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Hertzsprung–Russell (H-R) Diagrams DocumentsThis material has 2 associated documents. Select a document title to view a document's information. Main DocumentHertzsprung–Russell (H-R) Diagrams
written by
Mario Belloni The Hertzsprung–Russell (H-R) Diagrams model simulates Hertzsprung–Russell (HR or H-R) diagram for groups of stars. The diagram is a scatter plot of steller luminosity vs. stellar temperature. The luminosity of stars is proportional to the star's radius squared and its temperature to the fourth power, and for Main Sequence stars, their luminosity is also proportional to their mass to the 3.5 power. Since the range of stellar luminosities and stellar temperatures is so large, the plot uses a log-log scale. The diagram is a way to understand stellar evolution.
Last Modified June 6, 2014
This file has previous versions. Source Code DocumentsHertzsprung–Russell (H-R) Diagrams Source CodeThe source code zip archive contains an XML representation of the Hertzsprung–Russell (H-R) Diagrams Model. Unzip this archive in your EJS workspace to compile and run this model using EJS.
Published November 11, 2010
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