Using the Doppler formula to find radial speed of a star

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SUMMARY

The discussion focuses on calculating the radial speed of a star using the Doppler formula. The observed wavelength of the Hα line is 656.250 nm, while the laboratory wavelength is 656.280 nm. By applying the formula Vr = (Δλ/λ0)c, where Δλ is the difference in wavelengths, the radial speed is determined to be 13.7 km/s. The units of Δλ and λ0 cancel out, confirming that the final velocity is expressed in km/s.

PREREQUISITES
  • Understanding of the Doppler effect in astrophysics
  • Familiarity with high-resolution spectroscopy
  • Knowledge of unit conversions, particularly between nanometers and kilometers per second
  • Basic proficiency in algebra for solving equations
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  • Study the principles of the Doppler effect in more detail
  • Learn about high-resolution spectroscopy techniques
  • Explore unit conversion methods in physics
  • Investigate other applications of the Doppler formula in astrophysics
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Astronomy students, astrophysicists, and anyone interested in understanding stellar motion and spectroscopy techniques.

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Homework Statement



High resolution spectroscopy reveals that the H line is located at a wavelength
of 656.250 nm for this star. The wavelength of H measured in the lab is 656.280 nm.
Calculate the line-of-sight velocity of the star.



Homework Equations



Here's the Doppler formula:

Vr = (Δλ/λ0)c

where Vr is the radial speed of the star, Δλ is the Doppler shift, λ0 is the rest wavelength or the wavelength measured in the lab, and c is the speed of light.



The Attempt at a Solution



I'm just having trouble with units. I need the answer (the radial speed of the star) in km/s, but i don't know what units to put the other variables (Δλ, λ0, c) in.
 
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λ= 656.28 nm
Δλ=656.28-656.25=.03 nm
c=3*108 m/s=3*105 km/s

so finally ,
v=13.7 km/s

The units of Δλ and λ cancel, so v has basically same units as c
 
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