A cow in orbit around the moon can be used to determine the moon's mass by applying principles of rotational motion and centripetal force. Key concepts include Newton's Law of Universal Gravitation and the relationships between centripetal acceleration, radius, and orbital period. The discussion emphasizes solving symbolically for the moon's mass using variables related to the cow's speed and distance from the moon's center. Assumptions about the cow's orbit are necessary for a numeric solution, but a symbolic approach suffices for the problem. The engaging nature of the question highlights the creativity of the teacher in presenting physics concepts.