File:ESO - Hertzsprung-Russell Diagram (by).jpg
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| Description | In the Hertzprung-Russell diagram the temperatures of stars are plotted against their luminosities. The position of a star in the diagram provides information about its present stage and its mass. Stars that burn hydrogen into helium lie on the diagonal branch, the so-called main sequence. Red dwarfs like AB Doradus C lie in the cool and faint corner. AB Dor C has itself a temperature of about 3 000 degrees and a luminosity which is 0.2% that of the Sun. When a star exhausts all the hydrogen, it leaves the main sequence and becomes a red giant or a supergiant, depending on its mass (AB Doradus C will never leave the main sequence since it burns so little hydrogen). Stars with the mass of the Sun which have burnt all their fuel evolve finally into a white dwarf (left low corner). | ||||
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| Source | Hertzsprung-Russell Diagram | ||||
| Author | ESO | ||||
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 10:42, 9 November 2008 | | 2,662 × 2,988 (1.42 MB) | ComputerHotline (talk | contribs) | {{Information |Description=In the Hertzprung-Russell diagram the temperatures of stars are plotted against their luminosities. The position of a star in the diagram provides information about its present stage and its mass. Stars that burn hydrogen into h |
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