
An object in uniform circular motion is accelerating toward the centre of orbit, O. Between A and B, the horizontal component of motion changes from v sinθ to –v sinθ




By taking the limit of angular displacement as zero, we can derive an equation for the instantaneous centripetal acceleration of the object at point C

This seems like a complicated derivation, but there is no maths in there that you haven't been introduced to already. It is important you know how to use the vector diagrams to reach the final equations for angular accelerations, understanding every step along the way. Try and do it without the notes to help memorise and see how far you get!
The acceleration of an object towards the centre of a circle when an object is in motion (rotating) around a circle at a constant speed

v = r⍵




Centripetal acceleration is always directed toward the centre of the circle, and is perpendicular to the object’s velocity
A ball tied to a string is rotating in a horizontal circle with a radius of 1.5 m and an angular speed of 3.5 rad s−1.
Calculate its centripetal acceleration if the radius was twice as large and angular speed was twice as fast.

Make sure you understand both the derivation and how to use the equation for centripetal acceleration. The most crucial step is to remember the small angle approximation, that sin θ is approximately equal to θ when the angle is very very small. Try this in your calculator (in radians!) and see for yourself!
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