Scale & fate of the universe

The observable universe

A bubble 93 billion light-years across, with us at the centre and the oldest light in the universe at its edge

Artist's impression · drag to rotate
Radius about 46.5 billion light-years 14.26 gigaparsecs, measured as the distance today [1]
Diameter about 93 billion light-years [1]
Age of the universe 13.787 ± 0.020 billion years Planck 2018 [1]
Oldest light the cosmic microwave background from about 380 000 years after the Big Bang [1]
Galaxies hundreds of billions to 2 trillion estimates differ [3]
Atoms about 10⁸⁰ [1]
Most distant galaxy MoM-z14 redshift 14.44, light from 280 million years after the Big Bang [5]

About the image. Drawn as a sphere seen from outside, with a slice cut away. Its surface shows the pattern of the cosmic microwave background, the oldest light we can see; inside is a stylised cosmic web, and the bright point at the centre is us. Nobody can see the observable universe from outside: every observer sits at the centre of their own.

The universe is about 13.8 billion years old, and light travels at a fixed speed. So there is a limit to how far we can see: only light that has had time to reach us since the beginning can be seen at all. Everything inside that limit is the observable universe. It is a sphere with Earth at its centre, though any observer anywhere would find themselves at the centre of their own.

Bigger than its age

You might expect the edge to be 13.8 billion light-years away. It is much further: about 46.5 billion light-years, making the observable universe about 93 billion light-years across. The difference comes from the expansion of space. While the oldest light was travelling towards us, the space it crossed kept stretching, and the matter that sent it was carried further away. The distance to that matter today is far greater than the distance the light itself covered.

Galaxies near the edge are moving away from us faster than light. This does not break relativity, which limits motion through space, not the stretching of space itself.

The edge

The farthest thing we can see is not a galaxy but a glow. For its first 380 000 years or so, the universe was a hot, opaque fog of charged gas. When it cooled enough for atoms to form, light could travel freely for the first time. That light, stretched by expansion into microwaves, still arrives from every direction. It is the cosmic microwave background, and it marks the edge of what light can show us.

The most distant galaxies sit just inside it. In 2024 the James Webb Space Telescope confirmed JADES-GS-z14-0, a galaxy seen as it was less than 300 million years after the Big Bang. In 2025 a team led by Rohan Naidu reported MoM-z14 at redshift 14.44, light that set out about 280 million years after the Big Bang.

How much is in it?

Estimates of the number of galaxies vary. A 2016 study by Christopher Conselice and colleagues suggested about two trillion, counting the many small, faint galaxies of the early universe. Measurements of the faint background light from far out in the Solar System, made with the New Horizons probe in 2021, pointed to fewer: hundreds of billions. All together, the observable universe holds something like 10⁸⁰ atoms.

Beyond the edge

The observable universe is not the whole universe. Nobody knows how large the whole is, or whether it is infinite. Because expansion is speeding up, some of what we can see now will one day slip out of reach: light we send today can never reach galaxies more than about 16 billion light-years away.

Gallery

A glowing sphere whose cut-open face shows swirling golden threads of galaxies around a bright centre, an impression of the observable universe. AI-generated painting.
The observable universe, 3D artist's impression, rendered from the interactive model.
The observable universe, 3D artist's impression, from another angle, rendered from the interactive model.
The observable universe, 3D artist's impression, close-up, rendered from the interactive model.

Timeline

  1. 2016 Conselice and colleagues estimate about two trillion galaxies.
  2. 2018 Planck gives the age of the universe as 13.787 ± 0.020 billion years.
  3. 2021 New Horizons measurements suggest hundreds of billions of galaxies instead.
  4. 2024 JWST confirms JADES-GS-z14-0.
  5. 2025 MoM-z14 at redshift 14.44 becomes the most distant galaxy known.

Questions people ask

How big is the observable universe?

About 93 billion light-years across, with a radius of about 46.5 billion light-years.

Why is the observable universe bigger than 13.8 billion light-years?

Space kept expanding while the light was travelling, so the matter that sent the oldest light is now much further away than the distance the light covered.

Is the observable universe the whole universe?

No. It is only the part whose light has had time to reach us. The whole universe may be far larger, or infinite.

How many galaxies are in the observable universe?

Estimates range from hundreds of billions to about two trillion.

Sources

  1. Wikipedia: Observable universe (Planck 2018)
  2. Wikipedia: Cosmic microwave background
  3. Conselice et al. (2016), The evolution of galaxy number density at z < 8, ApJ 830: 83
  4. CNN via ABC17 News (2021): There may be fewer galaxies in the universe than we thought (New Horizons)
  5. Naidu et al. (2025), A cosmic miracle: a remarkably luminous galaxy at z = 14.44
  6. Wikipedia: JADES-GS-z14-0