MadSci Network: Astronomy |
Subject: Red Shift and Planck's equation As a Astronomy grad of almost thirty years ago, but still very much interested, this one has puzzled me for some time: When we observe a distant galaxy, we see specific characteristic spectral emissions 'red-shifted'. I assume the photons are emmitted at their original characteristic frequency as would be seen from a stationary source, say here on earth, i.e. 'further blue' than photons from distant galaxies. Since the energy of a photon is determined by Planck's constant multiplied by the frequency, what happens to the energy loss in the drop of frequency??? Alan J. Maloney
Re:Subject: Red Shift and Planck's equation
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