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

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### Description

Witness the mesmerizing journey through time with "TIMELAPSE OF THE FUTURE: A Journey to the End of Time (4K)." This stunning visual masterpiece takes you from the present day to the farthest reaches of the future, exploring the evolution of the universe. Experience breathtaking visuals, scientific insights, and mind-blowing predictions in crystal-clear 4K quality. Join us on this epic voyage and marvel at the wonders of time and space.

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Transcript
00:30The Holocene has ended.
00:52What we do now, and in the next few years, will profoundly affect the next few thousand
01:00years.
01:01The only conditions modern humans have ever known so far are changing, and changing fast.
01:13Nothing stays the same on this planet.
01:16Everything changes.
01:17The Earth is going into one of these jumps and you don't know what is going to be on
01:22the other side of those jumps.
01:23The Earth is always jumping.
01:24Things move on this planet.
01:25Things are not still.
01:26Everything is turning.
01:52Everything is changing.
01:53Everything is changing.
01:54Everything is changing.
01:55Everything is changing.
01:56Everything is changing.
01:57Everything is changing.
01:58Everything is changing.
01:59Everything is changing.
02:00Everything is changing.
02:01Everything is changing.
02:02Everything is changing.
02:03Everything is changing.
02:04Everything is changing.
02:05Everything is changing.
02:06Everything is changing.
02:07Everything is changing.
02:08Everything is changing.
02:09Everything is changing.
02:10Everything is changing.
02:11Everything is changing.
02:12Everything is changing.
02:13Everything is changing.
02:14Everything is changing.
02:15Everything is changing.
02:16Everything is changing.
02:17Everything is changing.
02:18Everything is changing.
02:19Everything is changing.
02:20Everything is changing.
02:21Everything is changing.
02:22Everything is changing.
02:23Everything is changing.
02:24Everything is changing.
02:25Everything is changing.
02:26Everything is changing.
02:27Everything is changing.
02:28Everything is changing.
02:29Everything is changing.
02:30Everything is changing.
02:31Everything is changing.
02:32Everything is changing.
02:33Everything is changing.
02:34Everything is changing.
02:35Everything is changing.
02:36Everything is changing.
02:37Everything is changing.
02:38Everything is changing.
02:39Everything is changing.
02:40Everything is changing.
02:41Everything is changing.
02:42Everything is changing.
02:43Everything is changing.
02:44Everything is changing.
02:45Everything is changing.
02:46Everything is changing.
02:47Everything is changing.
02:48Everything is changing.
02:49Everything is changing.
02:50Everything is changing.
02:59As it begins to run out of fuel,
03:02the sun won't simply fade away to nothing
03:07It's core will collapse
03:09and the extra heat it generates
03:11will cause it's outer layers to expand
03:14The sun is now dead. It's remained slowly cooling in the freezing temperatures of deep
03:29space. The fate of the sun is the same as for all stars. One day, they must all eventually
03:47die, and the cosmos will be plunged into eternal night. All stars eventually will run out of
03:57fuel. The temperature of the universe drops. The stars, one by one, in the night sky, will turn off.
04:05And there'll be no more new stars created. And so that the universe will end, not with a bang,
04:16but with a winter. And not in fire, but in ice.
04:27The sun is now dead. It's remained slowly cooling in the freezing temperatures of deep
04:41space. The fate of the sun is the same as for all stars. One day, they must all eventually
04:56die. With no fuel left to burn, a white dwarf's faint glow comes from the last residual heat
05:08from its extinguished furnace. Looking at it from where the earth is now, it would only
05:18generate the same amount of light as the full moon on a clear night. The faint glow of white
05:30dwarfs will provide the only illumination in a dark and empty void, littered with dead stars
05:38and black holes. In some ways, it's kind of a ghost universe. It's the corpses, the zombie stars,
05:55that will take us into the future.
07:08A black dwarf will be the final fate of those last stars. White dwarfs that have become so cold
07:19that they barely emit any more heat or light. Black dwarfs are dark, dense, decaying balls of
07:31degenerate matter. Little more than the ashes of stars. Their constituent atoms are so severely
07:41crushed that black dwarfs are a million times denser than our sun. Stars take so long to reach
07:56this point, we believe there are currently no black dwarfs in the universe.
08:56We have a pace of life that's based on really the energy available to us now. You could imagine
09:11living conscious systems which have a very different pace and therefore can extend out at
09:17least a lot farther than you'd imagine otherwise. You could have a living system where if it had a
09:24thought every 10 trillion years, that would seem normal. Even if our life dies out, one could
09:33imagine at some time arbitrarily far in the future, a fluctuation occurs which allows intelligent life
09:41to exist again for a little while. So you might have islands in time of intelligence.
10:12So
10:34a proton, one of the fundamental building blocks of atomic matter, what makes us up,
10:40can just spontaneously fall apart. Any material that evades the pull of a black hole
10:47eventually dies away as its protons disintegrate.
11:10So the matter inside black dwarfs, the last matter in the universe, will eventually evaporate away
11:26and be carried off into the void as radiation leaving absolutely nothing behind.
11:40With the black dwarfs gone, there won't be a single atom of matter left.
11:50All that will remain of our once rich cosmos will be particles of light and black holes.
12:40So
12:57the arrow of time creates a bright window in the universe's adolescence
13:02during which life is possible.
13:03But it's a window that doesn't stay open for long.
13:15As a fraction of the lifespan of the universe, as measured from its beginning to the evaporation
13:22of the last black hole, life as we know it is only possible for one thousandth of a billion billion
13:30billionth billion billion billion billion billion billionth of a percent.
13:45Black holes become the fundamental building block of the universe.
13:53A galaxy will basically be a supermassive black hole in the center with smaller black holes forming.
14:00Zombie galaxies filled with black holes continue to evolve.
14:10They'll eat each other and they'll get bigger and maybe they'll fall into the supermassive
14:13black hole and it'll get bigger. The universe will still be an exciting dynamic place. It's
14:18just that the time scales we're talking about are now trillions of years instead of
14:22thousands or millions of years.
14:30So
14:39so
14:56black holes can bang on space-time like mallets on a drum.
15:09And they have a very characteristic song.
15:18Imagine two black holes that have lived a long life together.
15:22At the end of their lives they're going around each other crossing thousands of kilometers in
15:26a fraction of a second. As they do so they leave behind in their wake a ringing of space, an actual
15:37wave on space-time.
15:53Space squeezes and stretches as it emanates out from these black holes banging on the universe.
16:03Those are the gravitational waves. They're literally the sounds of space ringing and
16:07they will travel out from these black holes at the speed of light as they ring down
16:12and coalesce to one spinning quiet black hole.
16:21If you were standing near enough your ear would resonate
16:25with the squeezing and stretching of space. You would literally hear the sound.
16:32So imagine a lighter black hole falling into a very heavy black hole. The sound you're hearing
16:45is a light black hole banging on space each time it gets close.
16:51So
16:58as it falls in it gets faster and it gets louder.
17:21Scientists used to think black holes were immortal but even these will one day die.
17:29Now we're talking about time scales of unimaginable length quadrillions of years
17:34into the future. On that time scale even the black holes begin to evaporate.
17:51According to quantum mechanics space is filled with virtual particles and antiparticles that are
17:59constantly materializing in pairs, separating, coming together again and annihilating each other.
18:13In the presence of a black hole one member of a pair of virtual particles may fall into the hole.
18:21Leaving the other member without a partner with which to annihilate.
18:27The forsaken particle appears to be radiation emitted by the black hole.
18:36And so black holes are not eternal.
18:41They evaporate away at an increasing rate until they vanish in a gigantic explosion.
18:57Quantum mechanics has allowed particles and radiation
19:02to escape from the ultimate prison, a black hole.
20:02So
20:17philosophers and poets have asked the question will the world end in fire or ice?
20:23We can now give an answer.
20:26The latest evidence shows that the universe is not slowing down but it's speeding up out of control
20:33and the universe we think will die in ice. Trillions upon trillions of years from now.
20:43Empty space itself has energy. In every little cubic centimeter of space
20:48whether or not there's stuff, whether or not there's particles, matter, radiation or whatever
20:52there is still energy even in the space itself.
21:00And this energy according to Einstein exerts a push on the universe.
21:07What is the weird stuff that's accelerating the universe? We call it dark energy.
21:14And this stuff is the dominant stuff of the universe. Almost three quarters of the matter
21:20energy content of the universe is this dark energy and we don't know what it is.
21:29Dark energy unlike matter or radiation does not dilute away as the universe expands.
21:36This has crucial implications for what the universe is going to do in the future.
21:43So what will be the future of the universe?
21:45Well, if the dark energy remains dominant and repulsive, the universe will expand forever.
21:59Faster and faster and faster with time. A runaway universe.
22:0670% of the energy of the universe resides in empty space and we don't understand it.
22:15Why? But we do know what will happen if that energy continues to be there.
22:24The universe will become cold and dark and empty.
22:30That's the future as it might be. We don't know because we don't yet understand the nature of
22:36dark energy. Until we do, we won't know the future. We won't even understand our own origins
22:41and that's why we want to know and study this subject.
23:42So
23:52the forecast does seem to be for an ever colder ever empty universe.
24:03But then of course we have to ask could that end lead to a new beginning?
24:08And there are ideas whereby what actually is the end of our universe could in some sense be linked
24:13to the beginning of a new one.
24:37So
24:43we've worked out the mathematics, the equations. They seem to say that if you have an atom smasher
24:48that can concentrate tremendous amounts of energy at a single point,
24:53you can perhaps open up a gateway, a baby universe.
24:57Facing the death of everything there is, this perhaps is their only possibility of escape.
25:06And this also raises a very intriguing possibility, sheer speculation of course,
25:11that perhaps any universe that has intelligent life in it will create baby universes,
25:17will create lifeboats and proliferate child universes.
25:21So an evolution may take among universes in the multiverse.
25:26Survival of the fittest may take place.
25:30So those universes which do not have intelligent life are infertile,
25:34they have no children. But those universes that have mild temperatures,
25:38stars like us, would create civilizations that could open up child universes.
25:42And they would then proliferate.
26:12So
26:42so
27:12so
27:24after an unimaginable length of time, even the black holes will have evaporated and the universe
27:32will be nothing but a sea of photons gradually tending towards the same temperature as the
27:39expansion of the universe cools them towards absolute zero.
27:57Once the very last remnants of the very last stars have finally decayed away to nothing,
28:03and everything reaches the same temperature, the story of the universe finally comes to an end.
28:15For the first time in its life, the universe will be permanent and unchanging.
28:21Entropy finally stops increasing because the cosmos cannot get any more disordered.
28:27Nothing happens and it keeps not happening forever.
28:57you

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