Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3043
DC FieldValueLanguage
dc.contributor.authorKovačević, Anđelkaen_US
dc.date.accessioned2026-01-11T16:33:59Z-
dc.date.available2026-01-11T16:33:59Z-
dc.date.issued2006-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3043-
dc.description.abstractThe masses of the seven largest asteroids: (1) Ceres, (2) Pallas, (4) Vesta, (10) Hygiea, (52) Europa, (511) Davida and (704) Interamnia were determined from gravitational perturbations exerted on selected asteroids. These masses were calculated by means of the modified method. The procedure of the mass determination is based on calculation of perturbed orbit using observations which cover pre or post enco unter part of the orbit. Then the pre and post encounter parts of perturbed orbit has been linked by some chosen value for the mass of a perturbing body. The procedure is an iterative one. The resulting mass of the perturbing asteroid is obtained as one which provides the minimum O-C residuals in the RMS sense.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of the Astronomical Observatory of Belgradeen_US
dc.titleGravitational influence of asteroids and determination of their massesen_US
dc.typeConference Objecten_US
dc.relation.conferenceNational Conference of Astronomers of Serbia and Montenegro (14 ; 2005 ; Belgrade)en_US
dc.relation.publicationProceedings of the XIV National Conference of Astronomers of Serbia and Montenegroen_US
dc.identifier.isi000245309100030-
dc.identifier.urlhttps://publications.aob.rs/80/pdf/197-202.pdf-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage197en_US
dc.relation.lastpage202en_US
dc.relation.issue80en_US
item.openairetypeConference Object-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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