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


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Tittel Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law
Omtale 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
Emne Astronomi
Nivå Student - introduksjon (bachelor)
Type Lab
Tid 60 minutt
Inneheld svar Nei
Språk English
Nøkkelord Stephan-Boltzmann Law. wavelength, Wein's Law, light intensity, stellar luminosity, stellar temperature, thermal spectrum
Simuleringar Blackbody Spectrum


Forfattarar Rhoda Berenson
E-post for kontakt rb143@nyu.edu
Skule / Organisasjon New York University
Lasta opp 18.07.14
Oppdatert 27.10.14