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Stars Mr. Skirbst Physical Science Topic 25
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Stars Composition: - determined by spectral analysis - hydrogen (60 – 80%) - helium (20 – 30%) - other (O, C, Ne, N)
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Star size Supergiants * 1,000x size of the sun (ex. Rigel)
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Star size Giants * 10 - 100x size of the sun (ex. Aldebaran)
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Star size Medium (Main-Sequence) * same size of the sun (ex. Sun, Sirius)
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Star size White Dwarfs * smaller than the Earth (ex. Van Maanens)
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Star size Neutrons * only several kilometers in diameter * a teaspoon would have a mass greater than the entire Earth!
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Relative Star Sizes Giant Star Neutron White dwarf Medium-sized Supergiant
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Star temperature Color of star can help determine the surface temperature of stars COLORTEMP (oC) Blue35,000 White10,000 Yellow6,000 Red-Orange5,000 Red3,000
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Star brightness Absolute brightness (magnitude) - light actually given off Apparent brightness (magnitude) - light observed by someone
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H-R Diagram Hertzsprung-Russell Diagram * Relates absolute magnitude and surface temperature of stars H-R DiagramH-R Diagram H-R Diagram AnimationH-R Diagram Animation
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Star Distances Parallax Method
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Parallax
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