A graphical approach to understanding the form of the centripetal acceleration.
Assumptions
We assume that we have uniform circular motion (motion with a constant radius and a constant speed centered at a fixed point in space).
The Diagram
The picture below illustrates the motion, with coordinates chosen so that the angular position at t = 0 is θ = 0.
To the right of the motion diagram is a vector diagram that shows the change in the velocity vector. The picture motivates the conclusion that if we take a very small Δt, the change in the velocity approaches:
![](/confluence/download/export/latex10032037550851924436.png)
In the infinitesimal limit, this equation becomes:
![](/confluence/download/export/latex12805839493985681453.png)
Using the fact that for uniform circular motion,
![](/confluence/download/export/latex14353037669556333183.png)
we arrive at the form of the centripetal acceleration:
![](/confluence/download/export/latex4204264030683513425.png)
Analogy with Gyroscopic Precession
Consider a gyroscope precessing. The angular momentum will trace out a circle as shown below.
The similarity to the Δv diagram implies that we can write:
![](/confluence/download/export/latex12862084999507248987.png)
where the derivative of φ with respect to time is the angular frequency of precession, usually written as Ω:
![](/confluence/download/export/latex5969717176321899107.png)
Fundamental Relationship for Gyroscopes
With that substitution, we have arrived at the fundamental relation for gyroscopes:
![](/confluence/download/export/latex13803008133461911747.png)