The gravitational field due to a mass distribution is $E=K / x^{3}$ 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) $K / x$
(b) $K / 2 x$
(c) $K / x^{2}$
(d) $K / 2 x^{2}$