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This thing is -270°C and is EVERYWHERE

January 21, 2020
by
Physics Girl
YouTube video player
This thing is -270°C and is EVERYWHERE

TL;DR

The Cosmic Microwave Background (CMB) is a signal discovered by accident in the 1960s that originated from the beginning of the universe, providing valuable information about its origin and evolution.

Transcript

(button clicks) (static crackling)- We eliminated just about everything. And then the only possibility was that it was coming from someplace outside our galaxy. And that seemed like such a far out idea. We just, we just didn't know what to do with that result. - Hey I'm Diana and you're watching Physics Girl. There's this thing that's all around us... Read More

Key Insights

  • 📻 The CMB was discovered accidentally in the 1960s by two radio astronomers, who initially mistook it for background noise.
  • 📡 The CMB is a signal from the beginning of the universe, originating just after the Big Bang.
  • 🎁 The CMB is composed of microwaves and is present everywhere in the universe.
  • 💁 Studying the CMB provides valuable information about the origin, composition, and evolution of the universe.
  • 👻 The CMB confirms the Big Bang theory and allows scientists to study phenomena like quantum fluctuations and dark energy.
  • 👾 Specialized probes have been sent into space to create detailed images of the CMB, revealing temperature fluctuations and assisting in the study of dark energy and galaxy clusters.
  • 😎 The CMB has cooled significantly over time and is currently at a temperature of 2.7 Kelvin.

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Questions & Answers

Q: How did scientists discover the Cosmic Microwave Background (CMB)?

Scientists Robert Wilson and Arno Penzias discovered the CMB while testing a microwave antenna and noticed a constant background noise that couldn't be eliminated. Further research by Robert Dickey's team at Princeton University revealed the origin of the noise as the CMB.

Q: What is the significance of the CMB?

The CMB is a signal from the beginning of the universe, providing valuable insights into the origin, evolution, and composition of the universe. It confirms the Big Bang theory and allows scientists to study phenomena like quantum fluctuations and dark energy.

Q: How did the CMB form?

After the Big Bang, the universe was hot and dense, filled with particles and radiation. The early universe was essentially opaque due to constant collisions between electrons, protons, and photons. After about 380,000 years, the universe cooled enough for atoms to form, allowing light to travel unobstructed and creating the CMB.

Q: How is the CMB studied?

Specialized probes, such as NASA's Cosmic Background Explorer and the ESA's Planck spacecraft, have been sent into space to create complete images of the CMB. These images provide insights into temperature fluctuations, dark energy, galaxy clusters, and the expansion of the universe.

Summary & Key Takeaways

  • In the 1960s, two radio astronomers accidentally discovered a constant background noise that turned out to be the Cosmic Microwave Background (CMB), a signal from the early universe.

  • The CMB is everywhere in the universe and is composed of microwaves, with wavelengths in the millimeter to centimeter range.

  • The CMB originated just after the Big Bang, when the universe was densely filled with matter and radiation, and has been traveling across the universe since its formation.


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