The total mass of a binary system can be calculated from a. the ratio of the angular separation from the center of mass of each of the stars. b. the distance to the binary and its radial velocity. c. the semi major axis and period of the orbit. d. the radial velocities of the two stars. e. the time required for the small star to eclipse the larger star.
The total mass of a binary system can be calculated from a. the ratio of the angular separation from the center of mass of each of the stars. b. the distance to the binary and its radial velocity. c. the semi major axis and period of the orbit. d. the radial velocities of the two stars. e. the time required for the small star to eclipse the larger star.
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The total mass of a binary system can be calculated from
| a. |
the ratio of the angular separation from the center of mass of each of the stars.
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| b. |
the distance to the binary and its radial velocity.
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| c. |
the semi major axis and period of the orbit.
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|
| d. |
the radial velocities of the two stars.
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|
| e. |
the time required for the small star to eclipse the larger star.
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