jonmtkisco
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Hi Wallace,
Jon
Apparently the explanation of this point wasn't clear in my post. I said:Wallace said:I don't quite follow this? How can the recession velocity 'at time of reception' of the distant galaxy be a factor? Once the photon leaves the emitting galaxy it doesn't know or care about what that galaxy does.
The reason for the attached diagram was to show that the equation must take account of the receiver's recessionary movement (away from the emission point) after the time of emission, but must NOT take account of the emitter's recessionary movement (away from the emission point) after that time. We are in agreement that what happens to the emitter after emission isn't relevant. A subtlety is required in order for the equation to accomplish this result from the data available, which after all does not distinguish between the recession of one party and the recession of the other party, since their recession is relative as between each other only. That's why I attribute 1/2 of the total post-emission recessionary movement to each party, rather than attribute the entire recessionary movement arbitrarily to just one of the parties.The equations divide by two in order to exclude the gravitational decrease in the emitter's proper recession velocity occurring place after the photon is emitted.
Jon
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