Quoting Wikipedia:
The nebular hypothesis says that the Solar System formed from the gravitational collapse of a fragment of a giant molecular cloud.
The question is: how much of the current form of the Solar System is determined by the macroscopic state of the molecular cloud and its surroundings? Are the number of planets, their orbits, sizes and composition determined? if not - at what point in the evolution of the Solar System were these determined?
(I understand that the system is chaotic; but I'm interested only in macroscopic properties; surely something macroscopic is determined by the initial macroscopic state)
(by "Y is determined from X" I mean that Y is very likely to happen given X, even if the probability is not exactly 1.0)