rdf:type |
qudt:QuantityKind |
dcterms:description |
In celestial mechanics the standard gravitational parameter of a celestial body is the product of the gravitational constant G and the mass M of the body. Expressed as \(\mu = G \cdot M\). The SI units of the standard gravitational parameter are \(m^{3}s^{-2}\). |
qudt:applicableUnit |
|
qudt:dbpediaMatch |
http://dbpedia.org/resource/Standard_gravitational_parameter |
qudt:hasDimensionVector |
qkdv:A0E0L3I0M0H0T-2D0 |
qudt:informativeReference |
http://en.wikipedia.org/wiki/Standard_gravitational_parameter |
qudt:latexSymbol |
\(\mu\) |
qudt:wikidataMatch |
http://www.wikidata.org/entity/Q579338 |
rdfs:comment |
“Applicable units are those of quantitykind:StandardGravitationalParameter” |
rdfs:isDefinedBy |
http://qudt.org/3.1.10/vocab/quantitykind |
rdfs:label |
“Standard Gravitational Parameter”@en |