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


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Pavadinimas Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law
Aprašymas 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 Astronomija
Lygis Bakalauras - įžanga
Tipas Lab
Trukmė 60 minutės
Įtraukti Atsakymai Ne
Kalba Anglų
Raktažodžiai Stephan-Boltzmann Law. wavelength, Wein's Law, light intensity, stellar luminosity, stellar temperature, thermal spectrum
Simuliacija(-os) Blackbody Spectrum


Autorius (-ai) Rhoda Berenson
Kontaktinis Elektroninis paštas rb143@nyu.edu
Mokykla / Organizacija New York University
Pateikimo data 14.7.18
Data atnaujinta 14.10.27