Introductory Astronomy - Luminosity, Temperature, and Surface Area
Offered By: Professor Paul Robinson via YouTube
Course Description
Overview
Explore the fundamental concepts of stellar physics in this 16-minute video lecture, delving into the intricate relationship between luminosity, temperature, and surface area. Learn about energy, temperature scales, and the Stefan-Boltzmann Law while examining practical examples and their applications to stars. Gain insights into the Hertzsprung-Russell (HR) Diagram and its significance in understanding stellar properties and evolution.
Syllabus
Introduction
Energy
Temperature
Kelvin vs Celsius
Luminosity
StefanBoltzmann Law
Surface Area
Examples
Stars
HR Diagram
Taught by
Professor Paul Robinson
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