STARS ARE BODIES of hot,glowing gas that are born in nebulae. They vary enormously in size, mass, and temperature: diameters range from about 450 times smaller to over 1,000 times bigger
between these extremes and appears yellow. The energy released by a shining star is usually produced by nuclear fusion in the star's core. The brightness of a star is measured in magnitudes - the brighter
Star
than that of the Sun; masses range from about a 20th to 50 solar masses; and surface temperatures range from about 3,000oC to over 50,000oC. The color star is determined by its temperature: the hottest stars are blue and the coolest are red. The Sun, with a surface temperature of 5,500oC, is
Hottest star (Blue in color)
Coolest Star (Red in Color)
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Nuclear fusion in the star's core
the star, the lower is magnitude. There are two types of magnitude;
(i) Apparent Magnitude:-Brightness seen from Earth (of the stars)
(ii)Apparent Magnitude:-Brightness seen from a standard distance of 10 parsecs (32.6 light years)
The light emitted by a star may be split to form a Spectrum containing a series of dark lines (absorption lines). The patterns of lines indicate the presence of particular chemical elements,
Birth of Star
Star spectrum |
enabling astronomers to deduce the composition of the star's atmosphere. The magnitude and spectral type (color) of stars may be plotted on a graph called a Hertzsprung-Russell diagram, which shows stars tend to fall into several well-defined groups. The principal groups are main sequence stars
Hertzsprung-Russell diagram |
(those are fusing hydrogen to form helium), giants, supergiants, and white dwarfs.
Star Color Chart |
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