LEVELJEE Main
Visualized Solution
The Sigma Insight: Orbital Motion of a Satellite
The Delicate Dance of Orbit
Imagine a satellite gracefully orbiting the Earth. It's moving at a tremendous speed, yet it doesn't fly off into the abyss of space. Why? Because of a delicate balance.
The satellite has a tangential velocity—it wants to go straight. However, the Earth's gravity acts as an invisible tether, constantly pulling the satellite towards the center. This inward pull provides the necessary centripetal force (), which continuously bends the satellite's path into a circle.
The Thought Experiment
Turning Off Gravity
Now, the problem asks us to imagine a scenario straight out of science fiction: what if the gravitational force of attraction suddenly becomes zero?
Let's visualize this. The invisible tether snaps. The centripetal force that was forcing the satellite to turn is instantly gone.
Newton's First Law Takes the Wheel
To understand what happens next, we must consult Sir Isaac Newton. His First Law of Motion (the law of inertia) states that an object in motion will stay in motion with the same speed and in the same direction unless acted upon by an unbalanced force.
While the satellite was in orbit, gravity was that unbalanced force changing its direction. But the moment gravity vanishes, the net force on the satellite becomes zero.
The Final Trajectory
Without any force to bend its path, the satellite's inertia takes over completely. It will continue moving in the exact direction it was heading at the instant gravity disappeared.
Since its velocity vector was tangential to the circular orbit at that moment, the satellite will fly off in a straight line, tangentially to the original orbit.
Furthermore, because there is no force acting along its direction of motion to speed it up or slow it down, it will continue with the same velocity it had. It becomes a free-floating object in deep space, traveling in a straight line forever!
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