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Highlights of the meeting include new insights into r and s-processes and an explosion of interesting abundance data on stars in the Galactic halo and in dwarf spheroidal galaxies. I include in this summary a few suggestions on the chemical evolution of the Thick and Thin disks, and on the present and past distribution of baryons and metals in the universe.
13 pages LaTeX, one figure, slightly revised after comments. To appear in Carnegie Observatories Astrophysics Series, Vol. 4: Origin and Evolution of the Elements, ed. A. McWilliam and M. Rauch (Cambridge University Press)

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