The masses of the bodies in orbit around each other can be measured, if we can measure the distances and periods of revolution.
Kepler's third law states that, the square of the period of a planet's orbit is proportional to the cube of its semimajor axis.
Newton reformed this law and the reformulation of Kepler's third law allows us to measure the masses of bodies in orbit around each other, if we can measure;
Thus, the masses of the bodies in orbit around each other can be measured, if we can measure the distances and periods of revolution.
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