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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1217
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dc.contributor.authorKuzmanoski, Mikeen_US
dc.contributor.authorApostolovska, Gordanaen_US
dc.contributor.authorNovaković, Bojanen_US
dc.date.accessioned2022-09-23T17:59:40Z-
dc.date.available2022-09-23T17:59:40Z-
dc.date.issued2010-09-01-
dc.identifier.issn00046256-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1217-
dc.description.abstractIn this paper, we present a recalculated value of the mass of (4) Vesta, derived from its largest gravitational perturbations on selected asteroids during their mutual close encounters. This was done by using a new method for mass determination, which is based on the linking of pre-encounter observations to the orbit determined from post-encounter ones. The estimated weighted mean of the mass of (4) Vesta is (1.300 ± 0.001) ×10?10 M⊙. © 2010. The American Astronomical Society.en_US
dc.relation.ispartofAstronomical Journalen_US
dc.subjectAsteroids: generalen_US
dc.subjectMinor planetsen_US
dc.titleThe mass of (4) Vesta derived from its largest gravitational effectsen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-6256/140/3/880-
dc.identifier.scopus2-s2.0-78049236183-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/78049236183-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage880en_US
dc.relation.lastpage886en_US
dc.relation.volume140en_US
dc.relation.issue3en_US
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairetypeArticle-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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