6.2.8

Cosmic Microwave Background Radiation

Test yourself on Cosmic Microwave Background Radiation

Test your knowledge with free interactive questions on Seneca — used by over 10 million students.

Cosmic Microwave Background Radiation

CMBR

CMBR

  • Scientists detect microwave radiation coming from all directions in space.
  • This is called cosmic microwave background radiation (CMBR).
Origin

Origin

  • CMBR was produced shortly after the Big Bang, when the Universe was very hot.
  • At that time, the radiation was in the visible and infrared regions of the spectrum.
Universe expansion

Universe expansion

  • As the Universe expanded, the radiation’s wavelength was stretched.
  • This stretching moved it into the microwave region of the electromagnetic spectrum.
Big Bang

Big Bang

  • The discovery of CMBR is strong evidence for the Big Bang theory.
  • It shows that the Universe once began in a hot, dense state and has been expanding ever since.

Speed of a Galaxy

Redshift

Redshift

  • When we look at light from distant galaxies, we often see a redshift.
  • Redshift means the wavelength of the starlight is stretched.
  • This happens because the galaxy is moving away from Earth.
  • The faster the galaxy moves away, the greater the redshift we observe.
Hubble's Law

Hubble's Law

  • The speed vv of the galaxy can be calculated from the change in wavelength of its starlight.
  • Astronomers can also estimate the distance dd of far galaxies.
  • Distance can be found using the relationship between redshift and the expansion of the Universe (Hubble’s law).
  • Together, speed and distance measurements give evidence that the Universe is expanding.
Jump to other topics
1

Motion, Forces & Energy

1.1

Physical Quantities & Measurement Techniques

1.2

Motion

1.3

Mass & Weight

1.4

Density

1.5

Forces: Effects of Forces

1.6

Forces: Turning Effects of Forces

1.7

Forces: Centre of Gravity

1.8

Momentum

1.9

Energy, Work, & Power: Energy

1.10

Energy, Work & Power: Work

1.11

Energy, Work & Power: Energy Resources

1.12

Energy, Work & Power: Power

1.13

Pressure

2

Thermal Physics

3

Waves

4

Electricity & Magnetism

4.1

Simple Phenomena of Magnetism

4.2

Electrical Quantities: Electric Charge

4.3

Electrical Quantities: Electric Current

4.4

Electromotive Force & Potential Difference

4.5

Electrical Quantities: Resistance

4.6

Electrical Energy & Electrical Power

4.7

Electric Circuits: Circuit Diagrams & Components

4.8

Electric Circuits: Series & Parallel Circuits

4.9

Electric Circuits: Action & Use

4.10

Electrical Safety

4.11

Electromagnetic Effects: Electromagnetic Induction

4.12

Electromagnetic Effects: The A.C. Generator

4.13

Magnetic Effect of a Current

4.14

Force on a Current-Carrying Conductor

4.15

Electromagnetic Effects: The D.C. Motor

4.16

Electromagnetic Effects: The Transformer

5

Nuclear Physics

6

Space Physics

Practice questions on Cosmic Microwave Background Radiation

Can you answer these? Test yourself with free interactive practice on Seneca — used by over 10 million students.

  1. 1
  2. 2
  3. 3
  4. 4
  5. 5
Answer all questions on Cosmic Microwave Background Radiation

Unlock your full potential with Seneca Premium

  • Unlimited access to 10,000+ open-ended exam questions

  • Mini-mock exams based on your study history

  • Unlock 800+ premium courses & e-books

Get started with Seneca Premium