Circular Motion
When a body has a uniform circular motion, its distance to a fixed point is always the same and it travels at equal angles in equal amounts of time.
We are given the equation of a circle as:

Where x is the horizontal distance and y is the vertical distance. The parametric equations for this motion are:
x = r cos θ
y = r sin θ
Differentiating with respect to time:
x' = -r sin θ θ'
y' = r cos θ θ'
Where θ' is the angular speed. The linear speed is defined as:
![v=\sqrt[]{x^(\prime)^2+y^(\prime2)}](https://img.qammunity.org/2023/formulas/mathematics/high-school/yp8mbrsj45xsx60ivypn9hms586y27rvek.png)
Substituting:

The angular speed is the number of radians traveled per unit of time.
The moon travels 29.8 days of 22 hours each per revolution, that is,
29.8*22 = 655.6 hours per revolution. The angular speed is:

Finally, the linear speed is:
