A heliocentric system is a sun-centered
centripetal acceleration is given by formula

given that


now we have




so the ratationa frequency is given by




Answer: The Earth and you are attracted to the centers of each other by a pair of equal gravitational forces. The size of the force attracting you toward the center of the Earth is your "weight" on Earth. The size of the force attracting the Earth toward the center of you is the Earth's "weight" on you.
Explanation:
Answer:
athe answer to this question is Synex BA-315