Given the variations in Ru isotopic compositions among early solar system materials, Ru isotopes show great promise for providing genetic fingerprints of diverse, late-stage accretionary additions to the Earth and Moon. This is possible because the Ru present in, for example, lunar impact melt rocks produced by basin-forming events, is primarily derived from the impactor. Ruthenium isotopes can be measured using either thermal ionization mass spectrometry or multiple-collector inductively coupled plasma mass spectrometry.