Cosmological concept · Cosmology
The Expansion of the Universe
Cosmology & UniverseEstablished Science
Definition
The observed stretching of space itself, which carries galaxies apart at rates proportional to their distance.
Scientific overview
Space between galaxies is expanding, so distant galaxies recede from us — and from each other — with a speed proportional to their distance. Galaxies are not moving through space so much as being carried along by the growth of space itself.
Evidence
- The redshift–distance relation of galaxies
- The cosmic microwave background
- Baryon acoustic oscillations
Rests on
Related discoveries & objects
Related scientists
Related topics
Knowledge connections
- Related toCosmological Redshift
- Related toThe Hubble–Lemaître Law
- Related toThe Hubble Constant
- Depends onGeneral Relativity
- Related toThe Expansion of the Universe
- Studied byEdwin Hubble
- Studied byGeorges Lemaître
- Related toCosmological Redshift
- Related toThe Hubble–Lemaître Law
- Related toThe Hubble Constant
- Related toThe Observable Universe
- Related toBaryon Acoustic Oscillations
- Related toDark Energy
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.