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dc.contributor.author | Habibullin S. | |
dc.date.accessioned | 2018-09-17T21:44:09Z | |
dc.date.available | 2018-09-17T21:44:09Z | |
dc.date.issued | 1992 | |
dc.identifier.issn | 0167-9295 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/135363 | |
dc.description.abstract | The method of estimation of the limits, containing the equator inclination of a celestial body, had been developed. In this method it is necessary to know the orbital elements and the mass of a celestial body. Another condition is that the axial rotation of a body should be in the resonance with its orbital motion. It has been found that the equator inclinations should have the values between 1 ‡.7 and 2 ‡.6 for Mercury and between 1 ‡.0 and 1 ‡.8 for the Moon. It also has been found that largest harmonics in Mercury's physical libration are the harmonics sin(Φ - 3 g), cos(Φ - 3 g), sin g and sin 2Ω. © 1992 Kluwer Academic Publishers. | |
dc.relation.ispartofseries | Earth, Moon and Planets | |
dc.title | The limits of possible values of inclination of Mercury's equator | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 58 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 79 | |
dc.source.id | SCOPUS01679295-1992-58-1-SID0027041108 |