Galilean Gravitation: Solar System Orbits: Difference between revisions
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| published = 1993 | | published = 1993 | ||
| journal = [[Galilean Electrodynamics]] | | journal = [[Galilean Electrodynamics]] | ||
| volume = | | volume = 4 | ||
| number = | | number = 3 | ||
| pages = 43-46 | | pages = 43-46 | ||
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==Abstract== | ==Abstract== | ||
The formalism obtained in [2] was defined up to a scalar field. This paper indicates how to fix this field in an approximate manner and apply the resulting approximately defined formalism to calculate orbital periods of solar system planets. | The formalism obtained in [2] was defined up to a scalar field. This paper indicates how to fix this field in an approximate manner and apply the resulting approximately defined formalism to calculate orbital periods of solar system planets. | ||
[[Category:Gravity]] | [[Category:Scientific Paper|galilean gravitation solar orbits]] | ||
[[Category:Gravity|galilean gravitation solar orbits]] | |||
Latest revision as of 09:29, 21 July 2026
| Scientific Paper | |
|---|---|
| Title | Galilean Gravitation: Solar System Orbits |
| Author(s) | David F Roscoe |
| Keywords | scalar field, orbital periods, solar system planets |
| Published | 1993 |
| Journal | Galilean Electrodynamics |
| Volume | 4 |
| Number | 3 |
| Pages | 43-46 |
Abstract
The formalism obtained in [2] was defined up to a scalar field. This paper indicates how to fix this field in an approximate manner and apply the resulting approximately defined formalism to calculate orbital periods of solar system planets.