This HTML5 document contains 11 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

Prefix	IRI
n4	http://qudt.org/vocab/quantitykind/
dcterms	http://purl.org/dc/terms/
n3	http://qudt.org/schema/qudt/
n2	http://qudt.org/vocab/unit/
n7	http://qudt.org/vocab/dimensionvector/
rdfs	http://www.w3.org/2000/01/rdf-schema#
n6	http://qudt.org/2.1/vocab/
rdf	http://www.w3.org/1999/02/22-rdf-syntax-ns#
xsdh	http://www.w3.org/2001/XMLSchema#
n9	http://www.ontology-of-units-of-measure.org/resource/om-2/

Statements

Subject Item

n2:SolarMass

rdf:type

n3:Unit

rdfs:label

Solar mass

rdfs:isDefinedBy

n6:unit

dcterms: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.

n3:dbpediaMatch

http://dbpedia.org/resource/Solar_mass

n3:hasDimensionVector

n7:A0E0L0I0M1H0T0D0

n3:informativeReference

http://en.wikipedia.org/wiki/Solar_mass?oldid=494074016

n3:symbol

S

n3:hasQuantityKind

n4:Mass

n3:conversionMultiplier

1.98843e+30

n3:omUnit

n9:solarMass