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Glossary

3 Degree Kelvin Background Radiation

Also called Cosmic Microwave Background Radiation. Radiation emitted when the universe used to be very hot. Some 300 thousand years after the Big Bang, electrons that had inhibited light to travel in a straight line were captured by atoms, allowing radiation to travel straight. The radiation then emitted cooled down to the temperature of 3K with the expansion of the universe, becoming observable for the first time. This observable radiation is known as 3 Degree Kelvin Background Radiation.

WMAP

A NASA program to accurately measure CMB radiation. In 2001 a satellite was launched, and in 2003 detailed radiation measurements were released.

Dark energy

Dark energy is a constant density energy regardless of the size of the universe. Its force causes the universe to expand. The nature of dark energy is not yet known.

Dark matter

Dark matter is the name given to most of the matter in the universe, which is invisible. Types of particles that could be dark matter are non-luminous materials, and elementary particles such as neutralinos and axions.




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