Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law
Download Tous les fichiers sous forme d'un zip compressé.
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 |
Ecole / Organisation | New York University |
Date de soumission | 18/07/14 |
Date de mise à jour | 27/10/14 |