Using Kepler's third law, if two binary star systems have identical masses, then the system that has a separation distance twice as large as the other will have $a (n)$ orbital period. larger smaller equal indeterminable (based on the given information)

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Using Kepler's third law, if two binary star systems have identical masses, then the system that has a separation distance twice as large as the other will have

a (n)

orbital period. larger smaller equal indeterminable (based on the given information)

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