Please use this identifier to cite or link to this item: https://open.uns.ac.rs/handle/123456789/2543
DC FieldValueLanguage
dc.contributor.authorStoiljković, Dragoslaven_US
dc.date.accessioned2019-09-23T10:22:14Z-
dc.date.available2019-09-23T10:22:14Z-
dc.date.issued2014-01-01-
dc.identifier.isbn9788680019802en_US
dc.identifier.urihttps://open.uns.ac.rs/handle/123456789/2543-
dc.description.abstractSavich and Kashanin in 1960-Ties developed a mathematical model to calculate the mean density of solar planets. The model used van der Waals (vdW) equation of state for real gases, from which it follows that the volume of a substance at absolute zero temperature (V0) is one third of volume at critical point (Vj, i.e. V0=Vc/3. However, empirical data published more recently confirmed that V0=Vc/4. Using this empirical fact we modified mathematical model of Savich and Kashanin thus enabling the more correct calculation of planet's mean densities.en
dc.relation.ispartofProceedings of the XVII National Conference of Astronomers of Serbiaen
dc.titleCalculation of mean density of solar planets by modified savich-kashanin methoden_US
dc.typeConference Paperen_US
dc.identifier.scopus2-s2.0-85040651691-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85040651691-
dc.description.versionUnknownen_US
dc.relation.lastpage111en
dc.relation.firstpage105en
item.fulltextNo Fulltext-
item.grantfulltextnone-
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