Scale & fate of the universe

Cosmic microwave background

The afterglow of the Big Bang, still arriving from every direction at 2.725 degrees above absolute zero

Artist's impression · drag to rotate
Temperature 2.72548 K (-270 °C) ± 0.00057 [2]
Emitted about 380 000 years after the Big Bang [1]
Discovered 1964 Arno Penzias and Robert Wilson [1]
Predicted 1948 Ralph Alpher and Robert Herman, about 5 K (-268 °C) [1]
Ripples about 1 part in 100 000 found by COBE in 1992 [3]
Photons about 411 per cm³ [1]
Best map Planck, 2009–2013 final results 2018 [4]
Nobel Prizes 1978 and 2006 [1]

About the image. Drawn as a sphere covered with a pattern like the Planck satellite's maps of the background, in false colour: blue slightly colder, red slightly warmer. The real pattern is invisible to the eye, and the differences are only about one part in 100 000.

In 1964 two radio astronomers at Bell Labs in New Jersey, Arno Penzias and Robert Wilson, were trying to get rid of a faint hiss in their horn-shaped antenna. It came from every direction, day and night, whatever they did. They checked the electronics and cleared out pigeon droppings. The hiss remained. They had found the cosmic microwave background, the oldest light in the universe, and in 1978 they shared the Nobel Prize in Physics for it.

Light from the beginning

For its first few hundred thousand years, the universe was a hot, glowing fog of charged particles. Light could not travel far before bouncing off an electron. About 380 000 years after the Big Bang, the universe cooled enough for electrons and nuclei to combine into atoms, and the fog cleared. The light released at that moment has been travelling ever since.

As the universe expanded, that light was stretched from visible and infrared light into microwaves. Today it is a bath of radiation with a temperature of just 2.725 degrees above absolute zero. Every cubic centimetre of space holds about 411 of its photons. Some of the snow on an old analogue television tuned between channels came from it.

Its existence had been predicted. In 1948 Ralph Alpher and Robert Herman calculated that light left over from a hot early universe should still fill space at about 5 K (-268 °C).

The ripples

At first the background looked perfectly smooth. In 1992 NASA’s COBE satellite found tiny differences in temperature from place to place, about one part in 100 000. These ripples are the imprint of slight differences in density in the young universe: the seeds from which gravity later built galaxies and the cosmic web. John Mather and George Smoot shared the 2006 Nobel Prize for COBE’s measurements.

NASA’s WMAP satellite and then ESA’s Planck mapped the ripples ever more precisely. From their pattern cosmologists measure the age of the universe, 13.8 billion years, and how much of it is ordinary matter, dark matter and dark energy.

The Cold Spot

One feature stands out. In the constellation Eridanus there is a region about 5 degrees across that is about 70 millionths of a degree colder than average, larger and colder than expected. Planck confirmed it is real. Whether it is a rare fluke, a huge void in front of it, or something stranger is still unknown.

How hot is it?

Earth (average)288 K · 15 °C
Water boils373 K · 100 °C
Venus surface737 K · 464 °C
Iron melts1 811 K · 1 540 °C
Sun's surface5 772 K · 5 500 °C
Cosmic microwave background2.725 K · -270 °C
Cosmic microwave background: temperature of the background. Logarithmic scale from 100 K to 10 000 K. Reference values: NASA, IAU.

Gallery

A sphere in black space covered in mottled orange and dark bluish patches, an impression of the cosmic microwave background drawn as a globe around the observer. AI-generated painting.
Cosmic microwave background, 3D artist's impression, rendered from the interactive model.
Cosmic microwave background, 3D artist's impression, from another angle, rendered from the interactive model.
Cosmic microwave background, 3D artist's impression, close-up, rendered from the interactive model.

Timeline

  1. 1948 Ralph Alpher and Robert Herman predict a leftover glow at about 5 K (-268 °C).
  2. 1964 Arno Penzias and Robert Wilson detect it at Bell Labs.
  3. 1992 COBE finds ripples of about one part in 100 000.
  4. 2006 John Mather and George Smoot win the Nobel Prize.
  5. 2018 Planck publishes its final results.

Questions people ask

What is the cosmic microwave background?

Light released about 380 000 years after the Big Bang, when the universe first became transparent, now stretched into microwaves.

How cold is the cosmic microwave background?

2.725 kelvin, less than three degrees above absolute zero.

Can you see the CMB on a TV?

Partly. Some of the snow on an analogue television tuned between channels came from it.

Sources

  1. Wikipedia: Cosmic microwave background
  2. Fixsen (2009), The temperature of the cosmic microwave background, ApJ 707
  3. Wikipedia: Cosmic Background Explorer
  4. Wikipedia: Planck (spacecraft)
  5. Wikipedia: CMB cold spot
  6. NASA Planetary Fact Sheet (planet temperatures, orbits, Jupiter's gravity)
  7. IAU 2015 Resolution B3 (nominal solar values)
  8. NASA: Voyager mission
  9. NASA: Parker Solar Probe
  10. Breakthrough Starshot