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Loading contentAn unseen form of matter, detected only through its gravity, that outweighs ordinary matter roughly five to one.
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.
| Fraction of the Universe | ≈ 27% | Planck Collaboration |
Facts on this topic will be cited from these primary and reference sources.
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.
Cosmic microwave background maps and the cosmological parameters of the ΛCDM model.
European missions, observatories, and space science imagery.