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


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Titre Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law
Description 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
Sujet Astronomie
Niveau Premier cycle - Intro
Type Labo
Durée 60 minutes
Réponses incluses Non
Langue Anglais
Mots clés Stephan-Boltzmann Law. wavelength, Wein's Law, light intensity, stellar luminosity, stellar temperature, thermal spectrum
Simulation(s) Spectre du corps noir


Auteur(s) Rhoda Berenson
Email de contact rb143@nyu.edu
Ecole / Organisation New York University
Date de soumission 18/07/14
Date de mise à jour 27/10/14