A satellite of mass m is in a circular orbit at radius r around Earth. What force keeps the satellite in orbit, and in which direction relative to the radius?

Study for the Newton's Laws of Motion Test. Engage with multiple choice and interactive questions, each hinting at concepts with detailed explanations. Master the principles and ace your exam!

Multiple Choice

A satellite of mass m is in a circular orbit at radius r around Earth. What force keeps the satellite in orbit, and in which direction relative to the radius?

Explanation:
Gravity from Earth provides the inward force that keeps the satellite moving in a circle. This gravitational pull points along the radius toward Earth's center, supplying the centripetal acceleration needed for circular motion. In a circular orbit the required inward force is m v^2 / r, and gravity provides F_g = G M_e m / r^2 in that inward direction, so the orbit remains stable. The outward options would imply a force pulling away, which isn’t present in free space, and a tension or normal force would require a tether or contact with a surface, neither of which applies to a satellite in orbit.

Gravity from Earth provides the inward force that keeps the satellite moving in a circle. This gravitational pull points along the radius toward Earth's center, supplying the centripetal acceleration needed for circular motion. In a circular orbit the required inward force is m v^2 / r, and gravity provides F_g = G M_e m / r^2 in that inward direction, so the orbit remains stable. The outward options would imply a force pulling away, which isn’t present in free space, and a tension or normal force would require a tether or contact with a surface, neither of which applies to a satellite in orbit.

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