Bulk elemental planetary compositions (in wt%) of rocky planets formed in five of our planet formation simulations assuming a proto-planetary disk around Kepler-62 star (the lowest metallicity star in the sample) and the formation time of planetesimals of 0.2 Myr. Only the planets within 0.25 AU from the star are displayed as the variations between the more distant planets are insignificant. Size of bodies is not to scale. The Earth values taken from McDonough (2014) are shown for comparison (in the upper right corner).