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One of the strongest emission lines observed from distant galaxies comes from hydrogen and has a wavelength of 122 nm (in the ultraviolet region). (a) How fast must a galaxy be moving away from us in order for that line to be observed in the visible region at 366 nm

Respuesta :

Answer:

[tex]v=2.4*10^8m/s[/tex]

Explanation:

From the question we are told that

Wavelength of emission [tex]\lambda=122nm[/tex]

Observation distance [tex]d=366nm[/tex]

Generally the s equation is given as

[tex]f'=f\sqrt{\frac{(1-\frac{v}{c} )}{1+\frac{v}{c} }[/tex]

where

F is inversely proportional to T

[tex]d=\lambda\sqrt{\frac{(1-\frac{v}{c} )}{1+\frac{v}{c} }[/tex]

[tex]\frac{v}{c} =\frac{(1-\frac{\lambda}{d})}{(1+\frac{\lambda}{d}}[/tex]

[tex]\frac{v}{c}=\frac{1-(\frac{122}{366} )^2}{1+(\frac{122}{366})^2}[/tex]

[tex]\frac{v}{c}=\frac{0.8888888889}{1.11111111}[/tex]

[tex]\frac{v}{c}=0.80[/tex]

[tex]v=0.80*3*10^6[/tex]

[tex]v=2.4*10^8m/s[/tex]

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