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Matches in DBpedia 2014 for { <http://dbpedia.org/resource/Solar_luminosity> ?p ?o. }

• Solar_luminosity abstract "The solar luminosity, L☉, is a unit of radiant flux (power emitted in the form of photons) conventionally used by astronomers to measure the luminosity of stars. One solar luminosity is equal to the current accepted luminosity of the Sun, which is 3.846×1026 W, or 3.846×1033 erg/s. This does not include the solar neutrino luminosity which would add an additional 0.023L☉. The Sun is a weakly variable star and its luminosity therefore fluctuates. The major fluctuation is the eleven-year solar cycle (sunspot cycle), which causes a periodic variation of about ±0.1%. Any other variation over the last 200–300 years is thought to be much smaller than this.".
• Solar_luminosity thumbnail Solar_evolution_(English).svg?width=300.
• Solar_luminosity wikiPageExternalLink LISIRD.
• Solar_luminosity wikiPageExternalLink node4.html.
• Solar_luminosity wikiPageExternalLink 5605.text.html.
• Solar_luminosity wikiPageExternalLink nature05072.html.
• Solar_luminosity wikiPageExternalLink stoykova_abs.html.
• Solar_luminosity wikiPageExternalLink solar-luminosity.
• Solar_luminosity wikiPageID "210900".
• Solar_luminosity wikiPageRevisionID "604057975".
• Solar_luminosity hasPhotoCollection Solar_luminosity.
• Solar_luminosity subject Category:Stellar_astronomy.
• Solar_luminosity subject Category:Sun.
• Solar_luminosity subject Category:Units_of_measurement_in_astronomy.
• Solar_luminosity subject Category:Units_of_power.
• Solar_luminosity type Abstraction100002137.
• Solar_luminosity type DefiniteQuantity113576101.
• Solar_luminosity type Measure100033615.
• Solar_luminosity type UnitOfMeasurement113583724.
• Solar_luminosity type UnitsOfPower.
• Solar_luminosity comment "The solar luminosity, L☉, is a unit of radiant flux (power emitted in the form of photons) conventionally used by astronomers to measure the luminosity of stars. One solar luminosity is equal to the current accepted luminosity of the Sun, which is 3.846×1026 W, or 3.846×1033 erg/s. This does not include the solar neutrino luminosity which would add an additional 0.023L☉. The Sun is a weakly variable star and its luminosity therefore fluctuates.".
• Solar_luminosity label "Jasność Słońca".
• Solar_luminosity label "Luminosidad solar".
• Solar_luminosity label "Luminosità solare".
• Solar_luminosity label "Luminosité solaire".
• Solar_luminosity label "Solar luminosity".
• Solar_luminosity label "Солнечная светимость".
• Solar_luminosity label "ضياء شمسي".
• Solar_luminosity label "太陽光度".
• Solar_luminosity label "太陽光度".
• Solar_luminosity sameAs Sluneční_zářivost.
• Solar_luminosity sameAs Luminosidad_solar.
• Solar_luminosity sameAs Luminosité_solaire.
• Solar_luminosity sameAs Luminositas_matahari.
• Solar_luminosity sameAs Luminosità_solare.
• Solar_luminosity sameAs 太陽光度.
• Solar_luminosity sameAs 태양광도.
• Solar_luminosity sameAs Jasność_Słońca.
• Solar_luminosity sameAs m.01dyjx.
• Solar_luminosity sameAs Q843877.
• Solar_luminosity sameAs Q843877.
• Solar_luminosity sameAs Solar_luminosity.
• Solar_luminosity wasDerivedFrom Solar_luminosity?oldid=604057975.
• Solar_luminosity depiction Solar_evolution_(English).svg.
• Solar_luminosity isPrimaryTopicOf Solar_luminosity.