JohnnyGui
- 796
- 51
Adrian59 said:This has been an interesting thread for me and I have had to re-examine the assumptions that the graph of magnitude v red shift make which has been a large part of the discussion. I still think that your graph is very similar to the one Saul Pelmutter used in his famous paper and this was taken as a true reflection of distance v receding velocity. I did come to a similar conclusion to yourself wrt this graph and I still don't quite know what the answer is.
The way I understood it is by realising that the graph in my OP is a measure of redshifts at one moment in time (all redshifts measured at once).
Therefore, one would have to consider a scenario in which you measure the 2 redshifts of 2 lights both at once, one from a nearby star ##A## and another from a very far star ##B##. To be able to measure them at once, you'd first have to calculate the new distance and velocity of star ##A## at the time at which the light of star ##B## passes star ##A## itself, during an acceleration. It's a quadratic formula in which you have to solve for the time duration until the light of star ##B## passes star ##A## (let's call that moment ##T_A##). So star ##A## is approaching the light of star ##B## while accelerating while star ##B##'s light is approaching star ##A## at ##c##
Once you have calculated the new velocity and distance of star ##A## at ##T_A##, you can calculate star ##A##'s redshift by calculating how much distance star ##A## has traveled from ##T_A## (with acceleration) until its light reaches the Earth and divide that by the distance of star ##A## at ##T_A##. Also, you can calculate the redshift of star ##B##'s light that was emitted before ##T_A## (it's the light that passed star ##A## at ##T_A##) at ##T_B## by calculating how much distance star ##B## has traveled from ##T_B## all up until it reached the earth, divided by the initial distance of star ##B##.
You should get 2 redshifts that are not proportional with distance, such that the redshift of star ##B## is actually less than one would expect with the Hubble value deduced from star ##A##'s redshift. I'm aware there are many factors into play but this is a basic concept that shows a simple case of the relation between redshift and acceleration. For more info on the calculation, see my post #15.
Last edited: