Seems much simpler to assume the moon formed in the same manner as most of the rest of the solar system. It coalesced out of the primordial accretion disc.- Chronos
No doubt that holds true for some of the moons. The problem in the case of Earth’s moon is pointed out by the article I referenced: “The Apollo missions proved that Earth and the Moon are closely related… the Moon has a low content of volatile elements, suggesting its birth involved high temperatures… While the Moon’s chemistry most closely resembles Earth’s mantle, the mantle is a
secondary feature of our planet’s evolution. It emerged when Earth, soon after formation, differentiated into mantle and core. How could any kind of moon, born as an independent body, have a composition matching the mantle.?”
Does the model in the magazine suggest that it just remained as debris, fell back to earth, condensed as part of the moon and/or flew off into space? Or did it condense as a single mass again?- check
As best I can explain the sequence in the article, it looks like about a third of the body that struck Earth just kind of slides on past, warping out of shape as it goes. It stretches into a tendril with an arcuate shape. Other bits and pieces continue being vomited out of the gouge in Earth for a while. In frame 6 it looks like a pretty fair chunk of stuff lands back on Earth, but the long tendril continues to revolve around Earth, eventually smoothing out into more of a disk shape. The simulation doesn’t proceed far enough to show the disk coagulating into the Moon proper.
We could simulate, in reverse, the exact path and the stellar bodies around it.- lightbeing
Years ago I remember reading a brief item about someone putting a bunch of digital processors together in a way so as to make a special-purpose device to do one thing: calculate the positions of planetary bodies in the solar system, forward or backward in time. The device was called a “digital orrery.” Whether it handled Earth’s moon as well, or just the planets, I don’t quite remember. At any rate, what you are talking about could surely be done, but the results would get less trustworthy the farther back in time you look with the calculations. For instance, what if we only know the mass of the (modern) moon to 1 part in 10,000? I imagine that kind of uncertainty causes all sorts of havoc in the calculations by the time you get back millions of years in the past, let alone billions. And of course we don’t know the history of long-term comets that pass through the solar system and ever-so-slightly perturb the planets, since we only know of ones that have passed by in historic times, and that would be a tiny fraction of the overall number of those critters.