Semimajor axis of the comets orbit


Comet orbits are highly elliptical. A periodic comet orbiting a two solar mass star with an orbital period of 200 years comes to a periastron distance of 0.7 AU. Using only Keplers third law calculate a) the semimajor axis of the comet's orbit b) the comet's apastron distance

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Physics: Semimajor axis of the comets orbit
Reference No:- TGS0720500

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