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Stellar Mass.

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Presentation on theme: "Stellar Mass."— Presentation transcript:

1 Stellar Mass

2 Alcor Mizar (Binary star) Ursa Major

3 Gravitational Orbits Animation

4 Binary star (system): two stars orbiting a common
center of mass (CM). 1 r1 r2 CM 2 r2 = 3 AU, r1 = 1 AU 

5 Kepler’s laws apply here . . .
Yuk! P: years a: AU M: Solar Masses

6 a = r1 + r2 = 4 AU Suppose: P = 8 yrs . . . 1 M

7 “Seeing” Binary Stars Visual Binary: Two stars seen in telescope e.g., Mizar Albireo

8 Sirius A & B A B

9 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 

10 2. Spectroscopic Binary: Motion of stars
detected via Doppler shift of spectrum lines. Mizar Each star is itself binary!

11

12 Earth * Doppler shift * No Doppler shift

13 Spectroscopic Binary Animation

14 Eclipsing Binary: Stars mutually eclipse each other. * No eclipse * Eclipse Earth

15 Binary ‘light curve’ Brightness Time ½ orbit period

16 Eclipsing Binary Animation

17 Binary Statistics * At least 50% of all stars reside in binaries. * The sun is apparently a loner!


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