Ibn al-Ha'im's Trepidation Model

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dc.contributor.authorComes, Mercè (Comes Maymó), 1949-2010
dc.date.accessioned2016-04-28T12:47:13Z
dc.date.available2016-04-28T12:47:13Z
dc.date.issued2001
dc.date.updated2016-04-28T12:47:18Z
dc.description.abstractThe aim of trepidation models was to account for two phenomena that puzzled medieval astronomers: the secular decrease of the obliquity of the ecliptic, and the apparent changes in the velocity of precession over the years.
dc.format.extent118 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec195885
dc.identifier.issn1576-9372
dc.identifier.urihttps://hdl.handle.net/2445/97991
dc.language.isoeng
dc.publisherUniversitat de Barcelona
dc.relation.isformatofReproducció del document publicat a: http://www.raco.cat/index.php/Suhayl/article/view/199592
dc.relation.ispartofSuhayl. Journal for the History of the Exact and Natural Sciences in Islam, 2001, vol. 2, p. 291-408
dc.rightscc-by-nc-nd (c) Comes, Mercè (Comes Maymó), 1949-2010, 2001
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es
dc.sourceArticles publicats en revistes (Filologia Clàssica, Romànica i Semítica)
dc.subject.classificationAstronomia àrab
dc.subject.classificationAstronomia antiga
dc.subject.classificationAstronomia medieval
dc.subject.otherArab astronomy
dc.subject.otherAncient astronomy
dc.subject.otherMedieval astronomy
dc.titleIbn al-Ha'im's Trepidation Model
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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