A Classical Approach of Newtonian Mechanics

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7 CIRCULAR MOTION 7.5 Non-uniform circular motion


Comparing with Eq. (7.28), recalling that e i θ represents er and i e i θ represents
eθ, we obtain


ar = ̈r − r θ ̇^2 = ̈r − r ω^2 , (7.41)
aθ = r θ ̈^ + 2 ̇r θ ̇^ = r ω ̇ + 2 ̇r ω. (7.42)

Thus, we now have expressions for the object’s radial and tangential accelerations


in terms of r and θ. The beauty of this derivation is that the complex analysis
has automatically taken care of the fact that the unit vectors er and eθ change
direction as the object moves.


Let us now consider the commonly occurring special case in which an object
executes a circular orbit at fixed radius, but varying angular velocity. Since the


radius is fixed, it follows that ̇r = ̈r = 0. According to Eqs. (7.3 8 ) and (7.3 9 ), the
radial velocity of the object is zero, and the tangential velocity takes the form


vθ = r ω. (7.43)

Note that the above equation is exactly the same as Eq. (7.6)—the only difference


is that we have now proved that this relation holds for non-uniform, as well as
uniform, circular motion. According to Eq. (7.41), the radial acceleration is given


by


ar = −r ω^2. (7.44)

The minus sign indicates that this acceleration is directed towards the centre


of the circle. Of course, the above equation is equivalent to Eq. (7.15)—the only


difference is that we have now proved that this relation holds for non-uniform, as


well as uniform, circular motion. Finally, according to Eq. (7.42), the tangential


acceleration takes the form


aθ = r ω ̇. (7.45)

The existence of a non-zero tangential acceleration (in the former case) is the


one difference between non-uniform and uniform circular motion (at constant


radius).

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