“…Precise information about the composition of Earth's core is critical for understanding planetary evolution (1-3) and discussing current important topics in geodynamic behavior, such as core-mantle boundary heat flow (3,4). However, samples from deep in the planetary interior are not available, so our knowledge is based on comparison of laboratory measurements (5)(6)(7)(8) with seismological observations (9), information from meteorite composition (3), and indications of Earth's core temperature (10)(11)(12). One of the most interesting results of such work has been the suggestion that Earth's core must contain light elements because the density of the core, as determined from seismological observations (9), is lower than the density of pure iron, its main constituent, as determined by laboratory measurements (5)(6)(7) and theoretical work (10,11).…”