The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
... a photonic 'fingerprint'. The picture of a star's spectral lines is its photo-spectrograph.
Elements have several spectral lines and although some lines may be the same between different elements most lines are not and the whole spectrum for each element is indeed unique.
... faster it moves away from us.
The spectral lines. Each element has a characteristic "fingerprint" in a spectrum.
Yes. If the star is moving away from the Earth, its spectral lines will shift towards the red end of the spectrum. If it is moving towards the Earth, its spectral lines will shift towards the violet end of the spectrum. This is due to Doppler effect.
The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
A molecule has additional spectral lines due to changes in its rotational and vibrational energies.
Chemical composition ;-)
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... a photonic 'fingerprint'. The picture of a star's spectral lines is its photo-spectrograph.
Elements have several spectral lines and although some lines may be the same between different elements most lines are not and the whole spectrum for each element is indeed unique.
Because the most important spectral lines of sodium are in the yellow region of the spectrum.
The red end of the spectrum.
The spectral lines. Each element has a characteristic "fingerprint" in a spectrum.
The spectral lines. Each element has a characteristic "fingerprint" in a spectrum.
... faster it moves away from us.