Difference between revisions of "Galilean Gravitation: Solar System Orbits"
Jump to navigation
Jump to search
(Imported from text file) |
(Imported from text file) |
||
(One intermediate revision by the same user not shown) | |||
Line 12: | Line 12: | ||
==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 19:34, 1 January 2017
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.