Here are the essential concepts you must grasp in order to answer the question correctly.
Gravitational Force
Gravitational force is the attractive force between two masses, calculated using Newton's law of universal gravitation. For an object near the Earth's surface, this force can be simplified to F = mg, where m is the mass of the object and g is the acceleration due to gravity (approximately 9.81 m/s²). In this scenario, the gravitational force acting on the ball can be determined by multiplying its mass (0.5 kg) by g.
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Centripetal Force
Centripetal force is the net force required to keep an object moving in a circular path, directed towards the center of the circle. It is essential for understanding the dynamics of the ball as it moves in a vertical circle. The centripetal force can be calculated using the formula F_c = mv²/r, where m is the mass, v is the speed, and r is the radius of the circle. At different points in the circle, the gravitational force and tension in the string contribute to this centripetal force.
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Energy Conservation
The principle of energy conservation states that the total mechanical energy of an isolated system remains constant if only conservative forces are acting. In the context of the ball moving in a vertical circle, potential energy (due to height) and kinetic energy (due to speed) interchange as the ball moves. At the top and bottom of the circle, the speeds and heights change, but the total energy (kinetic + potential) remains constant, allowing for the calculation of speeds at different points.
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