Scale & fate of the universe

Big Rip

Dark energy grows stronger until it pulls apart galaxies, then planets, then atoms themselves

Theoretical Artist's impression · drag to rotate
Proposed 2003 Robert Caldwell, Marc Kamionkowski and Nevin Weinberg [1]
Needs phantom energy dark energy with w < −1 [1]
Paper's example 22 billion years from now for w = −1.5 [1]
Milky Way torn apart 60 million years before the end [1]
Earth torn apart 30 minutes before the end [1]
Atoms torn apart 10⁻¹⁹ seconds before the end [1]
Measured w −1.028 ± 0.031 Planck; a rip, if any, at least 200 billion years away [2]

About the image. Drawn as a spiral galaxy whose stars are flying outward and fading as space between them stretches. It shows the idea of a Big Rip, not a real galaxy. Current measurements suggest a Big Rip is unlikely.

Since 1998 we have known that the expansion of the universe is speeding up. Whatever drives it is called dark energy. In the simplest picture its strength stays the same forever, and the universe slowly runs down into a cold heat death. But in 2003 three physicists asked what would happen if dark energy instead grew stronger over time. Their answer was the Big Rip.

Phantom energy

Physicists describe dark energy with a number called w. If w is exactly −1, dark energy is a cosmological constant: its density never changes. If w is less than −1, Robert Caldwell, Marc Kamionkowski and Nevin Weinberg showed in a paper titled “Phantom Energy and Cosmic Doomsday”, its density would increase as the universe expands, becoming infinite in a finite time. Expansion would then overpower every force that holds things together.

The countdown

The paper worked through an example with w = −1.5. In that universe the end comes 22 billion years from now, and the order of events follows the strength of what holds each thing together:

  • About a billion years before the end, clusters of galaxies come apart.
  • About 60 million years before, the Milky Way is torn apart, its stars flung away from each other.
  • About three months before, the planets come loose from the Sun.
  • About 30 minutes before, the Earth itself explodes.
  • About 10⁻¹⁹ seconds before, atoms are torn apart.

Then everything ends at once.

What the measurements say

The countdown depends entirely on w. The Planck satellite measured it as −1.028 ± 0.031, very close to −1. Even taking the most pessimistic end of the measurements, a Big Rip would be at least about 200 billion years away. Still, a Big Rip is very difficult to rule out completely, because a value of exactly −1 can never be measured with infinite precision.

Recent results point the other way. In 2025 the Dark Energy Spectroscopic Instrument (DESI), mapping millions of galaxies, found growing hints that dark energy is weakening, with w today greater than −1. The same analysis allows phantom behaviour in the distant past, but not now. If those hints hold up, the universe is heading away from a Big Rip, not towards it.

Gallery

A golden spiral galaxy whose outer stars stream away in loose, thinning arcs, an impression of a galaxy torn apart in a Big Rip. AI-generated painting.
Earth cracking apart, glowing lava in the gaps and broken chunks drifting away to the right, an impression of a planet torn apart in a Big Rip. AI-generated painting.
Big Rip, 3D artist's impression, rendered from the interactive model.
Big Rip, 3D artist's impression, from another angle, rendered from the interactive model.
Big Rip, 3D artist's impression, close-up, rendered from the interactive model.

Timeline

  1. 1998 The expansion of the universe is found to be accelerating.
  2. 2003 Caldwell, Kamionkowski and Weinberg publish "Phantom Energy and Cosmic Doomsday".
  3. 2025 DESI finds hints that dark energy is weakening, pointing away from a Big Rip.

Questions people ask

Will the Big Rip happen?

Probably not. It requires dark energy with w below −1, and measurements so far are close to −1, with recent DESI results hinting at w above −1.

When would the Big Rip happen?

In the 2003 paper's example with w = −1.5, in 22 billion years. With today's measurements, at least about 200 billion years away, if at all.

What is the difference between the Big Rip and the Big Freeze?

In the Big Freeze, galaxies drift apart and everything slowly runs down. In the Big Rip, expansion grows strong enough to tear apart galaxies, planets and atoms.

Sources

  1. Caldwell, Kamionkowski & Weinberg (2003), Phantom Energy and Cosmic Doomsday, Phys. Rev. Lett. 91: 071301
  2. Wikipedia: Big Rip
  3. DESI Collaboration (2025), DESI DR2 results II: baryon acoustic oscillations and cosmological constraints