On Dec 20, 8:55 am, Ilya Zakharevich <nospam-ab... DeleteThis @ilyaz.org> wrote:
> [A complimentary Cc of this posting was sent to
> David Bernier
> <david... DeleteThis @videotron.ca>], who wrote in article <T_kaj.6427$Bw2.501...@weber.videotron.net>:
>
> > Currently, effects from general relativity are included by JPL and
> > others. Trying to understand solar dynamics formulated
> > in general relativity is beyond me.
>
> I'm very sure that (maybe with an exception of Mercury; but I think
> even for it) the main term of the effects of GR can be expressed as
> minor additions to Newton inverse square law (a term of degree not
> -2, + a term depending on relative velocity). (I do not have a
> reference at hand, but I think it is in the beginning of any book on GR...)
I am pretty sure that the advance of the perihelion of mercury can be
accurately calculated from an eqn of motion that differs from the
Newtonian one only by a term (or 2) like the ones you describe. The
reason I'm so sure is that the last written exam I ever took was GR,
and that was one of the questions
