - 16:41
    Imagine a lighter black hole
  • 16:41 - 16:43
    falling into a very heavy black hole.
  • 16:43 - 16:45
    The sound you're hearing
  • 16:45 - 16:47
    is a light black hole banging
  • 16:47 - 16:50
    on space each time it gets close.
  • 16:58 - 17:01
    As it falls in, it gets faster, and it gets louder.
  • 17:23 - 17:26
    Scientists used to think black holes were immortal,
  • 17:26 - 17:28
    but even these will one day die.
  • 17:29 - 17:33
    Now we're talking about time scales of unimaginable length
  • 17:33 - 17:35
    quadrillions of years into the future.
  • 17:36 - 17:37
    On that time scale,
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    even the black holes begin to evaporate.
  • 17:44 - 17:47
    [Hawking radiation]
  • 17:47 - 17:50
    [Hawking radiation]
  • 17:50 - 17:52
    [Hawking radiation]
  • 17:52 - 17:52
    [Hawking radiation]
    According to quantum mechanics,
  • 17:52 - 17:53
    According to quantum mechanics,
  • 17:53 - 17:54
    [Hawking radiation]
    According to quantum mechanics,
  • 17:54 - 17:55
    space is filled with virtual particles
  • 17:55 - 17:57
    [Hawking radiation]
    space is filled with virtual particles
  • 17:57 - 17:57
    space is filled with virtual particles
  • 17:57 - 18:00
    [Hawking radiation]
    and antiparticles that are constantly materializing in pairs,
  • 18:00 - 18:01
    and antiparticles that are constantly materializing in pairs,
  • 18:01 - 18:03
    [Hawking radiation]
    and antiparticles that are constantly materializing in pairs,
  • 18:03 - 18:03
    [Hawking radiation]
    separating, coming together again,
  • 18:03 - 18:05
    separating, coming together again,
  • 18:05 - 18:06
    [Hawking radiation]
    separating, coming together again,
  • 18:06 - 18:07
    [Hawking radiation]
    and annihilating each other.
  • 18:07 - 18:07
    and annihilating each other.
  • 18:07 - 18:08
    [Hawking radiation]
    and annihilating each other.
  • 18:10 - 18:11
    [Hawking radiation]
  • 18:13 - 18:16
    [Hawking radiation]
    In the presence of a black hole,
  • 18:16 - 18:17
    one member of a pair of
  • 18:17 - 18:17
    [Hawking radiation]
    one member of a pair of
  • 18:17 - 18:19
    [Hawking radiation]
    virtual particles may fall into the hole,
  • 18:19 - 18:20
    virtual particles may fall into the hole,
  • 18:20 - 18:20
    [Hawking radiation]
    virtual particles may fall into the hole,
  • 18:20 - 18:20
    virtual particles may fall into the hole,
  • 18:21 - 18:22
    leaving the other member
  • 18:22 - 18:24
    without a partner with which to annihilate.
  • 18:24 - 18:24
    [Hawking radiation]
    without a partner with which to annihilate.
  • 18:24 - 18:25
    without a partner with which to annihilate.
  • 18:27 - 18:28
    [Hawking radiation]
    The forsaken particle appears to be radiation
  • 18:28 - 18:30
    The forsaken particle appears to be radiation
  • 18:30 - 18:31
    [Hawking radiation]
    The forsaken particle appears to be radiation
  • 18:31 - 18:31
    The forsaken particle appears to be radiation
  • 18:31 - 18:33
    emitted by the black hole.
  • 18:33 - 18:34
    [Hawking radiation]
    emitted by the black hole.
  • 18:34 - 18:35
    [Hawking radiation]
  • 18:35 - 18:36
    [Hawking radiation]
  • 18:37 - 18:37
    And so, black holes are not eternal.
  • 18:37 - 18:41
    And so, black holes are not eternal.
    [Black hole evaporation]
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    They evaporate away at an increasing rate,
  • 18:47 - 18:52
    until they vanish in a gigantic explosion.
  • 18:58 - 19:02
    Quantum mechanics has allowed particles and radiation
    [Black holes begin to die]
  • 19:02 - 19:05
    to escape from the ultimate prison -
  • 19:05 - 19:06
    A black hole.
  • 19:07 - 19:13
    "Black holes begin to evaporate away, erasing the last large-scale structures in the universe."
  • 19:15 - 19:19
    "As they die, they light up the darkness one by one."
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    "As the black holes slowly die off, the universe continues to expand, driven by a mysterious force we don't yet understand."
  • 20:00 - 20:09
    [Dark Energy inflates the universe]
    "As the black holes slowly die off, the universe continues to expand, driven by a mysterious force we don't yet understand."
  • 20:12 - 20:18
    "This is the frontier of human knowledge - a frontier ripe for exploration and discovery."
  • 20:18 - 20:20
    Philosophers and poets have asked the question,
  • 20:20 - 20:22
    "Will the world end in fire or ice?"
  • 20:23 - 20:26
    We can now give an answer.
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    The latest evidence shows that the universe
  • 20:31 - 20:32
    is not slowing down,
  • 20:32 - 20:34
    but it's speeding up out of control.
  • 20:35 - 20:38
    And the universe, we think, will die in ice
  • 20:39 - 20:42
    trillions upon trillions of years from now.
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    Empty space itself has energy.
  • 20:48 - 20:50
    In every little cubic centimeter of space,
  • 20:50 - 20:52
    whether or not there's stuff,
  • 20:52 - 20:53
    whether or not there's particles,
  • 20:53 - 20:54
    matter, radiation, whatever...
  • 20:54 - 20:57
    there is still energy, even in the space itself.
  • 21:00 - 21:02
    And this energy, according to Einstein,
  • 21:02 - 21:05
    exerts a push on the universe.
  • 21:07 - 21:10
    What is the weird stuff that's accelerating the universe?
  • 21:10 - 21:12
    We call it 'Dark energy'.
  • 21:15 - 21:18
    And this stuff is the dominant stuff of the universe
  • 21:18 - 21:21
    almost 3/4 of the matter-energy content
  • 21:21 - 21:23
    of the universe is this dark energy
  • 21:24 - 21:26
    and we don't know what it is.
  • 21:30 - 21:32
    Dark energy, unlike matter or radiation,
  • 21:32 - 21:35
    does not dilute away, as the universe expands.
  • 21:37 - 21:39
    This has crucial implications
  • 21:39 - 21:42
    for what the universe is going to do in the future.
  • 21:43 - 21:45
    So, what will be the future of the universe?
  • 21:48 - 21:51
    Well, if the dark energy remains dominant and repulsive,
  • 21:52 - 21:55
    the universe will expand forever.
  • 22:01 - 22:04
    Faster and faster and faster with time -
  • 22:04 - 22:06
    A runaway universe.
  • 22:08 - 22:11
    70% of the energy of the universe
  • 22:11 - 22:16
    resides in empty space and we don't understand why.
  • 22:18 - 22:20
    But we do know what will happen.
  • 22:21 - 22:24
    If that energy continues to be there,
  • 22:24 - 22:27
    the universe will become cold and dark and empty.
  • 22:30 - 22:32
    That's the future as it might be.
  • 22:33 - 22:34
    We don't know because
  • 22:35 - 22:37
    we don't yet understand the nature of dark energy.
  • 22:37 - 22:38
    until we do,
  • 22:38 - 22:40
    we won't know the future,
  • 22:40 - 22:42
    we won't even understand our own origins
  • 22:42 - 22:43
    and that's why we want to know
  • 22:43 - 22:45
    and study this subject.
  • 22:47 - 22:54
    "Discovering the true nature of dark energy could change our vision of the future dramatically."
  • 22:56 - 23:03
    "If it somehow weakens over time, the universe could collapse under gravity - a 'big crunch'."
  • 23:04 - 23:10
    "Given a boost, it could tear the universe apart at the seams - a 'big rip'."
  • 23:12 - 23:22
    [Black hole era]
    "Physicists increasingly suspect that there may be multiple universes beyond our own, each with their own unique laws of physics."
  • 23:25 - 23:34
    "Some would harbor the right conditions for life. Others could collapse or be ripped apart."
  • 23:35 - 23:42
    "Others sill could be far more exotic than anything we could imagine."
  • 23:46 - 23:52
    "New pieces to this puzzle are out there somewhere, waiting to be found."
  • 23:53 - 23:54
    The forecast does seem to be for
  • 23:54 - 23:58
    an ever-colder, ever-emptier universe.
  • 24:03 - 24:05
    But then of course we have to ask,
  • 24:05 - 24:08
    "Could that end lead to a new beginning?"
  • 24:10 - 24:13
    And there are ideas, whereby what actually is the end
  • 24:13 - 24:15
    of our universe, could in some sense,
  • 24:15 - 24:17
    lead to the beginning of a new one.
  • 24:23 - 24:30
    "Some speculate that there may be a way to escape our universe before entropy erases everything."
  • 24:32 - 24:38
    "We could create simulated virtual universes, or with enough energy, create another one just like our own."
  • 24:44 - 24:45
    We've worked out the mathematics,
  • 24:45 - 24:46
    the equations,
  • 24:46 - 24:47
    they seem to say that
  • 24:47 - 24:49
    if you have an atom smasher,
  • 24:49 - 24:51
    that can constrict tremendous
  • 24:51 - 24:53
    amounts of energy at a single point,
  • 24:53 - 24:56
    you can perhaps open up a gateway -
  • 24:56 - 24:57
    A 'Baby universe'
  • 25:03 - 25:06
    Facing the death of everything there is
  • 25:06 - 25:10
    this perhaps is their only possibility of escape.
  • 25:12 - 25:15
    And this also raises a very intriguing possibility,
  • 25:15 - 25:17
    sheer pure speculation of course,
  • 25:17 - 25:21
    that perhaps any universe that has intelligent life in it,
  • 25:21 - 25:24
    will create baby universes, will create 'Lifeboats',
  • 25:24 - 25:26
    and will proliferate child universes.
  • 25:26 - 25:28
    and will proliferate child universes.
    [Last Black Hole evaporates]
  • 25:28 - 25:30
    [Last Black Hole evaporates]
  • 25:30 - 25:34
    So an evolution may take place among universes,
    [Last Black Hole evaporates]
  • 25:34 - 25:35
    in the multiverse.
    [Last Black Hole evaporates]
  • 25:35 - 25:39
    Survival of the fittest may take place.
  • 25:39 - 25:42
    So those universes which do not have intelligent life are 'Infertile',
  • 25:42 - 25:43
    they have no children.
  • 25:44 - 25:45
    But those universes that have
  • 25:45 - 25:48
    mild temperatures, stars like ours,
  • 25:48 - 25:51
    would create civilizations that could open up child universes
  • 25:51 - 25:54
    and they would then proliferate.
  • 25:59 - 26:06
    "If there is no way to escape the universe, then entropy will march on, destroying the last remaining supermassive black holes."
  • 26:09 - 26:13
    "As the last one explodes and dies, it bathes the universe in light one last time."
  • 26:13 - 26:16
    [Black Hole era]
    "As the last one explodes and dies, it bathes the universe in light one last time."
  • 26:16 - 26:17
    [Last Black Hole evaporates]
    "As the last one explodes and dies, it bathes the universe in light one last time."
  • 27:11 - 27:12
    THE END.
  • 27:24 - 27:28
    After an unimaginable length of time,
  • 27:28 - 27:31
    even the black holes will have evaporated,
  • 27:31 - 27:33
    and the universe will be
  • 27:33 - 27:36
    nothing but a sea of photons
  • 27:36 - 27:39
    gradually tending towards the same temperature
  • 27:39 - 27:42
    as the expansion of the universe cools them
  • 27:42 - 27:43
    towards absolute zero.
  • 27:57 - 27:59
    Once the very last remnants
  • 27:59 - 28:01
    of the very last stars
  • 28:01 - 28:04
    have finally decayed away to nothing,
  • 28:04 - 28:07
    and everything reaches the same temperature,
  • 28:07 - 28:11
    the story of the universe finally comes to an end.
  • 28:12 - 28:15
    "TIME BECOMES MEANINGLESS"
  • 28:15 - 28:17
    For the first time in its life,
    "TIME BECOMES MEANINGLESS"
  • 28:17 - 28:21
    the universe will be permanent and unchanging.
    "TIME BECOMES MEANINGLESS"
  • 28:21 - 28:21
    "TIME BECOMES MEANINGLESS"
  • 28:21 - 28:24
    Entropy finally stops increasing,
    "TIME BECOMES MEANINGLESS"
  • 28:24 - 28:28
    because the cosmos cannot get any more disordered.
    "TIME BECOMES MEANINGLESS"
  • 28:28 - 28:29
    "TIME BECOMES MEANINGLESS"
  • 28:29 - 28:29
    Nothing happens,
    "TIME BECOMES MEANINGLESS"
  • 28:29 - 28:29
    Nothing happens,
    "TIME BECOMES MEANINGLESS
  • 28:29 - 28:29
    Nothing happens,
    "TIME BECOMES MEANINGLESS,
  • 28:29 - 28:29
    Nothing happens,
    "TIME BECOMES MEANINGLESS,
  • 28:29 - 28:29
    Nothing happens,
    "TIME BECOMES MEANINGLESS, F
  • 28:29 - 28:29
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FO
  • 28:29 - 28:30
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FOR
  • 28:30 - 28:30
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FORE
  • 28:30 - 28:30
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FOREV
  • 28:30 - 28:30
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FOREVE
  • 28:30 - 28:30
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FOREVER
  • 28:30 - 28:30
    Nothing happens,
    "TIME BECOMES MEANINGLESS, FOREVER.
  • 28:30 - 28:32
    and it keeps not happening,
    "TIME BECOMES MEANINGLESS, FOREVER.
  • 28:32 - 28:33
    "TIME BECOMES MEANINGLESS, FOREVER.
  • 28:33 - 28:34
    "TIME BECOMES MEANINGLESS, FOREVER."
  • 28:34 - 28:35
    "TIME BECOMES MEANINGLESS, FOREVER."
  • 28:37 - 28:45
    "Everything has its wonders, even darkness and silence...
    ...and I learn, whatever state I may be in, therein to be content."
    - Helen Keller
  • 28:48 - 28:52
    CRAFTED BY MELODYSHEEP
  • 28:53 - 28:54
    Supported by:
  • 28:54 - 28:56
    Supported by:
    Protocol Labs
  • 28:56 - 28:56
    Protocol Labs
  • 28:56 - 28:57
    Protocol Labs
    What will you discover?
  • 28:57 - 28:59
    Protocol Labs
    What will you discover?
    How will you change the future?
  • 28:59 - 28:59
    What will you discover?
    How will you change the future?
  • 29:00 - 29:01
    Featuring the voices of:
  • 29:01 - 29:01
    Featuring the voices of:
    David Attenborough
  • 29:01 - 29:01
    Featuring the voices of:
    Craig Childs
  • 29:01 - 29:01
    Featuring the voices of:
    Brian Cox
  • 29:01 - 29:02
    Featuring the voices of:
    Neil Degrasse Tyson
  • 29:02 - 29:02
    Featuring the voices of:
    Michelle Thaller
  • 29:02 - 29:02
    Featuring the voices of:
    Lawrence Krauss
  • 29:02 - 29:02
    Featuring the voices of:
    Michio Kaku
  • 29:02 - 29:03
    Featuring the voices of:
    Mike Rowe
  • 29:03 - 29:03
    Featuring the voices of:
    Phil Plait
  • 29:03 - 29:03
    Featuring the voices of:
    Janna Levin
  • 29:03 - 29:03
    Featuring the voices of:
    Stephen Hawking
  • 29:03 - 29:04
    Featuring the voices of:
    Sean Carroll
  • 29:04 - 29:04
    Featuring the voices of:
    Alex Filippenko
  • 29:04 - 29:05
    Featuring the voices of:
    Martin Rees
  • 29:06 - 29:10
    Thanks to:
    Juan Benet & my supporters on Patreon
    Patreon.com/melodysheep
  • 29:11 - 29:14
    MELODYSHEEP.COM | @MUSICALSCIENCE
  • 29:15 - 29:16
    For Ash
タイトル:
TIMELAPSE OF THE FUTURE: A Journey to the End of Time (4K)
概説:

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Video Language:
English
Duration:
29:21

English subtitles

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