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描述 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.
來源 The Hertzsprung Russell Diagram
作者 Richard Powell
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Hertzsprung–Russell diagram
Sun + Sirius sparse
Well-known stars in the Milky Way
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Hertzsprung–Russell diagram

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現時2011年5月18號 (三) 18:32響2011年5月18號 (三) 18:32嘅縮圖版本720 × 820(19 KB)SaiboReverted to version as of 03:42, 3 March 2007. Commons:Avoid_overwriting_existing_files
2011年3月25號 (五) 22:17響2011年3月25號 (五) 22:17嘅縮圖版本720 × 820(59 KB)Tomruenblack labels
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2007年3月3號 (六) 03:42響2007年3月3號 (六) 03:42嘅縮圖版本720 × 820(19 KB)Falcorian{{Information |Description=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 ri

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