. . . . . . . . . . . . . . . . . . . . "Die Leuchtkraft L ist eine vor allem in der Astronomie verwendete Bezeichnung f\u00FCr die abgestrahlte Leistung (Energie pro Zeit). Wenn die \u00FCber alle Bereiche des elektromagnetischen Spektrums summierte abgestrahlte Leistung betrachtet wird, ist die Leuchtkraft ein Synonym f\u00FCr \u201EStrahlungsleistung\u201C. Zur Angabe der Leuchtkraft k\u00F6nnen alle Einheiten der Leistung verwendet werden. Neben der SI-Einheit Watt war vor allem fr\u00FCher in der Astronomie auch Erg pro Sekunde \u00FCblich. Daneben wird auch die Sonnenleuchtkraft (L\u2609) als Einheit verwendet."@de . . "\u5149\u5EA6\u5728\u79D1\u5B78\u7684\u4E0D\u540C\u9818\u57DF\u4E2D\u6709\u4E0D\u540C\u7684\u610F\u7FA9\u3002"@zh . . . . . "Jasno\u015B\u0107, dzielno\u015B\u0107 promieniowania, moc promieniowania (ang. luminosity) \u2013 stosowana w astronomii wielko\u015B\u0107 fizyczna okre\u015Blaj\u0105ca ilo\u015B\u0107 energii, kt\u00F3r\u0105 cia\u0142o emituje w jednostce czasu. Jednostk\u0105 jasno\u015Bci jest wat lub wielokrotno\u015B\u0107 jasno\u015Bci S\u0142o\u0144ca (L\u2609) = 3,827\u00B71026 W.Jasno\u015B\u0107 mo\u017Ce by\u0107 podawana jako jasno\u015B\u0107 wizualna lub bolometryczna. W pierwszym przypadku pod uwag\u0119 bierze si\u0119 jedynie \u015Bwiat\u0142o widzialne, w drugim ca\u0142e spektrum promieniowania elektromagnetycznego."@pl . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "\u0421\u0432\u0435\u0442\u0438\u043C\u043E\u0441\u0442\u044C \u2014 \u043D\u0430\u0437\u0432\u0430\u043D\u0438\u0435 \u0440\u044F\u0434\u0430 \u0444\u0438\u0437\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0432\u0435\u043B\u0438\u0447\u0438\u043D."@ru . . . . . . . . "\u5149\u5EA6 (\u5929\u6587\u5B66)"@ja . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Leuchtkraft"@de . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "23892"^^ . . . . . . . . . . . . "\uAD11\uB3C4(\u5149\u5EA6, luminosity)\uB294 \uCC9C\uBB38\uD559\uC5D0\uC11C \uCC9C\uCCB4\uAC00 \uB2E8\uC704\uC2DC\uAC04\uC5D0 \uBC29\uC0AC\uD558\uB294 \uC5D0\uB108\uC9C0\uB97C \uAC00\uB9AC\uD0A4\uB294 \uBB3C\uB9AC\uB7C9\uC774\uB2E4. \uAD6D\uC81C \uB2E8\uC704\uACC4\uC5D0\uC11C\uB294 W, CGS \uB2E8\uC704\uACC4\uC5D0\uC11C\uB294 erg/s\uB85C \uB098\uD0C0\uB0B4\uC9C4\uB2E4. \uB610, \uD0DC\uC591\uC758 \uAD11\uB3C4 L\u2609(= 3.828\u00D71026 W)\uC744 \uB2E8\uC704\uB85C \uD558\uB294 \uAC83\uB3C4 \uB9CE\uB2E4. (\uCE21\uAD11\uC758 \uBD84\uC57C\uC5D0\uC11C \uC0AC\uC6A9\uB418\uB294 \u300C\uAD11\uB3C4\u300D(luminous intensity)\uB294 \uBCF8\uACE0\uC758 \uAD11\uB3C4\uC640\uB294 \uB2E4\uB978 \uCC28\uC6D0\uC744 \uAC00\uC9C0\uB294 \uB2E4\uB978 \uC591\uC774\uB2E4. \uC790\uC138\uD55C \uAC83\uC740 \uAD11\uB3C4\uB97C \uCC38\uC870) \uCC9C\uCCB4\uC758 \uC678\uAD00\uC758 \uBC1D\uAE30\uB294 \uAC70\uB9AC\uC758 2\uC2B9\uC5D0 \uBC18\uBE44\uB840 \uD574 \uC5B4\uB450\uC6CC\uC9C0\uC9C0\uB9CC, \uAD11\uB3C4\uB294 \uCC9C\uCCB4\uAE4C\uC9C0\uC758 \uAC70\uB9AC\uC5D0 \uC758\uD558\uC9C0 \uC54A\uB294 \uACE0\uC720\uC758 \uC591\uC774\uB2E4. \uCC9C\uCCB4\uC758 \uBC1D\uAE30\uB294 \uBCF4\uD1B5, \uB300\uC218 \uC2A4\uCF00\uC77C\uC758 \uC678\uAD00\uC758 \uB4F1\uAE09\uC744 \uC774\uC6A9\uD574 \uCE21\uC815\uD574\uC9C4\uB2E4. \uD56D\uC131\uC758 \uBC1D\uAE30\uB97C \uCE21\uC815\uD558\uB294 \uACBD\uC6B0, \uAD11\uB3C4\u00B7\uC678\uAD00\uC758 \uB4F1\uAE09\u00B7\uAC70\uB9AC\uB294 \uC11C\uB85C \uAD00\uACC4\uAC00 \uC788\uB294 \uBCC0\uC218\uC774\uB2E4. \uC774 3\uAC1C\uC758 \uBCC0\uC218\uC911 2\uB97C \uC54C \uC218 \uC788\uC73C\uBA74 \uB098\uBA38\uC9C0\uC758 \uD558\uB098\uB97C \uACB0\uC815\uD560 \uC218 \uC788\uB2E4. \uAD11\uB3C4\uC758 \uAE30\uC900\uC73C\uB85C\uC11C \uD0DC\uC591\uC758 \uAC12\uC744 \uC774\uC6A9\uD558\uB294 \uACBD\uC6B0\uAC00 \uB9CE\uAE30 \uB54C\uBB38\uC5D0, \uD0DC\uC591\uC758 \uC678\uAD00\uC758 \uB4F1\uAE09\uACFC \uD0DC\uC591\uAE4C\uC9C0\uC758 \uAC70\uB9AC\uB97C \uBAA9\uC801\uC758 \uCC9C\uCCB4\uB85C\uC758 \uAC12\uACFC \uBE44\uAD50\uD558\uBA74 \uAC00\uC7A5 \uAC04\uB2E8\uD558\uAC8C \uAC01 \uBCC0\uC218\uB97C \uACC4\uC0B0\uD560 \uC218 \uC788\uB2E4."@ko . . . . . . . . . . . . . . . . . . "Luminosity is an absolute measure of radiated electromagnetic power (light), the radiant power emitted by a light-emitting object over time. In astronomy, luminosity is the total amount of electromagnetic energy emitted per unit of time by a star, galaxy, or other astronomical object."@en . . . "1123909234"^^ . . . . . . . . . . . . . "En f\u00EDsica de part\u00EDculas se define la luminosidad instant\u00E1nea como el n\u00FAmero de part\u00EDculas por unidad de superficie y por unidad de tiempo en un haz. Se mide en unidades inversas de secci\u00F3n eficaz por unidad de tiempo. Al integrar esta cantidad durante un per\u00EDodo se obtiene la luminosidad integrada, la cual se mide en unidades inversas de secci\u00F3n eficaz (como por ejemplo el pb-1). Cuanto mayor es esta cantidad mayor es la probabilidad de que se produzcan sucesos interesantes en un experimento de altas energ\u00EDas. N\u00FAmero de sucesos = L \u00D7 \u03C3"@es . . . . . . . . . . . . . . . "\u0421\u0432\u0435\u0442\u0438\u043C\u043E\u0441\u0442\u044C"@ru . "Luminosidad"@es . . "Is \u00E9 rud is lonrachas ann n\u00E1 an dearbhmh\u00E9id n\u00F3 an bhunmh\u00E9id fuinnimh a rada\u00EDtear in aghaidh an tsoicind \u00F3 rinn sp\u00E9ire. Braitheann s\u00E9 ar fhairsinge dhromchlach na r\u00E9alta agus a teocht dhromchlach. M\u00E1 bh\u00EDonn dh\u00E1 r\u00E9alta ann leis an teocht dhromchlach ch\u00E9anna ach lonrachais dhifri\u00FAla, n\u00ED m\u00F3r go bhfuil difr\u00EDocht i m\u00E9id eatarthu. B\u00EDonn difr\u00EDochta\u00ED m\u00F3ra sna lonrachais a bhraitear ar Domhan \u00F3 r\u00E9alta\u00ED, \u00F3 mhilli\u00FAn oiread n\u00EDos m\u00F3 n\u00E1 lonrachas na Gr\u00E9ine s\u00EDos go dt\u00ED milli\u00FAn oiread n\u00EDos m\u00F3. Tomhaistear lonrachas i sainmh\u00E9id."@ga . . . "Z\u00E1\u0159iv\u00FD v\u00FDkon"@cs . "La lluminositat o brillantor \u00E9s la quantitat de flux llumin\u00F3s que emet una font de llum en una direcci\u00F3, en una unitat d'angle s\u00F2lid. La seva unitat de mesura en el sistema internacional d'unitats \u00E9s la candela (cd), que \u00E9s la intensitat lluminosa, en la direcci\u00F3 perpendicular respecte a una superf\u00EDcie d'1/600.000 m\u00B2 d'un cos negre a la temperatura de congelaci\u00F3 del plat\u00ED, a una pressi\u00F3 de 101.325 pascals. La seva expressi\u00F3 \u00E9s: en qu\u00E8 E \u00E9s la lluminositat, I la intensitat i D la dist\u00E0ncia. La intensitat lluminosa forma part de les magnituds fonamentals de la f\u00EDsica. Nombre de successos = L \u00D7 \u03C3"@ca . . . . . . . . "In astronomia, la luminosit\u00E0 \u00E8 la quantit\u00E0 di energia elettromagnetica emessa da una stella per unit\u00E0 di tempo, ovvero la sua potenza. Si misura pertanto in watt, in erg/secondo oppure in termini di luminosit\u00E0 solari. La luminosit\u00E0 \u00E8 detta assoluta o bolometrica (da bolometro)."@it . . . "En astronomie, la luminosit\u00E9 est la quantit\u00E9 totale d'\u00E9nergie \u00E9mise par unit\u00E9 de temps (le flux \u00E9nerg\u00E9tique), par une \u00E9toile, une galaxie, ou n'importe quel autre objet c\u00E9leste. Elle s'exprime en pratique en luminosit\u00E9 solaire ( = 3,827 5 \u00D7\u202F1026 W). Le flux lumineux, qui mesure plus particuli\u00E8rement l'\u00E9mission en lumi\u00E8re visible, peut \u00E9galement s'exprimer sur une \u00E9chelle logarithmique par la magnitude absolue."@fr . . . . "Luminositet"@sv . . . . . . . . . . . . . . . . . . . . . . "Luminosit\u00E9"@fr . . . . . . . . . . . "\u5149\u5EA6\uFF08\u3053\u3046\u3069\u3001\u82F1\u8A9E: luminosity\uFF09\u3068\u306F\u3001\u5929\u6587\u5B66\u3067\u5929\u4F53\u304C\u5358\u4F4D\u6642\u9593\u306B\u653E\u5C04\u3059\u308B\u30A8\u30CD\u30EB\u30AE\u30FC\u3092\u6307\u3059\u7269\u7406\u91CF\u3067\u3042\u308B\u3002\u56FD\u969B\u5358\u4F4D\u7CFB\u3067\u306F W\u3001CGS\u5358\u4F4D\u7CFB\u3067\u306F erg/s \u3067\u8868\u3055\u308C\u308B\u3002\u307E\u305F\u3001\u592A\u967D\u306E\u5149\u5EA6 L\u2609 (= 3.827\u00D71026 W) \u3092\u5358\u4F4D\u3068\u3059\u308B\u3053\u3068\u3082\u591A\u3044\u3002\u5929\u4F53\u306E\u898B\u304B\u3051\u306E\u660E\u308B\u3055\u306F\u8DDD\u96E2\u306E2\u4E57\u306B\u53CD\u6BD4\u4F8B\u3057\u3066\u6697\u304F\u306A\u308B\u304C\u3001\u5149\u5EA6\u306F\u5929\u4F53\u307E\u3067\u306E\u8DDD\u96E2\u306B\u3088\u3089\u306A\u3044\u56FA\u6709\u306E\u91CF\u3067\u3042\u308B\u3002\u5929\u4F53\u306E\u660E\u308B\u3055\u306F\u666E\u901A\u3001\u5BFE\u6570\u30B9\u30B1\u30FC\u30EB\u306E\u898B\u304B\u3051\u306E\u7B49\u7D1A\u3092\u7528\u3044\u3066\u6E2C\u3089\u308C\u308B\u3002 \u6052\u661F\u306E\u660E\u308B\u3055\u3092\u6E2C\u5B9A\u3059\u308B\u5834\u5408\u3001\u5149\u5EA6\u30FB\u898B\u304B\u3051\u306E\u7B49\u7D1A\u30FB\u8DDD\u96E2\u306F\u4E92\u3044\u306B\u95A2\u4FC2\u306E\u3042\u308B\u5909\u6570\u3067\u3042\u308B\u3002\u3053\u306E3\u3064\u306E\u5909\u6570\u306E\u3046\u30612\u3064\u3092\u77E5\u308B\u3053\u3068\u304C\u3067\u304D\u308C\u3070\u6B8B\u308A\u306E\u4E00\u3064\u3092\u6C7A\u3081\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002\u5149\u5EA6\u306E\u57FA\u6E96\u3068\u3057\u3066\u592A\u967D\u306E\u5024\u3092\u7528\u3044\u308B\u5834\u5408\u304C\u591A\u3044\u306E\u3067\u3001\u592A\u967D\u306E\u898B\u304B\u3051\u306E\u7B49\u7D1A\u3068\u592A\u967D\u307E\u3067\u306E\u8DDD\u96E2\u3092\u76EE\u7684\u306E\u5929\u4F53\u3067\u306E\u5024\u3068\u6BD4\u8F03\u3059\u308C\u3070\u6700\u3082\u7C21\u5358\u306B\u5404\u5909\u6570\u3092\u8A08\u7B97\u3067\u304D\u308B\u3002 \u6E2C\u5149\u306E\u5206\u91CE\u3067\u4F7F\u308F\u308C\u308B\u5149\u5EA6\uFF08\u82F1\u8A9E: luminous intensity\uFF09\u3068\u306F\u5225\u306E\u6B21\u5143\u3092\u6301\u3064\u7570\u306A\u308B\u91CF\u3067\u3042\u308B\u3002"@ja . . . "Lichtkracht"@nl . . . . . . . . . "Argitasun"@eu . . . . . . . . "Luminositas, kecemerlangan, atau kekilauan adalah istilah yang digunakan dalam ilmu Fisika dan turunannya."@in . . . . . . . . . . . "Luminosidade"@pt . . . . . . "\u5149\u5EA6\u5728\u79D1\u5B78\u7684\u4E0D\u540C\u9818\u57DF\u4E2D\u6709\u4E0D\u540C\u7684\u610F\u7FA9\u3002"@zh . . . . . "Lonrachas"@ga . "La lluminositat o brillantor \u00E9s la quantitat de flux llumin\u00F3s que emet una font de llum en una direcci\u00F3, en una unitat d'angle s\u00F2lid. La seva unitat de mesura en el sistema internacional d'unitats \u00E9s la candela (cd), que \u00E9s la intensitat lluminosa, en la direcci\u00F3 perpendicular respecte a una superf\u00EDcie d'1/600.000 m\u00B2 d'un cos negre a la temperatura de congelaci\u00F3 del plat\u00ED, a una pressi\u00F3 de 101.325 pascals. La seva expressi\u00F3 \u00E9s: en qu\u00E8 E \u00E9s la lluminositat, I la intensitat i D la dist\u00E0ncia. La intensitat lluminosa forma part de les magnituds fonamentals de la f\u00EDsica. En f\u00EDsica de part\u00EDcules, es defineix la lluminositat instant\u00E0nia com el nombre de part\u00EDcules per unitat de superf\u00EDcie i per unitat de temps en un feix. Es mesura en unitats inverses de secci\u00F3 efica\u00E7 per unitat de temps. En integrar aquesta quantitat durant un per\u00EDode, s'obt\u00E9 la lluminositat integrada, la qual es mesura en unitats inverses de secci\u00F3 efica\u00E7 (per exemple, el pb-1). Quant m\u00E9s gran \u00E9s aquesta quantitat, m\u00E9s gran \u00E9s la probabilitat que es produeixin successos interessants en un experiment d'altes energies. En un proc\u00E9s la secci\u00F3 efica\u00E7 (\u03C3) del qual coneixem, per a una lluminositat integrada L donada, es pot estimar el nombre de vegades que es produir\u00E0 aquest succ\u00E9s simplement multiplicant ambdues quantitats: Nombre de successos = L \u00D7 \u03C3 En astronomia, la lluminositat o lluminositat absoluta \u00E9s la quantitat d'energia per unitat de temps emesa en totes direccions per un cos celeste. Est\u00E0 directament relacionada amb la magnitud absoluta. Usualment, se sol mesurar per comparaci\u00F3 amb la lluminositat del Sol."@ca . . . . . . . . . . . . "Luminositas, kecemerlangan, atau kekilauan adalah istilah yang digunakan dalam ilmu Fisika dan turunannya."@in . . . . . . . . . . . . . "Luminositet \u00E4r en storhet som anv\u00E4nds inom astronomi. Den m\u00E4ter den sammanlagda utstr\u00E5lade effekten fr\u00E5n en himlakropp och m\u00E4ts i enheten watt. Luminositeten \u00E4r ett m\u00E5tt p\u00E5 en stj\u00E4rnas ljusstyrka och brukar r\u00E4knas i j\u00E4mf\u00F6relse med solen. Luminositeten \u00E4r relaterad till den absoluta magnituden \u2013 ju st\u00F6rre luminositet desto mindre magnitud."@sv . . . . . . . . . . . . . . . . "En f\u00EDsica de part\u00EDculas se define la luminosidad instant\u00E1nea como el n\u00FAmero de part\u00EDculas por unidad de superficie y por unidad de tiempo en un haz. Se mide en unidades inversas de secci\u00F3n eficaz por unidad de tiempo. Al integrar esta cantidad durante un per\u00EDodo se obtiene la luminosidad integrada, la cual se mide en unidades inversas de secci\u00F3n eficaz (como por ejemplo el pb-1). Cuanto mayor es esta cantidad mayor es la probabilidad de que se produzcan sucesos interesantes en un experimento de altas energ\u00EDas. Dado un proceso cuya secci\u00F3n eficaz, \u03C3, conocemos, para una luminosidad integrada, L, dada, podemos estimar el n\u00FAmero de veces que se va a producir ese suceso simplemente multiplicando ambas cantidades: N\u00FAmero de sucesos = L \u00D7 \u03C3"@es . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "In astronomia, la luminosit\u00E0 \u00E8 la quantit\u00E0 di energia elettromagnetica emessa da una stella per unit\u00E0 di tempo, ovvero la sua potenza. Si misura pertanto in watt, in erg/secondo oppure in termini di luminosit\u00E0 solari. La luminosit\u00E0 \u00E8 detta assoluta o bolometrica (da bolometro)."@it . . . . . . . . . . . "Is \u00E9 rud is lonrachas ann n\u00E1 an dearbhmh\u00E9id n\u00F3 an bhunmh\u00E9id fuinnimh a rada\u00EDtear in aghaidh an tsoicind \u00F3 rinn sp\u00E9ire. Braitheann s\u00E9 ar fhairsinge dhromchlach na r\u00E9alta agus a teocht dhromchlach. M\u00E1 bh\u00EDonn dh\u00E1 r\u00E9alta ann leis an teocht dhromchlach ch\u00E9anna ach lonrachais dhifri\u00FAla, n\u00ED m\u00F3r go bhfuil difr\u00EDocht i m\u00E9id eatarthu. B\u00EDonn difr\u00EDochta\u00ED m\u00F3ra sna lonrachais a bhraitear ar Domhan \u00F3 r\u00E9alta\u00ED, \u00F3 mhilli\u00FAn oiread n\u00EDos m\u00F3 n\u00E1 lonrachas na Gr\u00E9ine s\u00EDos go dt\u00ED milli\u00FAn oiread n\u00EDos m\u00F3. Tomhaistear lonrachas i sainmh\u00E9id."@ga . . . . . . . . . . . . . . . . . . . . . . "Luminosity is an absolute measure of radiated electromagnetic power (light), the radiant power emitted by a light-emitting object over time. In astronomy, luminosity is the total amount of electromagnetic energy emitted per unit of time by a star, galaxy, or other astronomical object. In SI units, luminosity is measured in joules per second, or watts. In astronomy, values for luminosity are often given in the terms of the luminosity of the Sun, L\u2299. Luminosity can also be given in terms of the astronomical magnitude system: the absolute bolometric magnitude (Mbol) of an object is a logarithmic measure of its total energy emission rate, while absolute magnitude is a logarithmic measure of the luminosity within some specific wavelength range or filter band. In contrast, the term brightness in astronomy is generally used to refer to an object's apparent brightness: that is, how bright an object appears to an observer. Apparent brightness depends on both the luminosity of the object and the distance between the object and observer, and also on any absorption of light along the path from object to observer. Apparent magnitude is a logarithmic measure of apparent brightness. The distance determined by luminosity measures can be somewhat ambiguous, and is thus sometimes called the luminosity distance."@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "University of Southampton radio luminosity calculator"@en . . . . . . . . "\uAD11\uB3C4 (\uCC9C\uBB38\uD559)"@ko . . . . . . . . . . . . . . . . . . . . . . . . . . "44790"^^ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "\u5149\u5EA6"@zh . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Jasno\u015B\u0107, dzielno\u015B\u0107 promieniowania, moc promieniowania (ang. luminosity) \u2013 stosowana w astronomii wielko\u015B\u0107 fizyczna okre\u015Blaj\u0105ca ilo\u015B\u0107 energii, kt\u00F3r\u0105 cia\u0142o emituje w jednostce czasu. Jednostk\u0105 jasno\u015Bci jest wat lub wielokrotno\u015B\u0107 jasno\u015Bci S\u0142o\u0144ca (L\u2609) = 3,827\u00B71026 W.Jasno\u015B\u0107 mo\u017Ce by\u0107 podawana jako jasno\u015B\u0107 wizualna lub bolometryczna. W pierwszym przypadku pod uwag\u0119 bierze si\u0119 jedynie \u015Bwiat\u0142o widzialne, w drugim ca\u0142e spektrum promieniowania elektromagnetycznego."@pl . . . . . . . . . "\u0636\u064A\u0627\u0621"@ar . . . . "Em astronomia, luminosidade \u00E9 a quantidade de energia que um corpo irradia em uma unidade de tempo. Ela \u00E9 tipicamente expressa em unidades de watts ou em termos da Luminosidade solar, Lsol. Neste caso, ela \u00E9 a quantidade de energia que o objeto irradia comparada com a do Sol, cuja luminosidade \u00E9 3,827\u00D71026 Watt. Luminosidade n\u00E3o deve ser confundida com lumin\u00E2ncia."@pt . . . . . "\u0421\u0432\u0456\u0442\u043D\u0456\u0441\u0442\u044C"@uk . . . "Em astronomia, luminosidade \u00E9 a quantidade de energia que um corpo irradia em uma unidade de tempo. Ela \u00E9 tipicamente expressa em unidades de watts ou em termos da Luminosidade solar, Lsol. Neste caso, ela \u00E9 a quantidade de energia que o objeto irradia comparada com a do Sol, cuja luminosidade \u00E9 3,827\u00D71026 Watt. Luminosidade n\u00E3o deve ser confundida com lumin\u00E2ncia. Luminosidade \u00E9 uma constante intr\u00EDnseca independente da dist\u00E2ncia, enquanto que o brilho aparente observado est\u00E1 relacionado com a dist\u00E2ncia atrav\u00E9s de uma lei do tipo inverso do quadrado da dist\u00E2ncia. Brilho \u00E9 usualmente medido por meio da magnitude aparente, e \u00E9 uma escala logar\u00EDtmica. Ao medir o brilho de uma estrela, luminosidade, magnitude aparente (brilho) e dist\u00E2ncia s\u00E3o par\u00E2metros interrelacionados. Se se conhecem dois deles, o terceiro pode ser calculado. Como a luminosidade do Sol \u00E9 o padr\u00E3o, comparar estes par\u00E2metros com a magnitude aparente e dist\u00E2ncia \u00E9 a forma mais f\u00E1cil de lembr\u00E1-los."@pt . "Luminositet \u00E4r en storhet som anv\u00E4nds inom astronomi. Den m\u00E4ter den sammanlagda utstr\u00E5lade effekten fr\u00E5n en himlakropp och m\u00E4ts i enheten watt. Luminositeten \u00E4r ett m\u00E5tt p\u00E5 en stj\u00E4rnas ljusstyrka och brukar r\u00E4knas i j\u00E4mf\u00F6relse med solen. Luminositeten \u00E4r relaterad till den absoluta magnituden \u2013 ju st\u00F6rre luminositet desto mindre magnitud."@sv . . . . "Lumeco estas la energio, kiun luma objekto (plejofte stelo) disradias portempe. Lumeco estas mezurita per vatunuoj (W). Lumeco de stelo estas sendependa de distanco."@eo . . . . . . "Luminosit\u00E0 (astronomia)"@it . . . . . "\u0627\u0644\u0636\u064A\u0627\u0621 \u0641\u064A \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643\u060C \u0647\u0648 \u0627\u0644\u0643\u0645\u064A\u0629 \u0627\u0644\u0625\u062C\u0645\u0627\u0644\u064A\u0629 \u0644\u0644\u0637\u0627\u0642\u0629 \u0627\u0644\u0645\u0646\u0628\u0639\u062B\u0629 \u0645\u0646 \u0646\u062C\u0645 \u0623\u0648 \u0645\u062C\u0631\u0629 \u0623\u0648 \u0623\u064A \u062C\u0631\u0645 \u0641\u0644\u0643\u064A \u0622\u062E\u0631 \u0644\u0643\u0644 \u0648\u062D\u062F\u0629 \u0632\u0645\u0646\u064A\u0629\u060C \u0623\u064A \u0627\u0644\u0637\u0627\u0642\u0629 \u0627\u0644\u0643\u0644\u064A\u0629 \u0627\u0644\u0635\u0627\u062F\u0631\u0629 \u0641\u064A \u062C\u0645\u064A\u0639 \u0627\u0644\u0627\u062A\u062C\u0627\u0647\u0627\u062A \u0648\u062A\u0642\u0627\u0633 \u0628\u0627\u0644\u0648\u0627\u0637."@ar . . . . . . . . . . . . . . . . . "Argitasuna argia denaren nolakotasuna da. Argitasuna erradiazio elektromagnetikoaren magnitude absolutua da, argia igortzen duen objektu batek igortzen duen irradiatze-energia. Astronomian, argitasuna, izar, galaxia edo beste objektu astronomiko batek denbora unitate bakoitzeko igortzen duen energia elektromagnetikoaren kopuru osoa da. SI unitateetan, argitasuna segundoko jouletan edo wattetan neurtzen dute. Astronomian, argitasun balioak, sarri, eguzki-argitasun terminoetan agertzen dira, L\u2299 ikurra duena."@eu . . . . . . "In de astronomie wordt onder de lichtkracht (luminositeit, helderheid) van een ster verstaan het totaal uitgezonden vermogen in de vorm van elektromagnetische straling. De lichtkracht is afhankelijk van de effectieve temperatuur van de ster en z'n omvang. De lichtkracht wordt uitgedrukt in watt of in eenheden van de nominale lichtkracht van de zon (L\u2609), een vaste waarde waar de daadwerkelijke lichtkracht van de zon ongeveer aan gelijk is. De Internationale Astronomische Unie heeft deze eenheid gedefinieerd als De lichtkracht van een andere ster bepaalt men door z'n absolute helderheid te vergelijken met die van de zon of van een andere ster met reeds bekende lichtkracht. Er moet onderscheid worden gemaakt tussen de bolometrische lichtkracht, dat wil zeggen de lichtkracht gemeten over alle golflengten van het elektromagnetische spectrum, en de , dat wil zeggen de lichtkracht in het zichtbare deel van het spectrum. Bij sterren die in oppervlaktetemperatuur sterk afwijken van de zon is deze laatste vaak een stuk kleiner dan de eerste, omdat zij een groot deel van hun energie uitzenden in het infrarood (bijvoorbeeld rode dwergen en rode reuzen) of in het ultraviolet (bijvoorbeeld witte dwergen en blauwe reuzen). Voor het omrekenen tussen de bijbehorende magnitudes wordt de bolometrische correctie toegepast."@nl . . . . "Lluminositat"@ca . . "2015-05-08"^^ . . . . . . . "Jasno\u015B\u0107 (astronomia)"@pl . . . . . . "Z\u00E1\u0159iv\u00FD v\u00FDkon je souhrnn\u00FD v\u00FDkon, kter\u00FD t\u011Bleso vyza\u0159uje do prostoru jako elektromagnetick\u00E9 z\u00E1\u0159en\u00ED. M\u016F\u017Ee j\u00EDt o \n* r\u00E1diov\u00E9 vlny, nap\u0159. u pulsar\u016F nebo jin\u00FDch ant\u00E9n; \n* sv\u011Bteln\u00FD tok \u017Ehav\u00E9ho t\u011Blesa, nap\u0159. \u017E\u00E1rovky, nebo i sv\u011Btlo chladn\u00FDch sv\u011Bteln\u00FDch zdroj\u016F, jako z\u00E1\u0159ivek nebo LED; \n* tepeln\u00E9 z\u00E1\u0159en\u00ED nebo jinak tak\u00E9 pro lidsk\u00E9 oko neviditeln\u00E9 infra\u010Derven\u00E9 z\u00E1\u0159en\u00ED t\u011Bles podle jejich teploty. Rozlo\u017Een\u00ED energie do jednotliv\u00FDch frekven\u010Dn\u00EDch p\u00E1sem popisuje Planck\u016Fv vyza\u0159ovac\u00ED z\u00E1kon."@cs . . . "\u0421\u0432\u0435\u0442\u0438\u043C\u043E\u0441\u0442\u044C \u2014 \u043D\u0430\u0437\u0432\u0430\u043D\u0438\u0435 \u0440\u044F\u0434\u0430 \u0444\u0438\u0437\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0432\u0435\u043B\u0438\u0447\u0438\u043D."@ru . . . . "Luminositas"@in . "\u0421\u0432\u0456\u0301\u0442\u043D\u0456\u0441\u0442\u044C \u0443 \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u0456\u0439 \u0444\u0456\u0437\u0438\u0446\u0456 \u2014 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0439 \u043F\u043E\u0442\u0456\u043A, \u0449\u043E \u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0454\u0442\u044C\u0441\u044F \u043E\u0434\u0438\u043D\u0438\u0446\u0435\u044E \u043F\u043B\u043E\u0449\u0456 \u0441\u0432\u0456\u0442\u043D\u043E\u0457 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u0456 (\u044F\u043A\u0430 \u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0454, \u0432\u0456\u0434\u0431\u0438\u0432\u0430\u0454 \u0430\u0431\u043E \u043F\u0440\u043E\u043F\u0443\u0441\u043A\u0430\u0454 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0439 \u043F\u043E\u0442\u0456\u043A) \u0432 \u0443\u0441\u0456\u0445 \u043D\u0430\u043F\u0440\u044F\u043C\u043A\u0430\u0445 (\u0432 \u0441\u0435\u0440\u0435\u0434\u0438\u043D\u0456 \u0442\u0456\u043B\u0435\u0441\u043D\u043E\u0433\u043E \u043A\u0443\u0442\u0430 2) , [M]=[\u043B\u043C/\u043C\u00B2] \u0426\u0435\u0439 \u0442\u0435\u0440\u043C\u0456\u043D \u043C\u0430\u0454 \u0441\u043F\u0435\u0446\u0438\u0444\u0456\u0447\u043D\u0435 \u0437\u043D\u0430\u0447\u0435\u043D\u043D\u044F \u0432 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u0457 \u0442\u0430 \u0444\u0456\u0437\u0438\u0446\u0456 \u0435\u043B\u0435\u043C\u0435\u043D\u0442\u0430\u0440\u043D\u0438\u0445 \u0447\u0430\u0441\u0442\u0438\u043D\u043E\u043A."@uk . . . . . . "Argitasuna argia denaren nolakotasuna da. Argitasuna erradiazio elektromagnetikoaren magnitude absolutua da, argia igortzen duen objektu batek igortzen duen irradiatze-energia. Astronomian, argitasuna, izar, galaxia edo beste objektu astronomiko batek denbora unitate bakoitzeko igortzen duen energia elektromagnetikoaren kopuru osoa da. SI unitateetan, argitasuna segundoko jouletan edo wattetan neurtzen dute. Astronomian, argitasun balioak, sarri, eguzki-argitasun terminoetan agertzen dira, L\u2299 ikurra duena."@eu . "Lumeco"@eo . . . . . . . . . . . . "\u0421\u0432\u0456\u0301\u0442\u043D\u0456\u0441\u0442\u044C \u0443 \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u0456\u0439 \u0444\u0456\u0437\u0438\u0446\u0456 \u2014 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0439 \u043F\u043E\u0442\u0456\u043A, \u0449\u043E \u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0454\u0442\u044C\u0441\u044F \u043E\u0434\u0438\u043D\u0438\u0446\u0435\u044E \u043F\u043B\u043E\u0449\u0456 \u0441\u0432\u0456\u0442\u043D\u043E\u0457 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u0456 (\u044F\u043A\u0430 \u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0454, \u0432\u0456\u0434\u0431\u0438\u0432\u0430\u0454 \u0430\u0431\u043E \u043F\u0440\u043E\u043F\u0443\u0441\u043A\u0430\u0454 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0439 \u043F\u043E\u0442\u0456\u043A) \u0432 \u0443\u0441\u0456\u0445 \u043D\u0430\u043F\u0440\u044F\u043C\u043A\u0430\u0445 (\u0432 \u0441\u0435\u0440\u0435\u0434\u0438\u043D\u0456 \u0442\u0456\u043B\u0435\u0441\u043D\u043E\u0433\u043E \u043A\u0443\u0442\u0430 2) , [M]=[\u043B\u043C/\u043C\u00B2] \u0426\u0435\u0439 \u0442\u0435\u0440\u043C\u0456\u043D \u043C\u0430\u0454 \u0441\u043F\u0435\u0446\u0438\u0444\u0456\u0447\u043D\u0435 \u0437\u043D\u0430\u0447\u0435\u043D\u043D\u044F \u0432 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u0457 \u0442\u0430 \u0444\u0456\u0437\u0438\u0446\u0456 \u0435\u043B\u0435\u043C\u0435\u043D\u0442\u0430\u0440\u043D\u0438\u0445 \u0447\u0430\u0441\u0442\u0438\u043D\u043E\u043A."@uk . . . . . . . . . . . . . . . . "Z\u00E1\u0159iv\u00FD v\u00FDkon je souhrnn\u00FD v\u00FDkon, kter\u00FD t\u011Bleso vyza\u0159uje do prostoru jako elektromagnetick\u00E9 z\u00E1\u0159en\u00ED. M\u016F\u017Ee j\u00EDt o \n* r\u00E1diov\u00E9 vlny, nap\u0159. u pulsar\u016F nebo jin\u00FDch ant\u00E9n; \n* sv\u011Bteln\u00FD tok \u017Ehav\u00E9ho t\u011Blesa, nap\u0159. \u017E\u00E1rovky, nebo i sv\u011Btlo chladn\u00FDch sv\u011Bteln\u00FDch zdroj\u016F, jako z\u00E1\u0159ivek nebo LED; \n* tepeln\u00E9 z\u00E1\u0159en\u00ED nebo jinak tak\u00E9 pro lidsk\u00E9 oko neviditeln\u00E9 infra\u010Derven\u00E9 z\u00E1\u0159en\u00ED t\u011Bles podle jejich teploty. Rozlo\u017Een\u00ED energie do jednotliv\u00FDch frekven\u010Dn\u00EDch p\u00E1sem popisuje Planck\u016Fv vyza\u0159ovac\u00ED z\u00E1kon."@cs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Luminosity"@en . . . . . . . . "En astronomie, la luminosit\u00E9 est la quantit\u00E9 totale d'\u00E9nergie \u00E9mise par unit\u00E9 de temps (le flux \u00E9nerg\u00E9tique), par une \u00E9toile, une galaxie, ou n'importe quel autre objet c\u00E9leste. Elle s'exprime en pratique en luminosit\u00E9 solaire ( = 3,827 5 \u00D7\u202F1026 W). Le flux lumineux, qui mesure plus particuli\u00E8rement l'\u00E9mission en lumi\u00E8re visible, peut \u00E9galement s'exprimer sur une \u00E9chelle logarithmique par la magnitude absolue."@fr . . . . . . . . . . . "In de astronomie wordt onder de lichtkracht (luminositeit, helderheid) van een ster verstaan het totaal uitgezonden vermogen in de vorm van elektromagnetische straling. De lichtkracht is afhankelijk van de effectieve temperatuur van de ster en z'n omvang. De lichtkracht wordt uitgedrukt in watt of in eenheden van de nominale lichtkracht van de zon (L\u2609), een vaste waarde waar de daadwerkelijke lichtkracht van de zon ongeveer aan gelijk is. De Internationale Astronomische Unie heeft deze eenheid gedefinieerd als"@nl . . . . . . "\uAD11\uB3C4(\u5149\u5EA6, luminosity)\uB294 \uCC9C\uBB38\uD559\uC5D0\uC11C \uCC9C\uCCB4\uAC00 \uB2E8\uC704\uC2DC\uAC04\uC5D0 \uBC29\uC0AC\uD558\uB294 \uC5D0\uB108\uC9C0\uB97C \uAC00\uB9AC\uD0A4\uB294 \uBB3C\uB9AC\uB7C9\uC774\uB2E4. \uAD6D\uC81C \uB2E8\uC704\uACC4\uC5D0\uC11C\uB294 W, CGS \uB2E8\uC704\uACC4\uC5D0\uC11C\uB294 erg/s\uB85C \uB098\uD0C0\uB0B4\uC9C4\uB2E4. \uB610, \uD0DC\uC591\uC758 \uAD11\uB3C4 L\u2609(= 3.828\u00D71026 W)\uC744 \uB2E8\uC704\uB85C \uD558\uB294 \uAC83\uB3C4 \uB9CE\uB2E4. (\uCE21\uAD11\uC758 \uBD84\uC57C\uC5D0\uC11C \uC0AC\uC6A9\uB418\uB294 \u300C\uAD11\uB3C4\u300D(luminous intensity)\uB294 \uBCF8\uACE0\uC758 \uAD11\uB3C4\uC640\uB294 \uB2E4\uB978 \uCC28\uC6D0\uC744 \uAC00\uC9C0\uB294 \uB2E4\uB978 \uC591\uC774\uB2E4. \uC790\uC138\uD55C \uAC83\uC740 \uAD11\uB3C4\uB97C \uCC38\uC870) \uCC9C\uCCB4\uC758 \uC678\uAD00\uC758 \uBC1D\uAE30\uB294 \uAC70\uB9AC\uC758 2\uC2B9\uC5D0 \uBC18\uBE44\uB840 \uD574 \uC5B4\uB450\uC6CC\uC9C0\uC9C0\uB9CC, \uAD11\uB3C4\uB294 \uCC9C\uCCB4\uAE4C\uC9C0\uC758 \uAC70\uB9AC\uC5D0 \uC758\uD558\uC9C0 \uC54A\uB294 \uACE0\uC720\uC758 \uC591\uC774\uB2E4. \uCC9C\uCCB4\uC758 \uBC1D\uAE30\uB294 \uBCF4\uD1B5, \uB300\uC218 \uC2A4\uCF00\uC77C\uC758 \uC678\uAD00\uC758 \uB4F1\uAE09\uC744 \uC774\uC6A9\uD574 \uCE21\uC815\uD574\uC9C4\uB2E4. \uD56D\uC131\uC758 \uBC1D\uAE30\uB97C \uCE21\uC815\uD558\uB294 \uACBD\uC6B0, \uAD11\uB3C4\u00B7\uC678\uAD00\uC758 \uB4F1\uAE09\u00B7\uAC70\uB9AC\uB294 \uC11C\uB85C \uAD00\uACC4\uAC00 \uC788\uB294 \uBCC0\uC218\uC774\uB2E4. \uC774 3\uAC1C\uC758 \uBCC0\uC218\uC911 2\uB97C \uC54C \uC218 \uC788\uC73C\uBA74 \uB098\uBA38\uC9C0\uC758 \uD558\uB098\uB97C \uACB0\uC815\uD560 \uC218 \uC788\uB2E4. \uAD11\uB3C4\uC758 \uAE30\uC900\uC73C\uB85C\uC11C \uD0DC\uC591\uC758 \uAC12\uC744 \uC774\uC6A9\uD558\uB294 \uACBD\uC6B0\uAC00 \uB9CE\uAE30 \uB54C\uBB38\uC5D0, \uD0DC\uC591\uC758 \uC678\uAD00\uC758 \uB4F1\uAE09\uACFC \uD0DC\uC591\uAE4C\uC9C0\uC758 \uAC70\uB9AC\uB97C \uBAA9\uC801\uC758 \uCC9C\uCCB4\uB85C\uC758 \uAC12\uACFC \uBE44\uAD50\uD558\uBA74 \uAC00\uC7A5 \uAC04\uB2E8\uD558\uAC8C \uAC01 \uBCC0\uC218\uB97C \uACC4\uC0B0\uD560 \uC218 \uC788\uB2E4."@ko . . . . . . . . . . . . . "\u0627\u0644\u0636\u064A\u0627\u0621 \u0641\u064A \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643\u060C \u0647\u0648 \u0627\u0644\u0643\u0645\u064A\u0629 \u0627\u0644\u0625\u062C\u0645\u0627\u0644\u064A\u0629 \u0644\u0644\u0637\u0627\u0642\u0629 \u0627\u0644\u0645\u0646\u0628\u0639\u062B\u0629 \u0645\u0646 \u0646\u062C\u0645 \u0623\u0648 \u0645\u062C\u0631\u0629 \u0623\u0648 \u0623\u064A \u062C\u0631\u0645 \u0641\u0644\u0643\u064A \u0622\u062E\u0631 \u0644\u0643\u0644 \u0648\u062D\u062F\u0629 \u0632\u0645\u0646\u064A\u0629\u060C \u0623\u064A \u0627\u0644\u0637\u0627\u0642\u0629 \u0627\u0644\u0643\u0644\u064A\u0629 \u0627\u0644\u0635\u0627\u062F\u0631\u0629 \u0641\u064A \u062C\u0645\u064A\u0639 \u0627\u0644\u0627\u062A\u062C\u0627\u0647\u0627\u062A \u0648\u062A\u0642\u0627\u0633 \u0628\u0627\u0644\u0648\u0627\u0637."@ar . . . . . . "Die Leuchtkraft L ist eine vor allem in der Astronomie verwendete Bezeichnung f\u00FCr die abgestrahlte Leistung (Energie pro Zeit). Wenn die \u00FCber alle Bereiche des elektromagnetischen Spektrums summierte abgestrahlte Leistung betrachtet wird, ist die Leuchtkraft ein Synonym f\u00FCr \u201EStrahlungsleistung\u201C. Zur Angabe der Leuchtkraft k\u00F6nnen alle Einheiten der Leistung verwendet werden. Neben der SI-Einheit Watt war vor allem fr\u00FCher in der Astronomie auch Erg pro Sekunde \u00FCblich. Daneben wird auch die Sonnenleuchtkraft (L\u2609) als Einheit verwendet."@de . . . . . . . "Lumeco estas la energio, kiun luma objekto (plejofte stelo) disradias portempe. Lumeco estas mezurita per vatunuoj (W). Lumeco de stelo estas sendependa de distanco."@eo . . . . . . . . . . . "\u5149\u5EA6\uFF08\u3053\u3046\u3069\u3001\u82F1\u8A9E: luminosity\uFF09\u3068\u306F\u3001\u5929\u6587\u5B66\u3067\u5929\u4F53\u304C\u5358\u4F4D\u6642\u9593\u306B\u653E\u5C04\u3059\u308B\u30A8\u30CD\u30EB\u30AE\u30FC\u3092\u6307\u3059\u7269\u7406\u91CF\u3067\u3042\u308B\u3002\u56FD\u969B\u5358\u4F4D\u7CFB\u3067\u306F W\u3001CGS\u5358\u4F4D\u7CFB\u3067\u306F erg/s \u3067\u8868\u3055\u308C\u308B\u3002\u307E\u305F\u3001\u592A\u967D\u306E\u5149\u5EA6 L\u2609 (= 3.827\u00D71026 W) \u3092\u5358\u4F4D\u3068\u3059\u308B\u3053\u3068\u3082\u591A\u3044\u3002\u5929\u4F53\u306E\u898B\u304B\u3051\u306E\u660E\u308B\u3055\u306F\u8DDD\u96E2\u306E2\u4E57\u306B\u53CD\u6BD4\u4F8B\u3057\u3066\u6697\u304F\u306A\u308B\u304C\u3001\u5149\u5EA6\u306F\u5929\u4F53\u307E\u3067\u306E\u8DDD\u96E2\u306B\u3088\u3089\u306A\u3044\u56FA\u6709\u306E\u91CF\u3067\u3042\u308B\u3002\u5929\u4F53\u306E\u660E\u308B\u3055\u306F\u666E\u901A\u3001\u5BFE\u6570\u30B9\u30B1\u30FC\u30EB\u306E\u898B\u304B\u3051\u306E\u7B49\u7D1A\u3092\u7528\u3044\u3066\u6E2C\u3089\u308C\u308B\u3002 \u6052\u661F\u306E\u660E\u308B\u3055\u3092\u6E2C\u5B9A\u3059\u308B\u5834\u5408\u3001\u5149\u5EA6\u30FB\u898B\u304B\u3051\u306E\u7B49\u7D1A\u30FB\u8DDD\u96E2\u306F\u4E92\u3044\u306B\u95A2\u4FC2\u306E\u3042\u308B\u5909\u6570\u3067\u3042\u308B\u3002\u3053\u306E3\u3064\u306E\u5909\u6570\u306E\u3046\u30612\u3064\u3092\u77E5\u308B\u3053\u3068\u304C\u3067\u304D\u308C\u3070\u6B8B\u308A\u306E\u4E00\u3064\u3092\u6C7A\u3081\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002\u5149\u5EA6\u306E\u57FA\u6E96\u3068\u3057\u3066\u592A\u967D\u306E\u5024\u3092\u7528\u3044\u308B\u5834\u5408\u304C\u591A\u3044\u306E\u3067\u3001\u592A\u967D\u306E\u898B\u304B\u3051\u306E\u7B49\u7D1A\u3068\u592A\u967D\u307E\u3067\u306E\u8DDD\u96E2\u3092\u76EE\u7684\u306E\u5929\u4F53\u3067\u306E\u5024\u3068\u6BD4\u8F03\u3059\u308C\u3070\u6700\u3082\u7C21\u5358\u306B\u5404\u5909\u6570\u3092\u8A08\u7B97\u3067\u304D\u308B\u3002 \u6E2C\u5149\u306E\u5206\u91CE\u3067\u4F7F\u308F\u308C\u308B\u5149\u5EA6\uFF08\u82F1\u8A9E: luminous intensity\uFF09\u3068\u306F\u5225\u306E\u6B21\u5143\u3092\u6301\u3064\u7570\u306A\u308B\u91CF\u3067\u3042\u308B\u3002"@ja . . .