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| Opis | Hertzsprung–Russell diagram. A plot of luminosity (absolute magnitude) against the colour of the stars ranging from the high-temperature blue-white stars on the left side of the diagram to the low temperature red stars on the right side. "This diagram below is a plot of 22000 stars from the Hipparcos Catalogue together with 1000 low-luminosity stars (red and white dwarfs) from the Gliese Catalogue of Nearby Stars. The ordinary hydrogen-burning dwarf stars like the Sun are found in a band running from top-left to bottom-right called the Main Sequence. Giant stars form their own clump on the upper-right side of the diagram. Above them lie the much rarer bright giants and supergiants. At the lower-left is the band of white dwarfs – these are the dead cores of old stars which have no internal energy source and over billions of years slowly cool down towards the bottom-right of the diagram." Converted to png and compressed with pngcrush. |
| Izvor | The Hertzsprung Russell Diagram |
| Autor | Richard Powell |
| Dopuštenje (Ponovna upotreba ove datoteke) |
   Ova datoteka je licencirana pod Creative Commons Attribution-Share Alike 2.5 generičkom licencom.
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This diagram image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with
{{vector version available|new image name}}.It is recommended to name the SVG file “HRDiagram.svg”—then the template Vector version available (or Vva) does not need the new image name parameter. |
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| Datum/vrijeme | Minijatura | Dimenzije | Korisnik | Komentar | |
|---|---|---|---|---|---|
| aktualna | 18. maja 2011. u 20:32 | | 720 × 820 (19 kB) | wikimediacommons>Saibo | Reverted to version as of 03:42, 3 March 2007. Commons:Avoid_overwriting_existing_files |
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