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:
[tex]y^2+x^2=r^2[/tex]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:
[tex]v=\sqrt[]{x^{\prime}^2+y^{\prime2}}[/tex]Substituting:
[tex]v=r\theta^{\prime}[/tex]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:
[tex]\theta^{\prime}=\frac{2\pi}{655.6}=0.0095839\text{ rad/h}[/tex]Finally, the linear speed is:
[tex]\begin{gathered} v=2.5\cdot10^5\cdot0.0095839 \\ v=2,396\text{ mi/h} \end{gathered}[/tex]