To solve this problem, it is necessary to apply the concepts related to angular momentum and express these units in a way related to the values we have. Mathematically and initially it can be expressed as,
[tex]L = mvr[/tex]
Here,
m = mass
v = Linear velocity
r = Radius
We know that linear speed is the product of angular speed times radius, so the expression can be converted
[tex]L = mr^2\omega[/tex]
At the same the expression representing the angular velocity in terms of the period,
[tex]L = mr^2 (\frac{2\pi}{T})[/tex]
[tex]L = \frac{(5.49*10^{22})(2.32*10^8)^2(2 \pi)}{(21.2)(24)(3600)}[/tex]
[tex]L = 1.01363*10^{34} kg \cdot m^2/s[/tex]
Therefore the angular momentum of the moon about the planet is [tex]1.013*10^{34} kg\cdot m^2/s[/tex]