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![]() Henri Wilson wrote: How does the light know that it should adjust its speed relative to the barycentre rather than something else? In actual fact light only 'knows' of one object, its own source. Theoretically the source could be the only object in the universe. The best reference for a change in speed is the source itself. That is what I expected. Since I am discussing the unification of light speed from the star over a complete orbit, I am suggesting that its barycentre is the most practical reference to use. It is not the only reference one could use. I agree. My questions were about the behavior of the light, as you discuss next, rather than choice of reference. How does the light determine its speed relative to the barycentre of the system it has left? It leaves at between c+v and c-v in the observer direction, wrt the orbit centre. I'm saying, that in time, it unifies to something like c wrt that centre. Don't ask me how or why... but this seems to happen in varying amounts according to the BaTh. It is most astonishing. Light from the star adjusts its speed relative to something with which it has no connection. If the light came only from the far side of the orbit, would it unify relative to the mean radial speed during that half-orbit, instead of unifying relative to the mean radial speed over the full orbit? I presume it unifies to the mean, rather than the median. Is that correct? Would light leaving the Moon toward a distant viewer unify its speed to c relative to the Earth-Moon barycentre or to the Moon-Sun barycentre? For a three body system, The radial velocity would be something like c+Acos(xt)+Bcos(yt). The max amd min are c+A+B and c-A-B. That seems reasonable. So I presume there would be two separate unification processes occuring simultaneously at different rates. The A would go towards zero over relatively short distances followed by the B over larger distances. So light from the Moon would tend to unify relative to the Earth-Moon barycentre, and then tend to unify relative to the Moon-Sun barycentre. It is a puzzle how the light could seem to know that it was emitted from a body which is orbiting other bodies. And it is a puzzle how the light could seem to know its speed relative to the different barycentres. I say this because unification rate appears to be dependent on orbit period. Don't ask me why. There could be an entirely different explanation as to why the hipparcos distances are generally longer than those I need to match brightness curves. The obvious relationship is that the shorter the orbit period, the higher the radial speed, and thus the greater the initial bunching effect, so the unification distance needs to be shorter in order to prevent excessive bunching during transit. Leonard |
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