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Cosmic Microwave Background Trivia Questions

How much do you really know about Cosmic Microwave Background? Below are 8 true or false statements. Click each one to reveal the answer and explanation.

1.

The CMB is perfectly uniform across the entire sky with no variations at all.

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Easy
✗ FALSE

The CMB has tiny temperature fluctuations (about 1 part in 100,000) that reveal the seeds of galaxies and large-scale cosmic structure.

2.

The cosmic microwave background was first detected accidentally by radio astronomers in 1964.

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Easy
✓ TRUE

Arno Penzias and Robert Wilson found the CMB as unexplained noise in their horn antenna at Bell Labs, earning them the Nobel Prize in 1978.

3.

CMB photons have been traveling toward Earth for over 13.8 billion years, since the universe became transparent.

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Medium
✓ TRUE

The CMB originated about 380,000 years after the Big Bang, when protons and electrons combined to form neutral hydrogen, releasing photons that still travel today.

4.

The CMB temperature is exactly 3 Kelvin everywhere in the universe, with no directional differences.

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Medium
✗ FALSE

The CMB is about 2.725 K on average, but shows a dipole anisotropy due to Earth’s motion relative to the cosmic rest frame—about 0.003 K warmer in one direction.

5.

The CMB is actually radio static that fills the universe, and you can see it on an old TV as snow.

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Medium
✓ TRUE

About 1% of the static on an analog TV tuned to a blank channel comes from the CMB—a faint hiss from the Big Bang’s afterglow.

6.

The CMB was emitted by the first stars, which formed when the universe was about 500 million years old.

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Hard
✗ FALSE

The CMB comes from the recombination era, long before stars existed. The first stars ignited hundreds of millions of years later.

7.

The CMB has a perfect blackbody spectrum, matching theoretical predictions better than any other source in nature.

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Hard
✓ TRUE

COBE satellite measurements in the 1990s showed the CMB spectrum matches a 2.725 K blackbody curve with astonishing precision, confirming the Big Bang model.

8.

The CMB is slowly cooling over time because the universe’s expansion stretches its wavelengths.

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Hard
✓ TRUE

As space expands, CMB photons are redshifted to longer wavelengths, lowering their effective temperature—from about 3000 K at emission to 2.725 K today.

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