Captain Swoop,

This is the summary of the gravity equations:

F=G x Mm/r^n where "n" = 2^ 1 + (plus) cr./ar. for the "inside range" of gravity for stallar sized bodies and for the "outside range;"
where n = 2^ 1 - (minus) cr./ar for groups of stars, galaxies and galaxy clusters structures. These are simple vector division tensor equations. All combined vector forces of this pushing gravity model are Newtonian. Additionally there are "e" factor equations for redshifts greater than 1 that effect what we will observe at these distances. These can be found on pages 101 - 102A. The null effect condition for the first equation is Newtonian gravity, and the limit of the second equation is equivalent to MOND gravity. The use of these equations always would consist of at least two equations for stellar systems and many for complicated best-fit modeling of galaxy structures.

respectfully, forrest