\(-\frac{20 Gm}{R}\)
\(-\frac{8Gm}{R}\)
\(-\frac{12Gm}{R}\)
\(-\frac{16Gm}{R}\)
To find the gravitational potential on the line joining two masses where the gravitational field equals zero, we need to first determine the point where the gravitational field due to both masses is equal and opposite, thus cancelling each other out.
Let's assume the two masses, \( m \) placed at \( A \) and \( 9m \) at \( B \), are separated by a distance \( R \). Let the point where the gravitational field equals zero be at a distance \( x \) from mass \( m \). Thus, it is \( (R - x) \) from mass \( 9m \).
The gravitational field due to a mass \( M \) at a distance \( r \) is given by:
\(E = \frac{GM}{r^2}\)
For the net gravitational field to be zero at point \( P \), the magnitudes should be equal:
\(\frac{Gm}{x^2} = \frac{G \times 9m}{(R-x)^2}\)
By simplifying:
\(\frac{1}{x^2} = \frac{9}{(R-x)^2}\)
Taking the square root of both sides, we get:
\(\frac{1}{x} = \frac{3}{R-x}\)
Rearranging gives:
\(R-x = 3x\)
Solve for \( x \):
\(R = 4x \Rightarrow x = \frac{R}{4}\)
Now, calculate the gravitational potential at this point. The potential \( V \) due to a mass \( M \) at a distance \( r \) is:
\(V = -\frac{GM}{r}\)
The total potential \( V \) at point \( P \) is the sum of the potentials due to both masses:
Total potential at point \( P \):
\(V = V_1 + V_2 = -\frac{4Gm}{R} - \frac{12Gm}{R} = -\frac{16Gm}{R}\)
Therefore, the correct answer is:
\(-\frac{16Gm}{R}\)
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)