The three famous Kepler laws are given in this Note for m theory. Kepler’s first law is that an orbit is an ellipse. This is changed completely using Eqs. (1) and (2), giving forward and retrograde precession, shrinking and expanding orbits and so on. Of particular interest is Kepler’s third law, Eq. (22), because the last note made the major discovery that the Newton theory in S2 is wildly wrong. In the m theory the central mass about which the S2 orbits is not a black hole, it is given by Eq. (35). By using Eq. (33) it is possible to find the time T for one orbit self consistently. Currently co author Horst Eckardt is working towards the same goal using a different method.

a419thpapernotes4.pdf

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