| 摘要 |
A method for determining the orbit of a planet comprises the initial step of empirical determination of 6, where 6 is the difference between the vernal to autumn equinox and the autumnal to vernal equinox. This is followed by empirical determination of planetary velocity and/or planetary radius. Comparisons of the empirical data with calculations based on cycloid orbit are then used to determine the planets orbit. |
