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Velocity is a vector quantity. Its magnitude is called speed and also it has a direction. A body of mass m is moving in a circular path of radius r. There are two possibilities:
If the speed is constant, the motion is called uniform circular motion. Speed is constant but the direction is changing continuously, so the motion is accelerated. And the acceleration is along the radius towards the center.
This acceleration is called centripetal acceleration or even radial acceleration and is given by the relation:
a = v^{2} / r
Where v is the speed. The direction of velocity is along the tangent to the circular path. Thus it changes as the body is at different positions at different times.
Centripetal force = Mass x Centripetal Acceleration
The relation between linear velocity v and angular velocity ω is v = ωr where ω = 2πf
f is the frequency of revolution (units rev/s) ω has the units rad/s
Since cetripetal force is always perpendicular to the velocity, it can not change the magnitude of velocity (speed) or it can not change its speed. It can only change its direction, thus making it move in circular path with constant speed.
Other relations for F:
Since v = ωr
Also
To change the speed of the body in circular motion, a tangential force has to be applied. If it acts along the direction of velocity, it will increase its speed, On the other hand if it acts opposite to the direction of velocity it will slow it down. Now the motion is called nonuniform circular motion
Net acceleration
In nonuniform circular motion, speed as well as direction changes continuously.
Consider that there are a number of particles forming a system, such that, when an external force is applied, the complete system moves as on. Now, if we are able to replace all these particles by just one particle. And, this new particle is placed in such a manner and has such a mass, that when acted on by an external force, it moves exactly in the same manner as the system it replaced. Then, we have found the center of mass of the system. (This sounds more complex than it is. So don't worry! read on)
Let us now consider two particles. Let them have masses m_{1} and m_{2}. Let r_{1}(t) and r_{2}(t) be the position vectors of the two particles at the instant of time t. (Note: On a web page it is difficult to use the usual vector notation. So I will use bold fonts to depict vectors). The position vector R_{c.m.}(t), giving the center of mass of this system is given by the formula.
R_{c.m.}(t) = {m_{1}r_{1}(t) + m_{2}r_{2}(t)} / (m_{1} + m_{2})
from the above it is obvious that for a two particle system the center of mass always lies between the two particles. It also lies on the line joining the two particles.
R_{c.m.}(t) = {m_{1}r_{1}(t) + m_{2}r_{2}(t) +  m_{n} r_{n}(t)} / (m_{1} + m_{2 }+  m_{n})
The position of the center of mass of a rigid body is a fixed point. This point may or may not lie in the body. Where is lies depends upon the shape of the body. For example of we take the case of a ring. The center of mass will lie at its geometrical center. Obviously this point does not lie in the ring.
Body  Center of mass  
Rod 
Mid point of rod 

Ring 
Center of ring 

Sphere 
Center of sphere 
Average angular velocity = Angular displacement / time interval
So if ω is the average angular velocity, θ the angular displacement and t the time interval. We can say
So we can write the instantaneous angular velocity as dθ /dt
Linear velocity = Radius of the circular path x Angular velocity
Average angular acceleration = Change in angular acceleration / Time interval
Linear acceleration = Radius of the circular path x Angular acceleration