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Andrea Miglio (University of Birmingham)
In the last few years asteroseismology has proven to be a main asset to the study of the structure and evolution of the Milky Way. In this talk I will summarise the recent progresses in this fast growing field, focussing primarily on the reliability of the asteroseismic age scale. I will then discuss future prospects and synergies with Gaia, and whether with K2, TESS, and PLATO we should expect incremental changes or breakthroughs in Galactic asteroseismology.