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

Explore the future of the universe from the Anthropocene era to the death of stars in this 4K timelapse journey to the end of time.

Key Takeaways

  • The future of the universe is shaped by predictable cosmic and planetary events based on scientific understanding.
  • Earth is undergoing rapid changes that will have long-lasting effects on its environment and life.
  • Stars, including our sun, have finite lifespans and will eventually die, leading to a dark, cold universe.
  • White dwarfs and dead stars will be the last remnants illuminating the cosmos before complete darkness.
  • Human actions today have significant consequences for the near-term future of Earth.

What the video covers

  • The video explores the future of Earth and the universe through a scientific lens, starting from the Anthropocene era.
  • It highlights the rapid environmental changes and geological events shaping Earth's near future.
  • Key cosmic events such as asteroid impacts, supernovae, and planetary changes are depicted.
  • The sun's lifecycle is detailed, including its expansion into a red giant and eventual collapse into a white dwarf.
  • The video explains the gradual death of stars and the cooling of the universe over time.
  • It describes the degenerate era, where the universe becomes a cosmic boneyard of dead stars and black holes.
  • The illumination from white dwarfs is portrayed as the last light in a dark, empty cosmos.
  • The video emphasizes the exponential passage of time, doubling speed every five seconds to cover vast timescales.
  • It underscores humanity's impact on Earth and the profound effects of current actions on the planet's future.
  • The journey concludes with the universe ending not with a bang but a whimper, fading into eternal night and cold.

Answers

Questions about this video

What is the main theme of the video?

The video explores the scientific predictions of the future of Earth and the universe, illustrating cosmic and planetary changes from the present to the end of time.

How does the video represent the passage of time?

Time is represented exponentially, doubling in speed every five seconds, allowing the video to cover vast periods from the Anthropocene era to the far future.

What happens to the sun according to the video?

The sun will increase in luminosity, expand into a red giant, destroy Earth, and eventually collapse into a white dwarf, cooling over time and marking the end of its life cycle.

Full Transcript — Download SRT & Markdown

00:00
Speaker A
Supported by: Protocol Labs.
00:06
Speaker A
What does our future hold?
00:19
Speaker A
Everything has its wonders, even darkness and silence...
00:32
Speaker A
- Helen Keller
00:39
Speaker A
What does the future look like?
00:47
Speaker A
How will the universe meet its end? We may never be truly certain. But science has begun to paint a stunning picture of how the future might unfold.
00:52
Speaker A
Let's take a journey to the end of time. We will travel through time exponentially, doubling our speed every 5 seconds.
01:04
Speaker A
The vision of the future will surely evolve as we probe for more clues. But one thing is clear: The universe has only just begun.
01:13
Speaker A
2019 [Anthropocene era]
01:24
Speaker A
2020 [Anthropocene era]
01:37
Speaker A
2021 [Anthropocene era]
02:18
Speaker A
2021 The Holocene has ended. [Anthropocene era]
03:01
Speaker A
2021 The Holocene has ended. [Anthropocene era]
03:10
Speaker A
2022 The Holocene has ended. [Anthropocene era]
03:25
Speaker A
2023 The Holocene has ended. [Anthropocene era]
03:40
Speaker A
2023 [Anthropocene era]
03:54
Speaker A
What we do now, and in the next few years, will profoundly affect the next few thousand years.
04:04
Speaker A
The only conditions modern humans have ever known so far are changing. And changing fast.
04:21
Speaker A
Nothing stays the same on this planet. Everything changes. The Earth is going into one of these jumps,
04:38
Speaker A
and you don't know what is going to be on the other side of those jumps.
05:02
Speaker A
The Earth is always jumping.
05:16
Speaker A
[Earth's magnetic field flips]
05:29
Speaker A
[Earth's magnetic field flips]
05:50
Speaker A
[Comet Hale-Bopp returns]
06:07
Speaker A
[Drastic sea level rise]
06:33
Speaker A
Things move on this planet.
07:17
Speaker A
[Drastic sea level rise]
07:28
Speaker A
Things are not still!
07:55
Speaker A
Everything is turning.
08:11
Speaker A
[30 meter asteroid impact]
09:05
Speaker A
[30 meter asteroid impact]
09:10
Speaker A
[Antares goes supernova]
09:22
Speaker A
[Sahara becomes tropical]
09:31
Speaker A
[Constellations begin to wander]
09:44
Speaker A
[Voyager I passes nearby star]
10:07
Speaker A
[Interglacial period ends]
10:28
Speaker A
[Supervolcano eruption]
10:44
Speaker A
[New Hawaiian island appears]
10:58
Speaker A
[New island chains]
11:30
Speaker A
[Apollo footprints fade]
12:07
Speaker A
[Betelgeuse goes supernova]
12:36
Speaker A
[Stone monuments erode]
13:00
Speaker A
[Deadly gamma ray burst]
13:15
Speaker A
[Mars moon becomes a ring]
13:29
Speaker A
[Saturn's rings vanish]
13:32
Speaker A
[Antarctica melts]
13:35
Speaker A
[Major asteroid impact]
13:53
Speaker A
[New supercontinent]
14:02
Speaker A
[Sun increases luminosity]
14:15
Speaker A
As it begins to run out of fuel,
14:30
Speaker A
[Sun increases luminosity]
14:56
Speaker A
As it begins to run out of fuel,
15:32
Speaker A
[Photosynthesis ceases]
15:53
Speaker A
the sun won't simply fade away to nothing.
16:03
Speaker A
[Photosynthesis ceases]
16:21
Speaker A
the sun won't simply fade away to nothing.
16:39
Speaker A
[All plant life dies]
16:58
Speaker A
[All plant life dies]
17:29
Speaker A
[Oceans evaporate]
17:36
Speaker A
Its core will collapse,
17:57
Speaker A
[Oceans evaporate]
18:03
Speaker A
[Oceans evaporate]
18:07
Speaker A
and the extra heat this generates
18:19
Speaker A
[Oceans evaporate]
18:24
Speaker A
will cause its outer layers to expand.
18:27
Speaker A
[Oceans evaporate]
18:33
Speaker A
will cause its outer layers to expand.
18:37
Speaker A
[All life dies]
18:58
Speaker A
[All life dies]
19:07
Speaker A
[Sun expands]
20:00
Speaker A
[Sun becomes red giant]
20:18
Speaker A
[Earth destroyed by the dying Sun]
20:28
Speaker A
[Sun becomes a White Dwarf]
20:35
Speaker A
The sun is now dead.
20:45
Speaker A
[Sun becomes a White Dwarf]
20:54
Speaker A
Its remains slowly cooling
21:07
Speaker A
[Sun becomes a White Dwarf]
21:30
Speaker A
in the freezing temperatures of deep space.
21:43
Speaker A
The fate of the sun is the same as for all stars. One day, they must all eventually die, and the cosmos will be plunged into eternal night.
22:01
Speaker A
All stars eventually will run out of fuel.
22:18
Speaker A
[Stars begin to die off]
22:30
Speaker A
[Stars begin to die off]
22:37
Speaker A
The temperature of the universe drops.
22:47
Speaker A
[Stars begin to die off]
23:12
Speaker A
[Stars begin to die off]
23:46
Speaker A
Stars, one by one, in the night sky,
24:03
Speaker A
will turn off. And there will be no more new stars created.
24:23
Speaker A
And so the universe will end not with a bang, but with the whimper.
24:46
Speaker A
And not in fire,
25:06
Speaker A
[Last Red Dwarf stars die]
25:26
Speaker A
[Last Red Dwarf stars die]
25:39
Speaker A
but in ice.
25:44
Speaker A
[Last Red Dwarf stars die]
25:59
Speaker A
[Last Red Dwarf stars die]
26:16
Speaker A
[Degenerate era]
27:24
Speaker A
"With the death of the last sun, the age of starlight comes to an end."
27:57
Speaker A
[Degenerate era]
28:12
Speaker A
[Degenerate era]
28:28
Speaker A
"The universe becomes a cosmic boneyard, strewn with remnants of dead stars."
28:30
Speaker A
"The universe becomes a cosmic boneyard, strewn with remnants of dead stars."
28:30
Speaker A
"Our Sun becomes a White Dwarf - a hot, dense, shrunken stellar corpse."
28:48
Speaker A
With no fuel left to burn, a white dwarf's faint glow comes from the last residual heat from its extinguished furnace.
28:57
Speaker A
Looking at it from where the Earth is now, it would only generate the same amount of light as the full moon on a clear night.
29:00
Speaker A
The faint glow of white dwarfs will provide the only illumination in a dark and empty void littered with dead stars and black holes.
29:02
Speaker A
In some ways, it's kind of a ghost universe. It's the corpses, the zombie stars, that will take us into the future.
29:04
Speaker A
"Over time, gravity ejects dead stars and planets from their galaxies, sending them out into the freezing void."
Topics:future of the universeAnthropocene erasun lifecyclecosmic eventstimelapseend of timewhite dwarfstar deathEarth changescosmology

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