Topic: Solar System evolution

Hal Levison explains how Jupiter’s Trojan asteroids could help distinguish competing accounts of Solar System evolution. The discussion compares scenarios in which giant planets formed near their present orbits with models involving substantial migration from a more compact configuration. It considers why the Lucy spacecraft’s observations can test these ideas and how discoveries of other planetary systems sharpen the questions.

When did the giant planets become dynamically unstable? This lecture compares evidence from lunar impact craters, binary objects in the Kuiper belt and dynamical models. It explains why these constraints matter for reconstructing Solar System evolution and why the timing remains an unresolved research question.