On the Inclination of Planetary Orbits

dc.contributor.author	Mian, Z.U.
dc.contributor.author	Qadir, Asghar
dc.contributor.author	Quamar, Jawaid
dc.date.accessioned	2019-12-09T05:35:18Z
dc.date.available	2019-12-09T05:35:18Z
dc.date.issued	1989-01-01
dc.identifier.issn	11 115
dc.identifier.uri	http://142.54.178.187:9060/xmlui/handle/123456789/1947
dc.description.abstract	Assuming 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.iso	en_US	en_US
dc.publisher	China Ocean Press	en_US
dc.subject	Natural Science	en_US
dc.subject	Planetary Orbits	en_US
dc.title	On the Inclination of Planetary Orbits	en_US
dc.type	Article	en_US