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Please use this identifier to cite or link to this item: http://localhost:80/xmlui/handle/123456789/1947
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dc.contributor.authorMian, Z.U.-
dc.contributor.authorQadir, Asghar-
dc.contributor.authorQuamar, Jawaid-
dc.date.accessioned2019-12-09T05:35:18Z-
dc.date.available2019-12-09T05:35:18Z-
dc.date.issued1989-01-01-
dc.identifier.issn11 115-
dc.identifier.urihttp://142.54.178.187:9060/xmlui/handle/123456789/1947-
dc.description.abstractAssuming that planets were formed in the equatorial plane of the Sun and that there was a small perturbation at the start, it is shown that relativistic effects could lead to the planetary orbit tilting observed. On the basis of this analysis, a prediction is made for the velocity of the planet Mercury out of its orbital 'plane'. This prediction is a lower limit. Further, this explanation may possibly provide a method for determining the solar angular momentum.en_US
dc.language.isoen_USen_US
dc.publisherChina Ocean Pressen_US
dc.subjectNatural Scienceen_US
dc.subjectPlanetary Orbitsen_US
dc.titleOn the Inclination of Planetary Orbitsen_US
dc.typeArticleen_US
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