Circular Motion
Circular Motion Basics
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Circular motion refers to the movement of an object along the circumference of a circle or rotation along a circular path.
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It can be uniform, with a constant angular rate, or non-uniform, with a changing rate of rotation.
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The rotating object maintains a constant distance from a central point, often termed the centre of rotation.
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Circular movement is a result of a centripetal force, directing toward the centre and causing the object to follow a circular path.
Centripetal Force
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Centripetal force is a force that makes a body follow a curved path—specifically in a circular path.
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Its direction is always orthogonal to the motion of the body and towards the fixed point of the instantaneous centre of curvature of the path.
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Centripetal force is calculated using the formula: F = mv^2/r, where:
- m = mass of the object,
- v = velocity of the object,
- r = radius of the circular path.
Centrifugal Force
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In some cases, you may come across the concept of centrifugal force.
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Centrifugal force is often considered a “fictitious” force. It does not come into play when analysing an object’s motion from an inertial reference frame.
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However, it’s sometimes useful when analysing motion from a rotating perspective (a non-inertial reference frame).
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You may think of it as an “outward force” that balances the centripetal force in a rotating system.
Angular Velocity and Acceleration
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Angular velocity is the rate of change of an angle with respect to time. It is represented as ω and given by the formula: ω = Δθ/Δt.
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Angular acceleration is the rate of change of angular velocity with respect to time. It is represented as α and is given by the formula: α = Δω/Δt.
Tangential Velocity and Acceleration
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Tangential velocity is the linear speed of any object moving along the circular path. It is perpendicular to the radius of the path.
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Tangential acceleration is the rate of change of the tangential velocity. It points along the curve in the direction of the velocity vector.
Some Practical Circular Motion Scenarios
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In reality, many motions are circular, such as the rotation of planets around stars, electrons around nuclei, and cars rounding bends.
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It’s crucial to understand that circular motion, whether uniform or non-uniform, involves acceleration. Even if the speed stays constant, the object is accelerating because its direction of motion is constantly changing.