{"@context":{"dc":"http:\/\/purl.org\/dc\/elements\/1.1\/","skos":"http:\/\/www.w3.org\/2004\/02\/skos\/core#","skos:broader":{"@type":"@id"},"skos:inScheme":{"@type":"@id"},"skos:related":{"@type":"@id"},"skos:narrower":{"@type":"@id"},"skos:hasTopConcept":{"@type":"@id"},"skos:topConceptOf":{"@type":"@id"}},"@id":"http:\/\/tematres.nb.no\/norvok\/skos421","@type":"skos:Concept","skos:prefLabel":{"@language":"nb","@value=":"Deklinasjon"},"skos:inScheme":"http:\/\/tematres.nb.no\/norvok","dct:created":"2022-06-16 10:47:34","skos:definition":[{"@lang":"no","@value":"\n\n\nDeklinasjon (astronomi) er et himmellegemes vinkelavstand fra\u00a0himmelekvator, m\u00e5lt langs en\u00a0storsirkel\u00a0(deklinasjonssirkel) gjennom himmellegemet og himmelpolene.\n\n\n "}]}