To solve this problem, we need to calculate the gravitational potential at the origin due to an infinite number of bodies placed along the x-axis at specific intervals.
The gravitational potential \(V\) at a point due to a mass \(m\) located at a distance \(r\) is given by the formula:
\(V = -\frac{Gm}{r}\)
Where:
Let's calculate the contribution of gravitational potential from each mass and then sum it to find the total potential at the origin.
For the first mass at 1m:
\(V_1 = -\frac{G \times 2}{1} = -2G\)
For the second mass at 2m:
\(V_2 = -\frac{G \times 2}{2} = -G\)
For the third mass at 4m:
\(V_3 = -\frac{G \times 2}{4} = -\frac{G}{2}\)
For the fourth mass at 8m:
\(V_4 = -\frac{G \times 2}{8} = -\frac{G}{4}\)
Observing the pattern, the contribution from the nth mass at \((2^{(n-1)})\) m will be:
\(V_n = -\frac{G \times 2}{2^{(n-1)}} = -\frac{2G}{2^{(n-1)}}\)
The total potential \(V_{total}\) at the origin due to all masses is the sum of all individual potentials:
\(V_{total} = V_1 + V_2 + V_3 + V_4 + ...\)
\(V_{total} = -2G - G - \frac{G}{2} - \frac{G}{4} - ...\)
Recognizing this as an infinite geometric series, we find the sum using the formula for the sum of an infinite geometric series:
\(S = a/(1 - r)\) where \(a\) is the first term and \(r\) is the common ratio.
In our series, \(a = -2G\) and the common ratio \(r = \frac{1}{2}\). Hence,
\(V_{total} = \frac{-2G}{1 - \frac{1}{2}}\)
\(V_{total} = \frac{-2G}{\frac{1}{2}} = -4G\)
Thus, the resulting gravitational potential due to this system at the origin is \(-4G\).
The correct answer is:
-4G