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Stellar Mass
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Alcor Mizar (Binary star) Ursa Major
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Gravitational Orbits Animation
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Binary star (system): two stars orbiting a common
center of mass (CM). 1 r1 r2 CM 2 r2 = 3 AU, r1 = 1 AU
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Kepler’s laws apply here . . .
Yuk! P: years a: AU M: Solar Masses
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a = r1 + r2 = 4 AU Suppose: P = 8 yrs . . . 1 M
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“Seeing” Binary Stars Visual Binary: Two stars seen in telescope e.g., Mizar Albireo
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Sirius A & B A B
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0.0034 L 0.16 M Distance = 13 ly P = 44.6 yrs a = 9.5 AU A B
Kruger 60 L M A B 0.01 L L 0.28 M 0.16 M
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2. Spectroscopic Binary: Motion of stars
detected via Doppler shift of spectrum lines. Mizar Each star is itself binary!
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Earth * Doppler shift * No Doppler shift
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Spectroscopic Binary Animation
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Eclipsing Binary: Stars mutually eclipse each other. * No eclipse * Eclipse Earth
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Binary ‘light curve’ Brightness Time ½ orbit period
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Eclipsing Binary Animation
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Binary Statistics * At least 50% of all stars reside in binaries. * The sun is apparently a loner!
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