@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix dc: <http://purl.org/dc/terms/> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

<http://astrothesaurus.org/uat/999>
  skos:prefLabel "Magnitude"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/10> .

<http://astrothesaurus.org/uat/10>
  skos:editorialNote [ ] ;
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie>, <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin> ;
  skos:broader <http://astrothesaurus.org/uat/999> ;
  skos:prefLabel "Absolute magnitude"@en ;
  skos:definition "The magnitude a star would have if it were at a distance of 10 parsecs in a void space, without interstellar absorption. The absolute magnitude is usually deduced from the visual magnitude, measured through a V filter (UBV system), when it is written as M_V. If it is defined for another wavelength, it gets another index (U, B, etc). If the radiation on all wavelengths is included, it becomes absolute bolometric magnitude, M_bol. The Sun has the absolute magnitude +4.8. Most of the stars have absolute magnitudes ranging between -9 (supergiants) and +19 (red dwarfs)."@en ;
  dc:modified "2020-12-16T20:48:12.505Z"^^xsd:dateTime, "2020-11-03T17:44:54.488Z"^^xsd:dateTime ;
  a skos:Concept .