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Many stars are members of binary or multiple systems, and many also vary in brightness.
supportedMany stars are members of binary or multiple systems, and many also vary in brightness. Binary stars provide the most direct stellar mass measurements and calibrate stellar models.
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Evidence first
Many stars are members of binary or multiple systems, and many also vary in brightness.
supportedTwo bound stars orbit their common center of mass according to gravity.
supportedPeriodic radial-velocity shifts reveal orbital periods and velocity amplitudes, while eclipse light curves constrain radii and inclination.