To solve this problem it is necessary to apply the concepts related to gravity as an expression of a celestial body, as well as the use of concepts such as centripetal acceleration, angular velocity and period.
PART A) The expression to find the acceleration of the earth due to the gravity of another celestial body as the Moon is given by the equation
[tex]g = \frac{GM}{(d-R_{CM})^2}[/tex]
Where,
G = Gravitational Universal Constant
d = Distance
M = Mass
[tex]R_{CM} =[/tex] Radius earth center of mass
PART B) Using the same expression previously defined we can find the acceleration of the moon on the earth like this,
[tex]g = \frac{GM}{(d-R_{CM})^2}[/tex]
[tex]g = \frac{(6.67*10^{-11})(7.35*10^{22})}{(3.84*10^8-4700*10^3)^2}[/tex]
[tex]g = 3.4*10^{-5}m/s^2[/tex]
PART C) Centripetal acceleration can be found throughout the period and angular velocity, that is
[tex]\omega = \frac{2\pi}{T}[/tex]
At the same time we have that centripetal acceleration is given as
[tex]a_c = \omega^2 r[/tex]
Replacing
[tex]a_c = (\frac{2\pi}{T})^2 r[/tex]
[tex]a_c = (\frac{2\pi}{26.3d(\frac{86400s}{1days})})^2 (4700*10^3m)[/tex]
[tex]a_c = 3.34*10^{-5}m/s^2[/tex]