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http://142.54.178.187:9060/xmlui/handle/123456789/1947Full metadata record
| DC Field | Value | Language |
|---|---|---|
| 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 |
| Appears in Collections: | Journals | |
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