Kinematic Description of Solar System Dynamics from Position Observables Alone (Paper I of the SSEG Series)

We demonstrate that all solar system dynamics are fully

determined by positional observables alone, without

presupposing masses or a reference frame. Eight observables

O1–O8 are defined and measured. The kinematic weights

coincide with Newtonian masses to 0.013% (H3). Bootstrap

confidence intervals confirm all results at 95%.

Paper I of five.