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TeethWhitener
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Start here:kelly0303 said:What I meant is that, as far as I know, that idea was not heavily developed into a solid mathematical formulation (if it was and I am not aware of it, I would like to read some papers about it). For example, when the light curves of the galaxies were not what we expected, we didn't say: "oh it's just some matter we can't see, let's move on". The scientific community came up with thousands of theoretical models trying to explain it, and hundreds of experiments to test it. I am not aware of this with Mercury precession. Again, if I am wrong please show me attempts to solve that problem (I am actually really interested in that, I just didn't find anything). Thank you!
https://en.wikipedia.org/wiki/Vulcan_(hypothetical_planet)
plus links therein. Clemence's Rev. Mod. Phys. article gives some pertinent observations:
So it looks like there was a solid 70 years of experimental and theoretical work before Einstein's general relativity took care of the problem of Mercury's precession. A propos of nothing, Vera Rubin's first paper on dark matter came out almost 50 years ago.Clemence said:In justice it should be said that the questions involved are not simple ones, but are complicated by three causes: (1) Observations of Mercury are among the most difficult in positional astronomy. They have to be made in the daytime, near noon, under unfavorable conditions of the atmosphere; and they are subject to large systematic and accidental errors arising both from this cause and from the shape of the visible disk of the planet. (2) The planet's path in Newtonian space is not an ellipse but an exceedingly complicated space-curve due to the disturbing effects of all of the other planets. The calculation of this curve is a difficult and laborious task, and significantly different results have been obtained by different computers. (3) The observations cannot be made in the Newtonian frame of reference. They are referred to the moving equinox, that is, they are affected by the precession of the equinoxes, and the determination of the precessional motion is one of the most difficult problems of positional astronomy, if not the most difficult. In the light of all these hazards it is not surprising that a difference of opinion could exist regarding the closeness of agreement between the observed and theoretical motions.