Astromony Q: Red Shift of 500nm Wavelength Line in Hydra Galaxy

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A distant galaxy in Hydra is receding from Earth at 6.12 x 10^7 m/s, prompting a question about the redshift of a green spectral line at 500nm. The relativistic Doppler effect is applied to calculate the shift, using the formula ν_obs/ν_source = √((1+β)/(1-β)), where β = v/c = 0.204. The discussion highlights the importance of the Doppler effect in understanding redshift phenomena. Additionally, a minor spelling correction from "astromony" to "astronomy" is noted. The conversation emphasizes the application of physics principles to astronomical observations.
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There's an astromony question that I'm stuck on~
" A distant galaxy in the constellation Hydra is receding from the Earth at 6.12*10^7 m/s. By how much is a green spectral line of wavelength 500nm (1nm=10^(-9) )emitted by this galaxy shifted toward the red end of the spectrum?
 
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what knowledge do you have?
 
asdf1 said:
There's an astromony question that I'm stuck on~
" A distant galaxy in the constellation Hydra is receding from the Earth at 6.12*10^7 m/s. By how much is a green spectral line of wavelength 500nm (1nm=10^(-9) )emitted by this galaxy shifted toward the red end of the spectrum?

Just use the relativistic doppler effect:

\nu_{obs}/\nu_{source} = \sqrt{\frac{1+\beta}{1-\beta}}

where \beta = v/c = .204 and \nu_{source} = c/\lambda_{source}

AM
 
How did you think of to use the Doppler effect?
 
Probably because the question is about the Doppler effect (well, it's about red shift, which is to do with the Doppler effect). Also, you mean "astronomy", not "astromony".
 
I see~
Thanks for correcting my spelling mistake!
 
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