This is not an easy question. Yes, you can calculate the forces of the Sun, the planets, and the Moon on each other at some point in time using Newton's law -- if you know where everything is. Now, what does that tell you? The answer: Not a whole lot.
To see the effect of these forces are one needs to integrate these forces over time. This cannot be done analytically. This is a many body problem. Numerical integration techniques are needed. For high accuracy, some aspects of general relativity must be incorporated into the model, and the model needs to encompass small bodies as well as large. What will this tell you? You will get the positions of the solar system bodies as a function of time over the period during which you performed the integration. This is the approach taken by JPL and the Russian space agency in formulating their planetary ephemerides model.
This approach doesn't say much about orbits (orbital elements). If you want to know about orbits you will need to take a different approach. That approach is what people used before computers. The approach taken by Lagrange, Dalaunay, Hill, Newcomb, and Brown (these were the key developers) was to describe the behavior of the Moon in the form of Hamiltonian written in terms of the orbital elements. Lagrange started this by developing Lagrange's planetary equations. Dalaunay's planetary equations refined Lagrange's approach. Hill wrote his own planetary equations because Lagrange's and Dalauney's approaches converged very slowly. Newcomb added some refinements to Hill's work. Brown put the capstone on the whole thing.
Some of the seminal papers:
Brown, E.W., "On the theoretical values of the secular accelerations in the lunar theory," Monthly Notices of the Royal Astronomical Society 57:5 342-349 (1897)
http://articles.adsabs.harvard.edu//full/1897MNRAS..57..342B/0000342.000.html
Hill, G.W., "On the application of Delaunay transformations to the elaboration of the secular perturbations of the solar system," Astronomical Journal, 22:527 183-189 (1902).
http://adsabs.harvard.edu/full/1902AJ...22..183H
Newcomb, S., "On the action of the planets on the moon," Astronomical Journal 25:592 129-132 (1907).
http://adsabs.harvard.edu/full/1907AJ...25..129N
A couple more recent papers that use a planetary equations formulation:
Standaert, D., "Direct perturbations of the planets on the moon's motion," Celestial Mechanics, vol. 22:40 357-369 (1980)
http://articles.adsabs.harvard.edu//full/1980CeMec..22..357S/0000357.000.html
Chapront, J. & Chapront-Touze, M., "Planetary Perturbations of the Moon in ELP 2000," Celestial Mechanics, 26:1, 83-94 (1982)
http://articles.adsabs.harvard.edu//full/1982CeMec..26...83C/0000083.000.html