Do we get from the most distant galaxies mostly the spectral lines of heavy elements or of light elements?
The thought behind my question is that on our time axis, the nuclear reactions on bodies moving with velocities close to c, should be much slower: Δt = τ / (1 - v2/c2)1/2, where Δt is the time on the Earth' time axis, τ is the reaction duration in the rest-frame, and v is the velocity with which we suppose that the star recedes from us.
Can we use these issues for cheching whether indeed the far galaxies recede from us and the space-time expands?
(Note: there was an ERROR here. Thanks to Remi and Paul I corrected it.)