One of the wavelengths of light emitted by hydrogen atoms under normal laboratory conditions is λ = 656.3 nm, in the red portion of the electromagnetic spectrum. In the light emitted from a distant galaxy this same spectral line is observed to be Doppler-shifted to λ = 953.4 nm, in the infrared portion of the spectrum. How fast are the emitting atoms moving relative to the earth? Are they approaching the earth or receding from it?
One of the wavelengths of light emitted by hydrogen atoms under normal laboratory conditions is λ = 656.3 nm, in the red portion of the electromagnetic spectrum. In the light emitted from a distant galaxy this same spectral line is observed to be Doppler-shifted to λ = 953.4 nm, in the infrared portion of the spectrum. How fast are the emitting atoms moving relative to the earth? Are they approaching the earth or receding from it?
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One of the wavelengths of light emitted by hydrogen atoms under normal laboratory conditions is λ = 656.3 nm, in the red portion of the
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