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Cosmological concept · Cosmology

Dark Energy

Cosmology & UniverseStrong Evidence

Definition

The unknown component driving the accelerating expansion of the Universe, making up roughly 68% of it.

Scientific overview

In 1998 two teams found that cosmic expansion is speeding up, not slowing down. The cause — dubbed dark energy — behaves like an energy of empty space with negative pressure. It dominates the present Universe but its nature is a complete mystery.

Evidence

  • Type Ia supernovae (1998)
  • The CMB combined with large-scale structure
  • Baryon acoustic oscillations

Current measurements

Fraction of the Universe≈ 68%Planck Collaboration

Open questions

  • Is dark energy a cosmological constant, or does it evolve?
  • Why is its value so small yet non-zero?

Rests on

Related discoveries & objects

Measured by

Related scientists

Knowledge connections

Sources & references

The primary and reference sources this topic draws on.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.

  • ESAEuropean Space Agency

    European missions, observatories, and space science imagery.

  • DESIDark Energy Spectroscopic Instrument

    Spectroscopic redshift survey measuring baryon acoustic oscillations and dark energy.