the discovery of a cosmic microwave background


Why was cosmic background radiation an important discovery?

This radiation was discovered in 1964. It is called cosmic microwave background radiation or CMBR. CMBR is a second piece of evidence to show the expansion of space, and this supports the Big Bang model of the origin of the Universe.

Why do we still see Cosmic Background radiation?

The cosmic microwave background (CMB) is leftover radiation from the Big Bang or the time when the universe began. As the theory goes, when the universe was born it underwent rapid inflation, expansion and cooling. (The universe is still expanding today, and the expansion rate appears different depending on where you look ).

Where can cosmic background radiation be found?

Cosmic Background Radiation. In 1964 Arno Penzias and Robert Wilson discovered a form of radiation found everywhere in the universe. This data was later theorized to be connected with the Big Bang Theory. Penzias and Wilson noticed a radio background source all across the sky. It was later discovered that the sky is uniformly lit up in a ...

Who discovered cosmic background radiation?

The discovery of cosmic microwave background radiation constitutes a major development in modern physical cosmology. In 1961, US physicist Arno Allan Penzias and radio-astronomer Robert Woodrow Wilson discovered the CMB, estimating its temperature as 3.5 K, as they experimented with the Holmdel Horn Antenna.

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