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There are MORE than 200 billion, billion stars in a universe. Most stars contain mainly hydrogen and helium. I. Color of a star: tells what the surface temperature of the star is HOTTEST STAR: shines with a blue-white light COOLEST STAR: shines with a red light Star Temperatures http://www.eudesign.com/mnems/startemp.htm http://www.geocities.com/SummerDale33/Mnemonic.html Star Type OUR SUN O B A F G K M K Temperature ◦C ◦F > 25,000 > 24,727 > 44,540 11,000 – 25,000 10,727 – 24,727 19,340 – 44,540 7,500 – 11,000 7,227 – 10,727 13,040 – 19,340 6,000 – 7,500 5,727 – 7,227 10.340 – 13,040 5,000 – 6,000 4,727 – 5,727 8,540 – 10,340 3,500 – 5,000 3,227 – 4,727 5,840 – 8,540 < 3,500 < 3,227 < 5,840 Color blue blue white yellow yellow red red II. Magnitude: star’s brightness (luminosity) Absolute Magnitude The actual brightness of a star How bright it IS Apparent Magnitude The brightness of a star as viewed from Earth How bright it SEEMS Apparent magnitude affected by: –Distance –Size –Temperature H-R Diagram --illustrates the relationship that exists between the average surface temperature of stars and their absolute magnitude. As absolute magnitude(brightness) increases, surface temperature increases. Star Brightness vs Temperature