One thing that comes out of the scattering theory is the scattering (in the rest frame of the moon) makes two asymptotes, (incoming and outgoing), where the total scattering angle is ## 2 \arctan(GM/(v_o^2 b )) ## where ## v_o ## is the asymptotic speed and ## b ## is the impact parameter which comes about with the conservation of angular momentum. I had no luck in showing though why this scattering angle is such a simple expression, but I was able to show that the scattering angle would simply depend upon some form of ## GM/(v_o^2 b ) ##, from the differential expression involving the energy and angular momentum.
Note: M=mass of moon.
and to expound upon this, the complete scattering angle comes out of the solution in polar coordinates ## r=r_o/(1+\epsilon \sin{\theta}) ## of the differential equation, where the asymptotes are easily determined. I thought there should be a good reason for this that might show up in x-y coordinates, but so far it has eluded me. Note: ## \epsilon=\sqrt{1+(v_o^2 b/GM)^2} ##.