rdf:type |
qudt:Unit |
dcterms:description |
The Planck energy divided by the Planck time is the Planck power \(P_p \), equal to about \(3.62831 \times 10^{52} W\). This is an extremely large unit; even gamma-ray bursts, the most luminous phenomena known, have output on the order of \(1 \times 10^{45} W\), less than one ten-millionth of the Planck power. |
qudt:applicableSystem |
sou:PLANCK |
qudt:conversionMultiplier |
36283100000000000000000000000000000000000000000000000.0 |
qudt:conversionMultiplierSN |
3.62831E52 |
qudt:dbpediaMatch |
http://dbpedia.org/resource/Planck_power |
qudt:derivedUnitOfSystem |
sou:PLANCK |
qudt:hasDimensionVector |
qkdv:A0E0L2I0M1H0T-3D0 |
qudt:hasQuantityKind |
quantitykind:Power |
qudt:informativeReference |
http://en.wikipedia.org/wiki/Planck_power?oldid=493642483 |
qudt:latexDefinition |
\(P_p = {\frac{ c^5}{G}}\), where \(c\) is the speed of light in a vacuum, and \(G\) is the gravitational constant. |
qudt:scalingOf |
unit:J-PER-SEC |
qudt:symbol |
“planckpower” |
qudt:wikidataMatch |
http://www.wikidata.org/entity/Q914151 |
rdfs:isDefinedBy |
http://qudt.org/3.1.11/vocab/unit |
rdfs:label |
- “Planck Power”
- “Planck Power”@en
|