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Summary

Description This is an example of a Hertzsprung–Russell diagram; a plot of luminosity versus spectral class for a group of stars. The diagonal band labelled "main sequence" is where dwarf stars such as the Sun spend most of their active lifespan. Red giants and supergiants are evolved stars with a mass greater than a red dwarf, that are burning elements heavier than hydrogen. However, White Dwarfs are quite dense, non-luminous, but are still less in mass than supergiants. Once this supply of fuel is exhausted, these stars will migrate to the lower left on this diagram, becoming white dwarfs.
Date (UTC)
Source Image:Hertzsprung-russel diagram.png
Author User:Rursus
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Hertzsprung–Russell diagram
Sun + Sirius sparse
Well-known stars in the Milky Way

Licensing

GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.
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30 April 2007

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Date/TimeThumbnailDimensionsUserComment
current19:38, 24 June 2009Thumbnail for version as of 19:38, 24 June 2009700 × 830 (177 KB)RursusChange sun position to something more realistical: c:a G2
19:58, 30 April 2007Thumbnail for version as of 19:58, 30 April 2007700 × 830 (168 KB)Rursus{{Information |Description= |Source= |Date= |Author= }}
19:52, 30 April 2007Thumbnail for version as of 19:52, 30 April 2007700 × 830 (168 KB)Rursus{{Information |Description= |Source= |Date= |Author= }}
19:45, 30 April 2007Thumbnail for version as of 19:45, 30 April 2007700 × 830 (165 KB)Rursus{{Information |Description=This is an example of a Hertzsprung-Russell diagram; a plot of luminosity versus spectral class for a group of stars. The diagonal band labelled "main sequence" is where dwarf stars such as the Sun spend most of their active lif

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