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
E-peyama Peywendiyê rb143@nyu.edu
Dibistan / Organîzasyon New York University
Şandin 7/18/14
Rojanekirin 10/27/14