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Connecting star and planet properties in a single model is notstraightforward. Stellar population synthesis models are key to explorecombined statistical constraints from stars and planets observations. TheBesan\c{c}on stellar population synthesis model (Robin et al. 2003, Lagarde etal. 2017) includes now the stellar evolutionary tracks computed with thestellar evolution code STAREVOL (Lagarde et al. 2012, Amard et al. 2016). Itprovides the global (M, R, Teff, etc) and chemical properties of stars for 54chemical species. It enables to study the different galactic populations of theMilky Way (the halo, the bulge, the thin and thick disc) and a specificobservational survey. Here, we couple the Besan\c{c}on model with a simplestoichiometric model (Santos et al. 2017) in order to determine the expectedcomposition of the planet building blocks (PBB). We investigate the trends andcorrelations of the expected chemical abundances of PBB in the differentstellar populations of the Milky Way (Cabral et al. 2018).

Chemical connections between low-mass stars and planets building blocks investigated by stellar population synthesis