The change in the received frequency due to the Doppler shift can be written as follows:
"\\omega = \\frac{\\omega_0}{1 + \\frac{v}{c}}" ,
where we take into account the fact that the star is receding from the observer. Hence,
"v=c\\left(\\frac{\\omega_0}{\\omega}-1\\right)" .
Utilizing the relationship between the angular velocity and wavelength "\\lambda = \\frac{2 \\pi c}{\\omega}" , we derive:
"v=c\\left( \\frac{\\lambda}{\\lambda_0}-1\\right)=c \\left(\\frac{\\lambda_0 + \\Delta \\lambda}{\\lambda_0}-1\\right) = c \\frac{\\Delta \\lambda}{\\lambda_0}"
Substituting the numerical values, we obtain (answer is measured in the number of speed of light):
"v = c \\frac{100}{5890} \\approx 0.017c"
or substituting the speed of light:
"v \\approx 5.1 \\times 10^6" m/s
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