3.9.1
Doppler Effect
Doppler Effect
Doppler Effect
The Doppler effect, applied to electromagnetic radiation, is very useful in astrophysics and cosmology.


Formula
Formula
- For electromagnetic radiation, the following formula holds providing that the velocity of the source of the radiation is significantly lower than the speed of light.
- Where f is the frequency of light, and v is the speed of the emitting source.


Moving star
Moving star
- For a single star moving away from the Earth at a constant speed, the light from the star decreases in frequency.
- If the star is moving away at 0.01c (one hundredth of the speed of light), then the frequency of any given wavelength (typically one of the hydrogen lines) will be lower by 1%.
Binary Stars
Binary Stars
Binary stars are systems where two similar stars orbit around their combined centre of gravity.


Spectral line splitting
Spectral line splitting
- In a binary system, in which two stars orbit around a common centre of gravity, then the spectral line splits into two.


Explanation
Explanation
- This is explained by one star moving away from the Earth slightly less quickly and the other star moving away from the Earth slightly more quickly than in the single star case.


Orbital velocity
Orbital velocity
- The orbital velocity can be found by finding the recession speeds of the two stars (the speed the stars are moving away from us) and finding the difference.
- Half of that difference is the orbital speed of the star (assuming the two stars to be identical).
Galaxies and Quasars
Galaxies and Quasars
Galaxies are vast collections of stars in space. Quasars are very massive, high energy objects found in deep space.


Cosmological redshift
Cosmological redshift
- For galaxies and quasars, there is also a cosmological redshift, z, which is due to the expansion of the Universe itself.
- For low velocities:


Very distant objects
Very distant objects
- Very distant galaxies and quasars can have enormous z-values which can only really be explained by general relativity calculations.
1Space, Time & Motion
1.1Motion
1.2Forces
1.3Momentum & Impulse
2The Particulate Nature of Matter
2.1Thermal Concepts
3Wave Behaviour
3.1Oscillations
3.2Travelling Waves
3.3Wave Characteristics
3.4Wave Behaviour
3.5Standing Waves
3.6Simple Harmonic Motion
3.7Single Slit Diffraction
3.8Interference
3.9Doppler Effect
4Fields
4.1Circular Motion
4.2Newton's Law of Gravitation
4.3Fields
4.4Fields at Work
4.5Electric Fields
4.6Magnetic Effect of Electric Currents
4.7Heating Effect of Currents
4.8Electromagnetic Induction
4.9Power Generation & Transmission
5Nuclear & Quantum Physics
5.1Discrete Energy & Radioactivity
5.2Nuclear Reactions
5.3The Interaction of Matter with Radiation
6Measurements
6.1Measurements & Errors
6.2Uncertainties & Errors
6.3Vectors & Scalars
Jump to other topics
1Space, Time & Motion
1.1Motion
1.2Forces
1.3Momentum & Impulse
2The Particulate Nature of Matter
2.1Thermal Concepts
3Wave Behaviour
3.1Oscillations
3.2Travelling Waves
3.3Wave Characteristics
3.4Wave Behaviour
3.5Standing Waves
3.6Simple Harmonic Motion
3.7Single Slit Diffraction
3.8Interference
3.9Doppler Effect
4Fields
4.1Circular Motion
4.2Newton's Law of Gravitation
4.3Fields
4.4Fields at Work
4.5Electric Fields
4.6Magnetic Effect of Electric Currents
4.7Heating Effect of Currents
4.8Electromagnetic Induction
4.9Power Generation & Transmission
5Nuclear & Quantum Physics
5.1Discrete Energy & Radioactivity
5.2Nuclear Reactions
5.3The Interaction of Matter with Radiation
6Measurements
6.1Measurements & Errors
6.2Uncertainties & Errors
6.3Vectors & Scalars
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