To solve this problem it is necessary to apply the concepts related to the acceleration of gravity due to the force exerted by a start and the calculation of angular velocity as a function of acceleration and radius.
By definition we know that the acceleration exerted by the celestial body is given under the equation
[tex]g = \frac{GM}{R^2}[/tex]
Where,
G = Gravitational Universal Constant
M = Mass
R = Radius
The radius of Europa is
[tex]R = \frac{D}{2} = \frac{31838*10^3}{2}[/tex]
[tex]R = 1569*10^3m[/tex]
Applying the gravitational equation,
[tex]g = \frac{GM}{R^2}[/tex]
[tex]g = \frac{(6.67*10^{-11})(4.8*10^{22})}{(1569*10^3)^2}[/tex]
[tex]g = 1.3m/s^2[/tex]
Therefore the angular acceleration can be obtained through the kinematic equation
[tex]a = r\omega^2[/tex]
Where,
a = acceleration
r = length of the arm
[tex]\omega =[/tex] Angular acceleration
As a = g then,
[tex]g = r\omega^2[/tex]
Where,
[tex]\omega = \sqrt{\frac{g}{r}}[/tex]
[tex]\omega = \sqrt{\frac{1.3}{4.25}}[/tex]
[tex]\omega = 0.553rad/s[/tex]
Therefore the angular speed of arm is 0.553rad/s