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The preparation procedure of the solar system is not too well known, but the common idea is that stars and planets etc. around them form out of clouds of some material which is denser at some location than on average, and then gravity does its job. All this is of course well described by classical (even Newtonian) physics. A complete microscopic description is neither possible nor necessary.A. Neumaier said:This only covers states of microscopic systems in the lab.
Which preparatin nprocedure determines the quantum state of the solar system? How is the result of a measurement of some observables (say the mass of the Sun and the major planets) of this quantum state described from first principles (assuming Newonian gravity, which is fully adequate for this situation)?
The solar system is not coupled to an external measurement device as in the usual analysis of measurements.; the measurement is done from within. Without an explanation how this works, even ordinary quantum mechanics is an incompletely understood (and indeed incomplete) theory.
A simpler example is the coffee in the cup on my desk, which has been prepared by me just some minutes ago. It's pretty well described as a system of local thermal equilibrium slowly equilibrating further to finally reach the temperature of my office which is also pretty well described to be in local thermal equilibrium, providing a "heat bath" within which the coffee sits and exchanges energy and water molecules, i.e., it cries to be described as a grand canonical ensemble close the thermal equilibrium and thus with classical physics like (viscous) hydro dynamics with heat conduction etc.
So preparation procedures need not be very "artificial" as, e.g., at a collider like the LHC, where proton bunches are accelerated and kept at high precision at a certain energy to get something accurately prepared to make experiments, where the much more microscopic detail is resolved. Already substituting the protons by Pb nuclei and performing heavy-ion collisions changes this completely, and again there's no better chance to understand what's going on than to use (semi-)classical methods like kinetic theory, relativistic viscous hydro, Langevin processes, etc. to describe the system. Even in p Pb and pp collisions one observes quite some "collectivity", at least in "high-multiplicity events".
It's a gift and a curse of nature at once that macroscopic, or even "mesoscopic" systems of some 1000 of particles, tend to behave according to classical or semi-classical models. It's a gift, because we have the chance to understand more by describing these system approximately with simpler models but also a curse, because we cannot so easily observe the (maybe) interesting quantum phenomena we are after.