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It is not really the universe that is changing, but rather the perception of our universe. The Cosmic Microwave Background Radiation (CMBR, or CMB) marks the limit of our ability to perceive our universe. Everything we know about the universe is based on our ability to observe and measure varying degrees of luminosity/radiation within this fourth dimensional confinement; i.e., this is our known universe. Our known universe has many imposed limitations, based on our ability to observe and measure it, but no one can really estimate as to the actual age and size of the universe beyond the interpretation of empirical evidence we are able to gather and collate. As of matter of contention is whether these measures for age and size have any real meaning outside our observable universe. ===== For example: While this CMB barrier may represent the primordial condition of our universe, it is only representative of past radiated events. Therefore at the extreme point in Space-Time to which an observer can view the CMB barrier, an opposing observer from this extreme point could be looking back at us and only see the CMB barrier as well. This would also imply that the universe is much larger than we are able to measure; for at the extreme point in Space-Time to which our first observer can view this CMB barrier, a second observer at this extreme point (and facing away from the first observer) can see even further into the universe than the first observer.

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

cosmic microwave background radiation.


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


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.


How the universe is changing by cosmic background?

The cosmic background radiation is an observation of the effects of the Big bang [See related question] it does not effect the Universe changing in anyway.


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.


How cosmic microwave background radiation shows us the universe is changing?

It shows that at the beginning of time all radiation was trapped in a small place and since the universe has expanded and cooled so has the radiation which is why it has dropped from very high radiation to its fairly low microwave radiation state. Today. It is the afterglow of the universe which heavily backs up the big bang theory.


Which theory of the universe did the 1964 discovery of cosmic microwave background radiation support?

The 1964 discovery of cosmic microwave background radiation supported the Big Bang theory of the universe. This radiation is considered a remnant of the early stages of the universe when it was hot and dense, aligning with the predictions of the Big Bang model.