Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law

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Sernav	Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law
Danasîn	The goals of this activity are to understand thermal spectra, to understand Wien’s Law and the Stephan-Boltzmann Law, to understand how thermal spectra can be used to evaluate the temperature of a star and to understand how temperature and radius of a star determine a star’s luminosity
Mijar	Fezazanî
Ast	Zanîngeh - Destpêk
Cure	Ezmûngeh
Dem	60 xulek
Bersîvan Dihewîne	Na
Ziman	Îngilizî
Peyvên Girîng	Stephan-Boltzmann Law. wavelength, Wein's Law, light intensity, stellar luminosity, stellar temperature, thermal spectrum
Şêwekar	Blackbody Spectrum