The Gaia spacecraft has brought our Milky Way into focus in an unprecedented way. The synergy with ground-based spectroscopic surveys has provided us with photometry, 6-D phase-space coordinates, and spectra for millions of stars. I will firstly discuss the constraints the inferred dynamical, chemical, and age properties of stars have placed on a major accretion event nine Gyrs ago that may have thickened the pre-existing disc and birthed a new thin disc. I will then discuss how interactions between the Miky Way and its satellite system continue to shape the discs until the present day. To finish, I will say some words about what our new perspective on the formation of the Milky Way can reveal about the evolution of disk galaxies throughout the Universe.
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