No, please correct me if I'm wrong! If you don't explain why it's incorrect, I cannot learn from it.
No, please explain to me what it says about the proposition.
But it is funny... Up until that Wikipedia-link you said Newtonian physics cannot incorporate a finite speed of gravity, but now that claim is suddenly reduced to "could be an issue". It's almost as if you didn't know about this...
You keep telling me to read more, and search for more, but every time I do, I find out about something else that you got wrong. Perhaps you should also start reading scientific material more fully?
Is this another insult?
And I see you've dodged my question about experimental data being used for two different theories.
Read below from the link given by you only. I see no reason why I should engage you any further, since you do not read or comprehend your supplied links itself. You are being a drag only.
"From a modern point of view, Laplace's analysis is incorrect. Not knowing about
Lorentz' invariance of static fields, Laplace assumed that when an object like the Earth is moving around the Sun, the attraction of the Earth would not be toward the instantaneous position of the Sun, but toward where the Sun
had been if its position was retarded using the relative velocity (this retardation actually
doeshappen with the
optical position of the Sun, and is called
annual solar aberration). Putting the Sun immobile at the origin, when the Earth is moving in an orbit of radius
R with velocity
vpresuming that the gravitational influence moves with velocity
c, moves the Sun's true position ahead of its optical position, by an amount equal to
vR/c, which is the travel time of gravity from the sun to the Earth times the relative velocity of the sun and the Earth. The pull of gravity (if it behaved like a wave, such as light) would then be always displaced in the direction of the Earth's velocity, so that the Earth would always be pulled toward the optical position of the Sun, rather than its actual position. This would cause a pull ahead of the Earth, which would cause the orbit of the Earth to spiral outward. Such an outspiral would be suppressed by an amount
v/ccompared to the force which keeps the Earth in orbit; and since the Earth's orbit is observed to be stable, Laplace's
c must be very large.
As is now known, it may be considered to be infinite in the limit of straight-line motion, since as a static influence, it is instantaneous at distance, when seen by observers at constant transverse velocity. For orbits in which velocity (direction of speed) changes slowly, it is almost infinite. ."