Learn / The universe

How big is the universe?

How it works

Cause and effect, with real numbers.

  1. First look
  2. How it works
  3. The physics, still to be written
  4. The frontier, still to be written

How it works

Cause and effect, with real numbers

Three different distances. When something is very far away, “how far?” has more than one answer.

The question For the oldest light
How long was the light on its way? 13.8 billion years
How far off was its source when the light left? About 42 million light years
How far off is that source now? About 46 billion light years

The third is the one meant when the observable universe is said to be 46 billion light years in radius. It is about 3.4 times the figure most people expect, and about 1,100 times the distance at the start. Both worked out here.

Does that break the speed of light? No. Nothing travels through space faster than light. But space itself can stretch, and when there is a great deal of space between two galaxies, the gap between them can grow faster than light could cross it. Tamara Davis and Charles Lineweaver set this out in 2003 and showed that many of the galaxies already in our pictures are, and always have been, moving away faster than light in this sense.

A horizon that closes in. The expansion is speeding up, and that sets a second limit. Light leaving a galaxy today will never reach us if the galaxy is now more than about 16 billion light years away. We go on seeing such galaxies by the old light already on its way, but nothing that happens there from now on will ever be seen from here.

What “flat” means. On a flat sheet the angles of a triangle add up to 180 degrees. On a ball they add up to more. Space can be tested in the same way, using the sizes of the patches in the oldest light as the far side of an enormous triangle. NASA’s WMAP spacecraft found space flat to within 0.4 per cent.

What cannot be said. Whether the universe is infinite is not something any measurement can settle, because no measurement can reach past the edge of sight. Science can say how big the visible part is, and that the rest is at least very much bigger. Beyond that, it is honest to say nobody knows.

An oval map of the whole sky mottled evenly in blue, green, yellow and red specks.
A map, not a photograph. The oldest light over the whole sky, from nine years of measurements by NASA's WMAP spacecraft. Microwaves have no colour: red was chosen for slightly warmer patches and blue for slightly cooler. Credit: NASA/WMAP Science Team.

Where this comes from

The words are written for this site. Sums in the text are worked from the figures in these sources.