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## PowerPoint Slideshow about 'The Doppler Shift' - bertha

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### The Doppler Shift

Brought to you by McCourty-Rideout enterprises- tuned into your frequency

image is courtesy of Windows to the Universe, http://www.windows.ucar.edu.

Astronomy and the Doppler Shift http://www.windows.ucar.edu.

- Astronomers can measure the Doppler Shift of a moving object.
- The radio wave has a known frequency for stationary objects.
- If target is moving away, waves in the signal will be stretched, and will have a lower frequency.
- If the target is moving closer, waves will be compressed and will have a higher frequency.
- For more information and a cool video click:

DYK??? http://www.windows.ucar.edu.

- Police radar guns transmit a continuous wave. The radar gun compares the frequency of the wave reflected (the echo) from the moving vehicle to the frequency of the transmitted wave from the gun, and displays the vehicle's computed speed.

Doppler Formula http://www.windows.ucar.edu.

The Doppler shift formula for a moving source:

where λ1 is the unshifted wavelength

λ2 is the shifted wavelength

c is the speed of light and

v is the velocity of the object emitting the light, relative to the observer

Let’s Try An Example http://www.windows.ucar.edu.

- A spectral line normally at 4000 angstroms is shifted to 3999 angstroms because of the motion of the source. What is the velocity of the source, along the line of sight?

Solve for v: http://www.windows.ucar.edu.

= [(3999 – 4000)/4000]•3 x 108

= -7.5 x 104 m/s

Is the source coming towards us or away from us?

Towards us! http://www.windows.ucar.edu.

The Doppler shift is called a

“Red shift” if v > 0 (moving away) since the wavelength is getting longer and the frequency shorter

“Blue Shift” if v < 0 (moving closer) since the wavelength is getting shorter and the frequency higher

(recall that blue light is higher in frequency than red)

To try another example click here. http://www.windows.ucar.edu.

If not proceed to the next slide.

Uses of the Doppler Shift http://www.windows.ucar.edu.

- Radio astronomers can find the motion of a source (stars, galaxies, gases, etc.) by observing whether the emission or absorption lines in its spectrum are shifted in wavelength relative to their wavelengths at rest

A typical passive http://www.windows.ucar.edu.radar system.The range and Doppler shift can determined

Doppler Shift in Action http://www.windows.ucar.edu.

- A telescope in both the US and Japan will have different velocities with respect to a galaxy they are observing since the signal received at each antenna is characterized by a Doppler shift that depends on the relative position and motion of the antenna and the signal source

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