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Question: Two bodies of masses m and 4 m are placed at a distance r. The gravitational potential at a point on...

Two bodies of masses m and 4 m are placed at a distance r. The gravitational potential at a point on the line joining them where the gravitational field is zero.

A

6Gmr\frac{6Gm}{r}

B

9Gmr\frac{-9Gm}{r}

C

Zero

D

4Gmr\frac{-4Gm}{r}

Answer

9Gmr\frac{-9Gm}{r}

Explanation

Solution

Let the two masses be mm and 4m4m placed at a distance rr. Let the point where the gravitational field is zero be at a distance xx from mass mm. Then its distance from mass 4m4m is (rx)(r-x). For the gravitational field to be zero, the point must lie between the two masses.

The gravitational field due to mass mm at this point is E1=Gmx2E_1 = \frac{Gm}{x^2}. The gravitational field due to mass 4m4m at this point is E2=G(4m)(rx)2E_2 = \frac{G(4m)}{(r-x)^2}.

For the net gravitational field to be zero, their magnitudes must be equal: Gmx2=G(4m)(rx)2\frac{Gm}{x^2} = \frac{G(4m)}{(r-x)^2} 1x2=4(rx)2\frac{1}{x^2} = \frac{4}{(r-x)^2} Taking the square root of both sides: 1x=2rx(since x and rx are positive)\frac{1}{x} = \frac{2}{r-x} \quad \text{(since } x \text{ and } r-x \text{ are positive)} rx=2xr-x = 2x r=3xr = 3x x=r3x = \frac{r}{3} The distance of the point from mass 4m4m is rx=rr3=2r3r-x = r - \frac{r}{3} = \frac{2r}{3}.

The gravitational potential at this point is the sum of the potentials due to each mass: V=Vm+V4mV = V_m + V_{4m} V=GmxG(4m)rxV = -\frac{Gm}{x} - \frac{G(4m)}{r-x} Substitute the values of xx and rxr-x: V=Gmr/3G(4m)2r/3V = -\frac{Gm}{r/3} - \frac{G(4m)}{2r/3} V=3Gmr4Gm×32rV = -\frac{3Gm}{r} - \frac{4Gm \times 3}{2r} V=3Gmr12Gm2rV = -\frac{3Gm}{r} - \frac{12Gm}{2r} V=3Gmr6GmrV = -\frac{3Gm}{r} - \frac{6Gm}{r} V=9GmrV = -\frac{9Gm}{r}