Question
Question: The gravitational field due to a mass distribution is \(E = \dfrac{K}{{{x^3}}}\) in the x-direction....
The gravitational field due to a mass distribution is E=x3K in the x-direction. (K is a constant). Taking the gravitational potential to be zero at infinity, its value at a distance x is:
A. xk
B. 2xk
C. x2k
D. 2x2k
Solution
Hint Use the definition of gravitational field as, the Force Exerted by a mass distribution on a unit mass, given by E=x3K
We will start with a test mass mexperiencing the given field at dx distance and integrate it from infinity to x to compute Gravitational Potential.
Complete step by step answer
Given a test mass m on the x-axis, the work done W to move it a distance dx in the given gravitational field will be:
⇒ W=x3mK.dx [Since, W=F.S, where F is the force and S is the displacement]
Hence, the work done in bringing the test mass from infinity to x will be
⇒W=∞∫xx3mKdx
Since gravitational potential is required work done to bring a unit mass from infinity to x,
⇒P=mW
Hence, for our case, gravitational potential P will be,
⇒P=m1∞∫xx3mKdx
Since, test mass m and constant K are independent of the variable x, we can bring it outside the integral,
⇒P=m1mK∞∫xx31dx
Cancelling m from the numerator and denominator and solving the integral using∫x−3dx=−3+1x−3+1 , we get
⇒P=K[−2x−2]∞x
Hence we get the gravitational potential as:
⇒P=−K[2x21]∞x
Putting the limits in the differential and using gravitational potential at ∞ = 0, we get
⇒P=−K[2x21−0]
This gives us the final value for potential at x, for the given electrical field as,
⇒P=−2x2K
This is of the form,
⇒P=2x2k
Note Alternative method – Use the formula for the Gravitational Potential as the Gravitational field from infinity to x as P=∞∫xx3Kdx. This method does not include the term for test mass m but is less intuitive.