Cosmological concept · Cosmology
The Cosmic Microwave Background
Cosmology & UniverseEstablished Science
Definition
The faint, uniform microwave glow left over from recombination — the oldest light in the Universe.
Scientific overview
The CMB is relic radiation released 380,000 years after the Big Bang, now cooled by expansion to just 2.7 K. Its near-perfect uniformity, tiny temperature fluctuations (1 part in 100,000), and detailed spectrum encode the composition, geometry, and age of the Universe.
Evidence
- Its perfect blackbody spectrum (COBE)
- Temperature anisotropies (WMAP, Planck) that fix the cosmological parameters
Current measurements
| Temperature | 2.7255 ± 0.0006 K | Planck Collaboration |
Rests on
Related discoveries & objects
Measured by
Related scientists
Knowledge connections
- Predicted byThe Big Bang
- Predicted byCosmic Inflation
- Predicted byRecombination
- Depends onRecombination
- Part of modelThe Lambda-CDM Model
- Related toThe Cosmic Microwave Background
- Studied byArno Penzias
- Studied byRobert Wilson
- Measured byCOBE (Cosmic Background Explorer)
- Measured byWMAP (Wilkinson Microwave Anisotropy Probe)
- Measured byPlanck
- Related toThe Lambda-CDM Model
- Associated withCMB Measurements
- Associated withScalar Spectral Index (ns)
- Associated withEarly Dark Energy
- Associated withQuantum Fluctuations
- Associated withThe Cosmic Neutrino Background
- Associated withThe GZK Limit
Sources & references
The primary and reference sources this topic draws on.
- Planck CollaborationESA Planck mission / Planck Collaboration
Cosmic microwave background maps and the cosmological parameters of the ΛCDM model.
- 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.