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Q. In hydrogen spectrum the wavelength of $H_\alpha$ line is 656 nm; whereas in the spectrum of a distant galaxy $H_\alpha$ line wavelength is 706 nm. Estimated speed of galaxy with respect to earth is

IIT JEEIIT JEE 1999

Solution:

Since, the wavelength $(\lambda)$ is increasing, we can say that the galaxy is receding. Doppler effect can be given by
$\lambda =\lambda \sqrt{\frac{c+v}{c-v}}$...(i)
or $706=656\sqrt{\frac{c+v}{c-v}}$ or $\frac{c+v}{c-v}=\bigg(\frac{706}{656}\bigg)^2=1.16$ $\therefore c+v-1.16c-1.16v$ $v=\frac{0.16c}{2.16}=\frac{0.16\times3.0\times10^8}{2.16}=0.22\times10^8 m/s$ $v\approx2.2\times10^7 m/s$ If we take the approximation then Eq. (i) can be written as $\Delta\lambda=\lambda\bigg(\frac{v}{c}\bigg)$...(ii) From here $v=\bigg(\frac{\Delta\lambda}{\lambda}\bigg),c=\bigg(\frac{706-656}{656}\bigg)(3\times10^8)$ $v=0.23\times10^8 m/s$ Which is almost equal to the previous answer. So, we may use Eq. (ii) also.