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Over the past two decades, the short-lived 182Hf–182W chronometer (T1/2 = 8.9 Myr) has been widely used for dating early Solar System processes, due to the unique geochemical properties of the system. Tungsten is a siderophile (iron-loving) element, and as such, it is largely (but not completely) extracted from the silicate mantles of planetary bodies during segregation of metallic cores. Hafnium, in contrast, is lithophile (silicate-loving) and is wholly retained in the silicate portion of planetary bodies. Therefore, determination of the abundance of the daughter nuclide, 182W, relative to other stable, non-radiogenic W isotopes (e.g., 184W) is of special interest for constraining the timing of planetary core formation.