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Cosmological concept · Cosmology

Dark Matter

Cosmology & UniverseStrong Evidence

Definition

An unseen form of matter, detected only through its gravity, that outweighs ordinary matter roughly five to one.

Scientific overview

Dark matter does not emit or absorb light, but its gravity is required to explain the rotation of galaxies, the motions of galaxy clusters, gravitational lensing, and the pattern of the cosmic microwave background. It makes up about 27% of the Universe.

Evidence

  • Flat galaxy rotation curves (Rubin)
  • Cluster dynamics (Zwicky, 1933)
  • Gravitational lensing, e.g. the Bullet Cluster
  • The CMB power spectrum

Current measurements

Fraction of the Universe≈ 27%Planck Collaboration

Open questions

  • What is dark matter made of (WIMPs, axions, something else)?
  • Why has no particle been detected directly?
  • Could modified gravity explain the observations instead?

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.

  • Planck CollaborationESA Planck mission / Planck Collaboration

    Cosmic microwave background maps and the cosmological parameters of the ΛCDM model.

  • ESAEuropean Space Agency

    European missions, observatories, and space science imagery.