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


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سه‌ردێر 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
Subject ئه‌ستێره‌ناسی
ئاست Undergrad - Intro
Type تاقیگه‌
Duration 60 خوله‌ک
Answers Included نا
زوان English
Keywords Stephan-Boltzmann Law. wavelength, Wein's Law, light intensity, stellar luminosity, stellar temperature, thermal spectrum
شێوه‌کاریه‌کان Blackbody Spectrum


نووسه‌ران Rhoda Berenson
به ئیمێل پێوه‌ندی بگرن rb143@nyu.edu
قوتابخانه‌/ ڕێکخراو New York University
ناردراو 7/18/14
به‌ڕۆژ بوه‌ 10/27/14