s8pe-41402-ca 10/31/05 7:11 PM MAZER Page 466 Star Systems Unlike our Sun, most stars do not exist alone. Instead, they are grouped with one or more companion stars. The stars are held together by the force of gravity between them. A binary star system consists of two stars that orbit each other. A multiple star system consists of more than two stars. In many star systems, the stars are too close together to be seen individually. However, astronomers have developed ways of detecting such systems. For example, in a binary star system, one of the stars may orbit in front of the other when viewed from Earth. The star that orbits in front will briefly block some of the other star’s light, providing a clue that more than one star is present. The illustration at right shows a binary star system that can be detected this way. Sometimes astronomers can also figure out whether a star is really a star system by studying its spectrum. Binary Star System Some binary star systems appear to dim briefly when one star orbits in front of the other and blocks some of its light. When neither star is in front of the other, the star system appears to give off more light. Star systems are an important source of information about star masses. Astronomers cannot measure the mass of a star directly. However, they can figure out a star’s mass by observing the effect of the star’s gravity on a companion star. Check Your Reading Why are star systems important to astronomers? KEY CONCEPTS CRITICAL THINKING 1. Why must astronomers figure out a star’s distance to calculate its actual brightness? (8.4.c) 4. Analyze Some of the brightest stars are red supergiants. How can stars with cooler red surfaces be so bright? 2. How are color and temperature related in stars? (8.4.b) 3. How does a star’s mass affect its life cycle? (8.4.b) 466 Unit 4: Space Science 5. Infer Will the Sun eventually become a black hole? Why or why not? CHALLENGE 6. Infer At what stage in the life cycle of the Sun will it be impossible for life to exist on Earth? Explain. PDF
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