Answer:
Acceleration, ![a=2.22\times 10^{-3}\ m/s^2](https://tex.z-dn.net/?f=a%3D2.22%5Ctimes%2010%5E%7B-3%7D%5C%20m%2Fs%5E2)
Explanation:
It is given that,
Time period of revolution of the moon, ![T=2060\times 10^3\ s](https://tex.z-dn.net/?f=T%3D2060%5Ctimes%2010%5E3%5C%20s)
If the distance from the center of the moon to the surface of the planet is, ![h=235\times 10^6\ m](https://tex.z-dn.net/?f=h%3D235%5Ctimes%2010%5E6%5C%20m)
The radius of the planet, ![r=3.9\times 10^6\ m](https://tex.z-dn.net/?f=r%3D3.9%5Ctimes%2010%5E6%5C%20m)
Let a is the moon's radial acceleration. Mathematically, it is given by :
, R is the radius of orbit
Since, ![\omega=\dfrac{2\pi}{T}](https://tex.z-dn.net/?f=%5Comega%3D%5Cdfrac%7B2%5Cpi%7D%7BT%7D)
The radius of orbit is,
![R=r+h](https://tex.z-dn.net/?f=R%3Dr%2Bh)
![R=3.9\times 10^6\ m+235\times 10^6\ m=238900000\ m](https://tex.z-dn.net/?f=R%3D3.9%5Ctimes%2010%5E6%5C%20m%2B235%5Ctimes%2010%5E6%5C%20m%3D238900000%5C%20m)
So, ![a=\dfrac{4\pi^2 R}{T^2}](https://tex.z-dn.net/?f=a%3D%5Cdfrac%7B4%5Cpi%5E2%20R%7D%7BT%5E2%7D)
![a=\dfrac{4\pi^2 \times 238900000}{(2060\times 10^3)^2}](https://tex.z-dn.net/?f=a%3D%5Cdfrac%7B4%5Cpi%5E2%20%5Ctimes%20238900000%7D%7B%282060%5Ctimes%2010%5E3%29%5E2%7D)
![a=2.22\times 10^{-3}\ m/s^2](https://tex.z-dn.net/?f=a%3D2.22%5Ctimes%2010%5E%7B-3%7D%5C%20m%2Fs%5E2)
Hence, this is the required solution for the radial acceleration of the moon.