On the Perihelion Precession of Solar Planetary Orbits

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dc.contributor.authorNyambuya, G. G.
dc.date.accessioned2014-12-17T07:24:20Z
dc.date.accessioned2023-06-26T13:01:49Z
dc.date.available2014-12-17T07:24:20Z
dc.date.available2023-06-26T13:01:49Z
dc.date.issued2013-02
dc.descriptionThis is an articleen_US
dc.description.abstractThe present letter presents an improved version of the Azimuthally Symmetric Theory of Gravitation (ASTG-model) which was presented for the first time in the present journal four years ago. We propose a solution to the standing problem of the -parameters in which effort we put the ASTG-model on a clear pedestal for falsification. As in the maiden reading, the perihelion precessional data of Solar planetary orbits is used to set the theory into motion.en_US
dc.identifier.citationNyambuya, G.G., 2013. On the Perihelion Precession of Solar Planetary Orbits.en_US
dc.identifier.urihttp://ir.nust.ac.zw:4000/handle/123456789/457
dc.language.isoenen_US
dc.rights.licenseThis article was downloaded from NUST Institutional repository, and is made available under the terms and conditions as set out in the Institutional Repository Policy.en_US
dc.subjectplanetary orbiten_US
dc.subjectperihelion shiften_US
dc.subjectsolar spinen_US
dc.titleOn the Perihelion Precession of Solar Planetary Orbitsen_US
dc.typeArticleen_US

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