answersLogoWhite

0

I didn't check the year... But the cosmic background radiation is said to support the big bang theory, because it agrees with the radiation that is expected from an expanding Universe.


User Avatar

Wiki User

12y ago

What else can I help you with?

Related Questions

The heat left over from the beginning of the universe is?

cosmic microwave background radiation.


What discovery destroyed the steady state theory?

The discovery of the cosmic microwave background radiation in 1965 by Penzias and Wilson provided strong evidence in support of the Big Bang theory, contradicting the predictions of the steady state theory. The steady state theory proposed a continuous creation of matter to maintain a constant density of the universe, but the presence of the cosmic microwave background radiation was better explained by the rapid expansion and cooling of the universe after the Big Bang.


What is background microwave?

microwave background radiation is a thermal radiation left from the early stage of universe when it was much small and much hotter and filled with uniformly distributed opaque fog of hydrogen plasma


What did the discovery of background radiation distributed evenly throughout the universe provide support for?

The discovery of background radiation, known as the Cosmic Microwave Background (CMB), provided strong evidence for the Big Bang theory of the universe's origin. Its presence and uniform distribution across the universe offer a snapshot of the early universe, supporting the idea of a hot, dense beginning followed by expanding and cooling over time.


The heat left over from the beginning of the universe?

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.


How is Olbers' paradox resolved in the context of the expanding universe and the presence of cosmic microwave background radiation?

Olbers' paradox is resolved in the context of the expanding universe and the presence of cosmic microwave background radiation by understanding that the universe is not infinite in age or size. The expansion of the universe causes light from distant stars to redshift, making them fainter and cooler, and the cosmic microwave background radiation fills the universe with a uniform glow, accounting for the darkness of the night sky.


The Doppler shifting of radiation from the early universe has resulted in today's universe being bathed in a sea of?

Cosmic Microwave Background (CMB) Radiation.


What helped scientist determine the age of the universe?

The redshift of the cosmic microwave background radiation


Where did the cosimc microwave background radiation take place?

Where? Everywhere. This is the residual radiation, from when the Universe was very, very hot.


What did Penzias and Wilson discover?

Penzias and Wilson discovered the cosmic microwave background radiation in 1965, providing strong evidence for the Big Bang theory of the origin of the universe. This discovery earned them the Nobel Prize in Physics in 1978.


Cosmic microwave background radiation found uniformly spread throughout the universe is supposed to be what?

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.


What is the leftover thermal energy from the big bang?

The leftover thermal energy from the Big Bang is known as the cosmic microwave background radiation (CMB). It is a faint glow of radiation that permeates the universe and is considered a remnant from the early universe when it was much hotter and denser. The CMB provides important clues about the early universe's properties and evolution.