Correlation between the assumed original meteorite bulk chemical composition (Table 1) and the measured intensities of corresponding emission lines in spectra of ablated meteorites. Meteorite labels containing three letters from the meteorite’s name and classification are given for all meteorites except most ordinary chondrites. In all figures, the HED achondrites are plotted separately from the rest of the achondrites. In Fig. 3c, meteorite Ragland (LL chondrite) is outside the displayed limits with Cr I-7/Mg I-2 intensity ≈25.