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 |
Nivîskar | Rhoda Berenson |
Dibistan / Organîzasyon | New York University |
Şandin | 7/18/14 |
Rojanekirin | 10/27/14 |