Video Summary

How To Destroy The Universe

Kurzgesagt – In a Nutshell

Main takeaways
01

The universe’s fate hinges on the balance between matter (gravity) and dark energy (repulsive pressure).

02

If dark energy stays constant, accelerating expansion causes heat death: stars die, black holes evaporate, and the universe becomes cold and empty.

03

If dark energy strengthens, a Big Rip would progressively tear galaxies, stars, planets, atoms, and spacetime itself apart.

04

If dark energy weakens, gravity could reverse expansion and cause a Big Crunch, possibly collapsing to a singularity or bouncing into a new expansion.

Key moments
Questions answered

What two forces determine the long-term fate of the universe?

The competition between matter (whose gravity pulls things together) and dark energy (an intrinsic energy of empty space that pushes the universe apart) determines the fate of cosmic expansion.

What happens in the Heat Death scenario?

If dark energy remains constant, expansion accelerates, galaxies become isolated, stars burn out, black holes evaporate, and the universe approaches a cold, featureless state of maximum entropy—the Big Freeze.

How does the Big Rip destroy structures?

If dark energy grows stronger over time it overcomes all binding forces: galaxies, then star systems, then planets and even atoms are pulled apart, ending in the disintegration of spacetime itself.

What is the Big Crunch and how could it lead to a new universe?

If dark energy weakens and gravity dominates, the universe could reverse expansion and collapse. That collapse might end in a singularity or rebound (a 'bounce') that triggers a new expansion and a possible new universe.

The Cosmic Battle: Matter vs. Dark Energy 00:00

"Our universe was born 14 billion years ago in the Big Bang and has been expanding ever since."

  • The universe began with the Big Bang approximately 14 billion years ago and has been continuously expanding. This expansion creates new empty space between galaxies, raising the question of whether this expansion will persist indefinitely or cease at some point in the future.

  • The fate of the universe is governed by two cosmic forces: matter and dark energy. Matter includes everything that we can observe, such as galaxies, gas, and dark matter, all of which gravitate towards one another due to the force of gravity, which slows down the expansion of space.

"Empty space has an intrinsic energy."

  • In contrast to the pull of matter, empty space possesses a mysterious energy known as dark energy. This energy counteracts the gravitational attraction of matter, pushing galaxies apart and accelerating the universe's expansion.

  • The outcome of this cosmic struggle between matter and dark energy ultimately determines the fate of the universe.

Heat Death: The End of Activity 01:54

"If the strength of dark energy stays constant, it will win the war."

  • If dark energy remains stable over time, it will dominate the universe by pushing matter farther apart, leading to what is known as "Heat Death." This scenario anticipates a future where the universe expands at an accelerating rate, as empty space continues to generate more dark energy.

  • As a result, galaxies will become increasingly sparse, and eventually, all visible galaxies will vanish from sight, leaving our galaxy to drift alone in an ever-expanding isolated void.

"All gas that could create new stars has been consumed."

  • After trillions of years, our supergalaxy's stars will die out, leaving behind a dark cosmic wasteland filled with stellar remnants. Over quadrillions of years, even these remnants will cool and fade away, resulting in a universe that becomes featureless and dark.

  • Eventually, every structure will dissolve into single particles pushed further apart by dark energy, leading to an unimaginable state for the universe: a solitary particle drifting in an endless void, characterized by the "Big Freeze" or Heat Death.

The Big Rip: Dark Energy's Ascendant Strength 04:48

"If dark energy gets stronger, it will literally rip matter to pieces."

  • If dark energy intensifies over time, the result would lead to the "Big Rip," where the repulsive force of dark energy overcomes the gravitational attraction of matter. In this scenario, individual galaxies would start to drift apart, followed by stars and ultimately planets.

  • Life on any planet would come to an abrupt end, as dark energy creates voids within star systems, causing planets to become detached from their stars.

"Half an hour later, even atoms are destroyed."

  • In a staggering collapse of physical reality, dark energy would tear apart even the subatomic components of atoms, leading to a chaos of destruction where not even the remnants of black holes can survive.

  • This catastrophic event culminates in a complete obliteration of spacetime, creating a scenario where space and time lose their meanings altogether during the final moments of the universe.

The Big Crunch: Matter's Last Stand 07:00

"If the strength of dark energy decreases over time, the pull of gravity will win."

  • In a different scenario where dark energy diminishes, matter could prevail over gravitational pull, leading to the collapse of the universe in a phenomenon referred to as the "Big Crunch." While scientists remain uncertain about when this might occur, the universe could begin to contract in the coming hundreds of millions of years.

  • As galaxies draw closer, their collision would be gentle due to the predominance of empty space, resembling merging clouds rather than catastrophic collisions. However, the surrounding empty space would become densely packed with radiation, heating up the universe to unbearable levels.

"The universe could 'bounce back,' restarting the cosmic expansion."

  • Ultimately, the Big Crunch could end in two ways: the universe may collapse into a singularity, a state of infinite density, or rebound and give birth to a new universe, reinitiating the cycle.

  • However, despite these intriguing possibilities, there is currently no evidence to suggest that such a process has occurred in the past or that it will in the future, leaving the long-term fate of the universe in uncertainty.