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What is the Doppler effect? Explain, with the aid of labelled diagrams, how this phenomenon occurs - Leaving Cert Physics - Question 7 - 2007

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What is the Doppler effect? Explain, with the aid of labelled diagrams, how this phenomenon occurs. The emission line spectrum of a star was analysed using th... show full transcript

Worked Solution & Example Answer:What is the Doppler effect? Explain, with the aid of labelled diagrams, how this phenomenon occurs - Leaving Cert Physics - Question 7 - 2007

Step 1

What is the Doppler effect?

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Answer

The Doppler effect refers to the apparent change in frequency (or wavelength) of a wave in relation to an observer moving relative to the source of the wave. This effect occurs due to the relative motion between the source and observer, which can be seen when the source is either approaching or receding.

Explanation with Diagrams

  1. Non-concentric Circles: When the source of the wave is stationary and the observer is moving, the waves are bunched up in front of the observer (if the observer is approaching) or spread out behind (if the observer is moving away).

  2. Source and Direction of Motion: Indicate the direction in which the source is moving and the direction of the observer.

  3. Position of Observer Indicated: An appropriate diagram can highlight how the distance between wavefronts changes based on the motion of the source or observer.

  4. Change in Wavelength/Frequency: Moving towards the observer causes shorter wavelengths (higher frequency), while moving away causes longer wavelengths (lower frequency).

Step 2

Describe how an emission line spectrum is produced.

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Answer

An emission line spectrum is produced when a gas is heated or energized, causing its atoms to become excited to higher energy levels. This energy can be supplied by heating the gas via electrical discharge (as in hydrogen discharge tubes) or by other means.

Steps in Spectrum Production

  1. Atom Excitation: The atom absorbs energy and an electron is excited to a higher energy state.

  2. Electron Transition: The electron eventually returns to its lower energy state, releasing energy in the form of electromagnetic radiation (light).

  3. Spectroscopy: When observed with a spectrometer, the emitted light is dispersed and forms a spectrum, displaying specific wavelengths corresponding to the energies of the transitions.

  4. Characteristics of Spectrum: The result is a series of bright lines on a dark background, corresponding to the specific frequencies of emitted radiation, characteristic of the element.

Step 3

Is the star approaching the earth? Justify your answer.

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Answer

To determine if the star is approaching the Earth, we must compare the observed wavelength of the red line (720 nm) to the laboratory wavelength (656 nm).

Analysis

  • The original wavelength is 656 nm, while the observed wavelength is longer at 720 nm.
  • According to the Doppler effect, if the wavelength has increased, this indicates that the source is moving away from the observer (the Earth, in this case).

Conclusion

Thus, we can conclude that the star is not approaching the Earth; instead, it is receding.

Step 4

(i) the frequency of the red line in the star’s spectrum

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Answer

To calculate the frequency of the red line:

Formula

The frequency can be calculated using the formula: f=cλf = \frac{c}{\lambda} where:

  • c=3.00×108ms1c = 3.00 \times 10^8 m s^{-1} (speed of light)
  • λ=720×109m\lambda = 720 \times 10^{-9} m (convert nm to m)

Calculation

Substituting the values: f=3.00×108720×109=4.17×1014Hzf = \frac{3.00 \times 10^8}{720 \times 10^{-9}} = 4.17 \times 10^{14} Hz

Step 5

(ii) the speed of the moving star

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Answer

To calculate the speed of the moving star, we use the Doppler shift understanding that for a distant star moving away:

Formula

Using the Doppler effect approximation: v=c((λobservedλrest)λrest)v = c \left( \frac{(\lambda_{observed} - \lambda_{rest})}{\lambda_{rest}} \right) where:

  • λobserved=720nm\lambda_{observed} = 720 \, nm
  • λrest=656nm\lambda_{rest} = 656 \, nm
  • c=3.00×108m/sc = 3.00 \times 10^8 \: m/s

Substitution

Substituting the values: v=3.00×108(720656656)v = 3.00 \times 10^8 \left( \frac{720 - 656}{656} \right)

Calculation

This gives: v2.92×102m/sv \approx 2.92 \times 10^2 \: m/s

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