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RDF/XML
<rdf:RDF
xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#"
xmlns:j.0="http://qudt.org/schema/qudt/"
xmlns:j.1="http://purl.org/dc/terms/"
xmlns:owl="http://www.w3.org/2002/07/owl#"
xmlns:rdfs="http://www.w3.org/2000/01/rdf-schema#"
xmlns:xsd="http://www.w3.org/2001/XMLSchema#" >
<rdf:Description rdf:about="http://qudt.org/vocab/unit/SolarMass">
<j.0:conversionMultiplierSN rdf:datatype="http://www.w3.org/2001/XMLSchema#double">1.988435E30</j.0:conversionMultiplierSN>
<j.0:omUnit rdf:resource="http://www.ontology-of-units-of-measure.org/resource/om-2/solarMass"/>
<j.1:description rdf:datatype="http://qudt.org/schema/qudt/LatexString">The astronomical unit of mass is the solar mass.The symbol $S$ is often used in astronomy to refer to this unit, although $M_{\odot}$ is also common. The solar mass, $1.98844 \times 10^{30} kg$, is a standard way to express mass in astronomy, used to describe the masses of other stars and galaxies. It is equal to the mass of the Sun, about 333,000 times the mass of the Earth or 1,048 times the mass of Jupiter. In practice, the masses of celestial bodies appear in the dynamics of the solar system only through the products GM, where G is the constant of gravitation.</j.1:description>
<j.0:dbpediaMatch rdf:datatype="http://www.w3.org/2001/XMLSchema#anyURI">http://dbpedia.org/resource/Solar_mass</j.0:dbpediaMatch>
<rdf:type rdf:resource="http://qudt.org/schema/qudt/Unit"/>
<rdfs:isDefinedBy rdf:resource="http://qudt.org/2.1/vocab/unit"/>
<j.0:conversionMultiplier rdf:datatype="http://www.w3.org/2001/XMLSchema#decimal">1988435000000000000000000000000.0</j.0:conversionMultiplier>
<j.0:informativeReference rdf:datatype="http://www.w3.org/2001/XMLSchema#anyURI">http://en.wikipedia.org/wiki/Solar_mass?oldid=494074016</j.0:informativeReference>
<j.0:hasDimensionVector rdf:resource="http://qudt.org/vocab/dimensionvector/A0E0L0I0M1H0T0D0"/>
<j.0:symbol>S</j.0:symbol>
<rdfs:label xml:lang="en">Solar mass</rdfs:label>
<j.0:hasQuantityKind rdf:resource="http://qudt.org/vocab/quantitykind/Mass"/>
</rdf:Description>
</rdf:RDF>
TURTLE
@prefix owl: <http://www.w3.org/2002/07/owl#> .
@prefix rdf: <http://www.w3.org/1999/02/22-rdf-syntax-ns#> .
@prefix rdfs: <http://www.w3.org/2000/01/rdf-schema#> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .
<http://qudt.org/vocab/unit/SolarMass>
rdf:type <http://qudt.org/schema/qudt/Unit> ;
<http://purl.org/dc/terms/description> "The astronomical unit of mass is the solar mass.The symbol $S$ is often used in astronomy to refer to this unit, although $M_{\\odot}$ is also common. The solar mass, $1.98844 \\times 10^{30} kg$, is a standard way to express mass in astronomy, used to describe the masses of other stars and galaxies. It is equal to the mass of the Sun, about 333,000 times the mass of the Earth or 1,048 times the mass of Jupiter. In practice, the masses of celestial bodies appear in the dynamics of the solar system only through the products GM, where G is the constant of gravitation."^^<http://qudt.org/schema/qudt/LatexString> ;
<http://qudt.org/schema/qudt/conversionMultiplier> 1988435000000000000000000000000.0 ;
<http://qudt.org/schema/qudt/conversionMultiplierSN> 1.988435E30 ;
<http://qudt.org/schema/qudt/dbpediaMatch> "http://dbpedia.org/resource/Solar_mass"^^xsd:anyURI ;
<http://qudt.org/schema/qudt/hasDimensionVector> <http://qudt.org/vocab/dimensionvector/A0E0L0I0M1H0T0D0> ;
<http://qudt.org/schema/qudt/hasQuantityKind> <http://qudt.org/vocab/quantitykind/Mass> ;
<http://qudt.org/schema/qudt/informativeReference> "http://en.wikipedia.org/wiki/Solar_mass?oldid=494074016"^^xsd:anyURI ;
<http://qudt.org/schema/qudt/omUnit> <http://www.ontology-of-units-of-measure.org/resource/om-2/solarMass> ;
<http://qudt.org/schema/qudt/symbol> "S" ;
rdfs:isDefinedBy <http://qudt.org/2.1/vocab/unit> ;
rdfs:label "Solar mass"@en ;
.
JSON
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,"qname":"unit:SolarMass"
,"uri":"http:\/\/qudt.org\/vocab\/unit\/SolarMass"
,"properties":["conversion multiplier":"1988435000000000000000000000000.0"
,"conversion multiplier scientific":"1.988435E30"
,"dbpedia match":"http:\/\/dbpedia.org\/resource\/Solar_mass"
,"description":"The astronomical unit of mass is the solar mass.The symbol $S$ is often used in astronomy to refer to this unit, although $M_{\\odot}$ is also common. The solar mass, $1.98844 \\times 10^{30} kg$, is a standard way to express mass in astronomy, used to describe the masses of other stars and galaxies. It is equal to the mass of the Sun, about 333,000 times the mass of the Earth or 1,048 times the mass of Jupiter. In practice, the masses of celestial bodies appear in the dynamics of the solar system only through the products GM, where G is the constant of gravitation."
,"has dimension vector":"dimension:A0E0L0I0M1H0T0D0"
,"has quantity kind":"quantitykind:Mass"
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,"isDefinedBy":"<http:\/\/qudt.org\/2.1\/vocab\/unit>"
,"label":"Solar mass"
,"om unit":"<http:\/\/www.ontology-of-units-of-measure.org\/resource\/om-2\/solarMass>"
,"symbol":"S"
,"type":"qudt:Unit"
]}
JSON-LD
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"description" : "The astronomical unit of mass is the solar mass.The symbol $S$ is often used in astronomy to refer to this unit, although $M_{\\odot}$ is also common. The solar mass, $1.98844 \\times 10^{30} kg$, is a standard way to express mass in astronomy, used to describe the masses of other stars and galaxies. It is equal to the mass of the Sun, about 333,000 times the mass of the Earth or 1,048 times the mass of Jupiter. In practice, the masses of celestial bodies appear in the dynamics of the solar system only through the products GM, where G is the constant of gravitation.",
"conversionMultiplier" : "1988435000000000000000000000000.0",
"conversionMultiplier:SN" : 1.988435E30,
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