Difference between revisions of "Hertzsprung–Russell diagram"
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[[Image:Hertzsprung-Russell.jpg|thumb|300px|right|Hertzsprung-Russell diagram]] | [[Image:Hertzsprung-Russell.jpg|thumb|300px|right|Hertzsprung-Russell diagram]] | ||
The '''Hertzsprung–Russell diagram''' is a type of chart showing the connection of temperature and brightness in stars. The diagram illustrates three groups of stars; the main sequence, the giants and supergiants, and the white dwarfs. It is named after the astronomers [[Ejnar Herzsprung]] and [[Henry Russell]]<ref> ''Universe: The Definitive Visual Guide'' (2005), DK Publishing , page 232.</ref> | The '''Hertzsprung–Russell diagram''' is a type of chart showing the connection of temperature and brightness in stars. The diagram illustrates three groups of stars; the main sequence, the giants and supergiants, and the white dwarfs. It is named after the astronomers [[Ejnar Herzsprung]] and [[Henry Russell]]<ref> ''Universe: The Definitive Visual Guide'' (2005), DK Publishing , page 232.</ref> | ||
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==References== | ==References== | ||
<references> | <references> | ||
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| + | [[Category:Astronomy]] | ||
| + | [[Category:Physics]] | ||
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Revision as of 22:06, January 6, 2017
The Hertzsprung–Russell diagram is a type of chart showing the connection of temperature and brightness in stars. The diagram illustrates three groups of stars; the main sequence, the giants and supergiants, and the white dwarfs. It is named after the astronomers Ejnar Herzsprung and Henry Russell[1]
References
<references>
- ↑ Universe: The Definitive Visual Guide (2005), DK Publishing , page 232.