On the Emmenthal distribution of highly inclined asteroids

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T13:28:04Z
dc.date.accessioned2022-10-05T13:24:46Z
dc.date.available2014-05-20T13:28:04Z
dc.date.available2022-10-05T13:24:46Z
dc.date.created2014-05-20T13:28:04Z
dc.date.issued2011-12-01
dc.identifierMonthly Notices of The Royal Astronomical Society. Malden: Wiley-blackwell, v. 418, n. 2, p. 1102-1114, 2011.
dc.identifier0035-8711
dc.identifierhttp://hdl.handle.net/11449/9306
dc.identifier10.1111/j.1365-2966.2011.19576.x
dc.identifierWOS:000297987400032
dc.identifierWOS000297987400032.pdf
dc.identifier4750709016042276
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3885717
dc.description.abstractHighly inclined asteroids are objects with sin (i) > 0.3. Among highly inclined asteroids, we can distinguish between objects with inclinations smaller than that of the centre of the ?6= g - g6 secular resonance and objects at higher inclinations. Using the current mechanisms of dynamical mobility, it is not easy to increase the values of an asteroid with an initial small inclination to values higher than that of the centre of the ?6 resonance. The presence of highly inclined objects might therefore be related to the early phases of the Solar system.
dc.languageeng
dc.publisherWiley-Blackwell
dc.relationMonthly Notices of the Royal Astronomical Society
dc.relation5.194
dc.relation2,346
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectcelestial mechanics
dc.subjectminor planets, asteroids: general
dc.titleOn the Emmenthal distribution of highly inclined asteroids
dc.typeArtigo


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