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 |
Skule / Organisasjon | New York University |
Lasta opp | 18.07.14 |
Oppdatert | 27.10.14 |