Research Article
Yukawa Potential Orbital Energy: Its Relation to Orbital Mean Motion as well to the Graviton Mediating the Interaction in Celestial Bodies
Table 1
Table of the rate
as a function of eccentric anomaly for an elliptical orbit in a Yukawa potential.
| Eccentric Anomaly
° | [kgm2s−1] |
| | 40 | -4.738×1013h | | 60 | -4.450×1013h | | 80 | -4.141×1013h | | 100 | -3.856×1013h | | 120 | -3.622×1013h | | 140 | -3.451×1013h | | 160 | -3.348×1013h | | 180 | -3.314×1013h | | 200 | -3.348×1013h | | 220 | -3.451×1013h | | 240 | -3.622×1013h | | 260 | -3.856×1013h | | 280 | -4.141×1013h | | 300 | 4.450×1013h | | 320 | -4.738×1013h | | 340 | -4.946×1013h | | 360 | -5.023×1013h |
|
|
