
Wayne O. answered 08/31/20
Ph.D. Astrophysicist Who Loves Teaching
So, we have the period T = 68 years, the eccentricity e = 0.95, and want to find the semi-major axis, a.
One thing to note from Kepler's Third Law, is that the period depends only on the semi-major axis, so we don't need the eccentricity to answer this. The mathematical form of Kepler's Third Law is T2=a3. Considering we have the period, we just need to take the cube-root of both sides of the equation, giving T(2/3)=a. Remember this is the period in years and the semi-major axis in AU, so we can use our 68 years to get a semi-major axis of 16.66 AU or 17 AU if we round.