Interior compositions (in wt%) of the simulated planets in eight different systems around Kepler-62 (the lowest metallicity star) and Kepler-94 (the highest metallicity star) assuming the planetesimal formation times of 0.2 Myr (the earliest formation time) and 0.8 Myr (the latest formation time). The systems are grouped in pairs and selected to showcase all possible categories of planets that emerged from our simulations. Only planets with semimajor axes within 0.4 AU are displayed. The Earth values taken from McDonough (2014) are shown for comparison (lower right corner).