Cosmic microwave background radiation. See related link for more information.
The radiation left over from the big bang, known as the cosmic microwave background radiation, has not dissipated to the far ends of the universe because it is constantly expanding and cooling as the universe expands. This radiation is spread uniformly throughout space, and although it has cooled significantly since the big bang, it can still be detected in all directions.
It follows logically from what we know about physics that the expansion of the universe from a hot and dense state should produce a remnant of microwave radiation. Reasoning from the Big Bang model (particularly the LCDM model), it is also possible to work out the intensity (temperature) of that radiation, and the nature, size and distribution of variations in that radiation. Detailed observations of the night sky have confirmed these predictions to a remarkable degree.
Cosmic Microwave Background Radiation is electromagnetic radiation left over from the events of the Big Bang. This radiation causes a very slight increase in the universe's temperature; the coldest areas of the universe will be only about 2 degrees kelvin (2 degrees above absolute zero). It is not spread in a perfectly uniform pattern, though the differences in density are very slight.
Among other things, it means Cosmic Microwave Background.
The Big Bang
Cosmic microwave background radiation. See related link for more information.
The radiation left over from the big bang, known as the cosmic microwave background radiation, has not dissipated to the far ends of the universe because it is constantly expanding and cooling as the universe expands. This radiation is spread uniformly throughout space, and although it has cooled significantly since the big bang, it can still be detected in all directions.
Cosmic background uniform microwave radiation left over from the big bang.
the universe underwent a Big Bang, as this radiation is the remnant heat left over from the early stages of the universe. This background radiation, known as the cosmic microwave background, supports the Big Bang theory as it provides a way to study the conditions in the early universe.
The Cosmic Microwave Background Radiation (CBR) was discovered by Arno Penzias and Robert Wilson in 1965. They were working on a radio telescope and found an unexpected source of noise that turned out to be radiation left over from the early universe, providing evidence for the Big Bang theory.
nothing happened to that radiation that still expanding one or another day it will explodes that radiation is one ane only has the velocity that equal to light that is gamma radiation
The heat left over from the beginning of the universe is known as the cosmic microwave background radiation. It is a faint glow of radiation that permeates the entire universe and is a remnant of the Big Bang. This radiation provides important clues about the early universe and the formation of galaxies.
The age of the universe is determined by CMBR, which is left over energy from the Big Bang Theory. CMBR stands for Cosmic Microwave Background Radiation.
It follows logically from what we know about physics that the expansion of the universe from a hot and dense state should produce a remnant of microwave radiation. Reasoning from the Big Bang model (particularly the LCDM model), it is also possible to work out the intensity (temperature) of that radiation, and the nature, size and distribution of variations in that radiation. Detailed observations of the night sky have confirmed these predictions to a remarkable degree.
A theory that states that the universe began with a tremendous explosion.
The cosmic microwave background radiation is visible in all directions because it represents the thermal radiation left over from the Big Bang. As the universe expanded and cooled, this radiation became uniform in all directions, making it observable from any location in the universe.