Difference between revisions of "Newton?s Equations of Motion in the Gravitational Field of an Oblate Mass"
Jump to navigation
Jump to search
(Imported from text file) |
(Imported from text file) |
||
| Line 13: | Line 13: | ||
In an earlier paper [1], we derived Newton?s gravitational scalar potential field due to an oblate spheroidal massive body. In this paper we derive the corresponding Newton?s equations of motion for a particle of nonzero rest mass in the Gravitational Field of a stationary, homogeneous, oblate spheroidal massive body, expressed in oblate spheroidal coordinates convenient for mathematical investigation, and hence physical interpretation and experimental investigation for all systems in the Universe. | In an earlier paper [1], we derived Newton?s gravitational scalar potential field due to an oblate spheroidal massive body. In this paper we derive the corresponding Newton?s equations of motion for a particle of nonzero rest mass in the Gravitational Field of a stationary, homogeneous, oblate spheroidal massive body, expressed in oblate spheroidal coordinates convenient for mathematical investigation, and hence physical interpretation and experimental investigation for all systems in the Universe. | ||
| − | [[Category:Scientific Paper]] | + | [[Category:Scientific Paper|newton s equations motion gravitational field oblate mass]] |
[[Category:Gravity]] | [[Category:Gravity]] | ||
Revision as of 10:45, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Newton?s Equations of Motion in the Gravitational Field of an Oblate Mass |
| Author(s) | S X K Howusu, E F Musongong |
| Keywords | {{{keywords}}} |
| Published | 2006 |
| Journal | Galilean Electrodynamics |
| Volume | 17 |
| Number | 3 |
| Pages | 57-59 |
Abstract
In an earlier paper [1], we derived Newton?s gravitational scalar potential field due to an oblate spheroidal massive body. In this paper we derive the corresponding Newton?s equations of motion for a particle of nonzero rest mass in the Gravitational Field of a stationary, homogeneous, oblate spheroidal massive body, expressed in oblate spheroidal coordinates convenient for mathematical investigation, and hence physical interpretation and experimental investigation for all systems in the Universe.
