A pulsating star emits light whose frequency in a laboratory is fs = 6.782 x 1014 Hz. The star is in a distant galaxy far from Earth and the same light, 1014 Hz. What is to an observer on Earth, appears to have a frequency of f. = 6.483 the relative speed, Vrel, of this galaxy with respect to Earth in km/s?
A pulsating star emits light whose frequency in a laboratory is fs = 6.782 x 1014 Hz. The star is in a distant galaxy far from Earth and the same light, 1014 Hz. What is to an observer on Earth, appears to have a frequency of f. = 6.483 the relative speed, Vrel, of this galaxy with respect to Earth in km/s?
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