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


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Título Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law
Descrición 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
Tema Astronomía
Nivel Universitario - Inicio
Tipo Laboratorio
Duración 60 minutos
Respostas incluidas Non
Linguaxe English
Palabras clave Stephan-Boltzmann Law. wavelength, Wein's Law, light intensity, stellar luminosity, stellar temperature, thermal spectrum
Simulacións Espectro do Corpo Negro


Autores Rhoda Berenson
Email de Contacto rb143@nyu.edu
Centro Escolar / Institución New York University
Presentado 7/18/14
Actualizado 10/27/14