11.8.
We know that Kepler's third law states that
T2 = k a2/3
where T is the period and a is the semi-major axis length. In
astronaumical units, that is, when the period is given in years and
the distance a is given in A.U., then the value for k is
k = 1
So, plugging in the numbers,
where we have used the geometry of the problem to get the distance
a in terms of the distance x.
solving for x, we find
x = 2(75.6)2/3 - 0.57 = 35.2 A.U.
which is near the orbit of Pluto.