The process to determine the composition of meteoritic fragments is not in doubt. The real question is identifying which fragments originated from Earth, and distinguishing them from other impact fragments of similar composition. At present we do not know the precise composition of the Chicxulub impactor, our second most-recent such body, and finding fragments of it on Mars or elsewhere will require considerable refinement of our understanding of multiple planetary morphologies to sort out Earth impactor fragments from others, including Martian ones. We need a larger body of knowledge of the composition of near-solar planets to accomplish this. But doing so will provide us the basis for an even more difficult identification task -- that of determining whether any fragments on Mars or Earth came in fact from impacts with Venus. That's going to be a search that must rely on much greater information on planetary composition than we possess at present.