Primordial Radiation: High Energy Light Big Bang Quiz

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| Questions: 20 | Updated: Feb 13, 2026
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1. What is the Cosmic Microwave Background (CMB) radiation?

Explanation

If the early universe was extremely hot and dense, then it was filled with high-energy plasma. If the universe expanded and cooled over 13.8 billion years, then that original high-energy light would stretch into longer wavelengths. If those waves are now in the microwave range, then they represent the earliest light we can detect. Therefore, the CMB is the afterglow of the Big Bang.

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About This Quiz
Primordial Radiation: High Energy Light Big Bang Quiz - Quiz

Tracing the universe back to its hottest, brightest moments. The light we see today began as high-energy radiation that has been traveling for billions of years. This high energy light big bang quiz deciphers the ancient signals left over from the start of time.

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2. The early universe was opaque to light because it was a hot plasma of free electrons and protons.

Explanation

If free electrons are present, then they scatter photons in every direction, preventing light from traveling long distances. If the universe was too hot for atoms to form, then electrons remained free. Therefore, light was "trapped" in a fog until the universe cooled enough for neutral atoms to form.

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3. What event allowed the universe to become transparent to light approximately 380,000 years after the Big Bang?

Explanation

If the universe cooled to about 3000 Kelvin, then protons could finally capture electrons to form neutral Hydrogen atoms. If electrons are bound in atoms, then they no longer scatter photons. Therefore, light could finally travel freely through space, an event known as Recombination.

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4. The stretching of light's wavelength as the universe expands is called ______ Redshift.

Explanation

If the fabric of space itself is expanding, then any light traveling through it will have its wavelength stretched along with space. If stretching a wavelength moves it toward the red end of the spectrum, then it is a redshift. Therefore, this specific type is called Cosmological Redshift.

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5. Why did the Big Bang produce mostly Hydrogen and Helium, but almost no heavy elements like Iron?

Explanation

If the synthesis of heavy elements requires high density and temperature for a long time, then the conditions must last. If the Big Bang expansion was extremely rapid, then the temperature dropped below the fusion threshold within minutes. Therefore, only the lightest elements had time to form before the "cosmic furnace" turned off.

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6. According to Wien’s Law, as the universe cools, the peak wavelength of its background radiation becomes shorter.

Explanation

If Wien's Law states that peak wavelength is inversely proportional to temperature (λmax​∝1/T), then a decrease in temperature must result in an increase in wavelength. If the universe is cooling, then the light shifts toward the longer (colder) end of the spectrum. Therefore, the statement is false.

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7. What does the "high-energy" part of the early universe's spectrum tell us about its initial state?

Explanation

If the earliest light we detect (stretched to microwaves) originated as high-energy Gamma or X-rays, then the source must have been incredibly hot. If that heat was spread throughout all of space, then the matter must have been packed tightly together. Therefore, the spectrum proves a hot, dense beginning.

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8. The observation that galaxies further away are moving away faster is known as ______ Law.

Explanation

If Edwin Hubble observed that a galaxy's redshift is proportional to its distance, then the universe must be expanding uniformly. If this relationship is expressed as v=H0​d, then it is the foundational law of expansion. Therefore, it is Hubble's Law.

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9. What is "Nucleosynthesis" in the context of the Big Bang?

Explanation

If the universe was a hot soup of subatomic particles, then collisions would eventually stick protons and neutrons together. If this occurred between 3 and 20 minutes after the Big Bang, then it created the first nuclei. Therefore, this is Big Bang Nucleosynthesis.

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10. Which of the following are evidence for the Big Bang theory?

Explanation

If a theory predicts a specific afterglow (CMB), a specific mix of light elements (H/He ratio), and an expanding universe (Redshift), then observing those three things confirms the theory. If Mars' water or the Milky Way's shape don't directly relate to the origin of the entire universe, then they are not primary evidence. Therefore, A, B, and D are correct.

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11. If the CMB temperature is currently 2.7 Kelvin, what does this tell us about the expansion of the universe?

Explanation

If the radiation started at thousands of degrees during Recombination and is now only 2.7 degrees above absolute zero, then a massive amount of cooling has occurred. If cooling in space is caused by the stretching of light waves (expansion), then the universe must have grown significantly. Therefore, 2.7K is proof of vast expansion.

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12. High-energy Gamma rays from the Big Bang have now been stretched into Microwaves.

Explanation

If the photons released during the early stages of the universe were high-energy, then they had very short wavelengths. If space has expanded by a factor of about 1100 since Recombination, then those wavelengths have increased 1100 times. Therefore, high-energy light has shifted into the low-energy microwave band.

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13. What is the "Planck Era"?

Explanation

If we trace the Big Bang back to t=0, then we reach a point of infinite density. If we reach 10−43 seconds (Planck time), then gravity and quantum mechanics conflict. Therefore, the Planck Era represents the theoretical limit of our current understanding.

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14. Tiny fluctuations in the temperature of the CMB are called ______ and they represent the seeds of future galaxies.

Explanation

If the CMB were perfectly smooth, then matter would never have clumped together. If there are tiny "hot" and "cold" spots (anisotropies), then these indicate regions of slightly higher or lower density. Therefore, gravity acted on these density differences to build galaxies.

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15. Which particles were present in the "Quark-Gluon Plasma" of the very early universe?

Explanation

If the temperature was trillions of degrees, then even protons and neutrons could not stay together. If protons are made of quarks and gluons, then those particles would roam free. If electrons were also present as fundamental particles, then A, B, and C are the correct constituents.

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16. What would happen to the CMB if the universe started to contract (shrink)?

Explanation

If expansion causes a redshift and cooling, then the opposite process (contraction) must cause a blueshift and heating. If the wavelengths are squeezed, then the energy of the photons increases. Therefore, the background radiation would get hotter.

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17. Dark Energy is the name given to the force that seems to be accelerating the expansion of the universe.

Explanation

If gravity is an attractive force, then the expansion of the universe should be slowing down. If observations of distant supernovas show that the expansion is actually speeding up, then an unknown "repulsive" energy must exist. Therefore, we call this Dark Energy.

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18. The period of extremely rapid expansion in the first fraction of a second is called ______.

Explanation

If the universe is remarkably flat and uniform, then it must have smoothed itself out very early on. If a burst of exponential expansion occurred at t=10−36 seconds, then it explains these features. Therefore, this event is called Inflation.

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19. What is the significance of the "Surface of Last Scattering"?

Explanation

If light was constantly bouncing (scattering) off electrons in the early plasma, then it couldn't travel. If Recombination happened, then the light scattered one "last" time before traveling to us. Therefore, looking at the CMB is like looking at the physical "surface" of the early universe.

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20. The Big Bang was an explosion that happened at a specific center point in empty space.

Explanation

If the Big Bang was the expansion of space itself, then it didn't happen in space. If every point in the universe was part of the initial hot state, then the expansion is happening everywhere at once. Therefore, there is no "center" to the Big Bang.

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What is the Cosmic Microwave Background (CMB) radiation?
The early universe was opaque to light because it was a hot plasma of...
What event allowed the universe to become transparent to light...
The stretching of light's wavelength as the universe expands is called...
Why did the Big Bang produce mostly Hydrogen and Helium, but almost no...
According to Wien’s Law, as the universe cools, the peak wavelength...
What does the "high-energy" part of the early universe's spectrum tell...
The observation that galaxies further away are moving away faster is...
What is "Nucleosynthesis" in the context of the Big Bang?
Which of the following are evidence for the Big Bang theory?
If the CMB temperature is currently 2.7 Kelvin, what does this tell us...
High-energy Gamma rays from the Big Bang have now been stretched into...
What is the "Planck Era"?
Tiny fluctuations in the temperature of the CMB are called ______ and...
Which particles were present in the "Quark-Gluon Plasma" of the very...
What would happen to the CMB if the universe started to contract...
Dark Energy is the name given to the force that seems to be...
The period of extremely rapid expansion in the first fraction of a...
What is the significance of the "Surface of Last Scattering"?
The Big Bang was an explosion that happened at a specific center point...
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