Rainfall scavenges meteoric cosmogenic 10 Be from the atmosphere.
10Be falls to the Earth surface, where it binds tightly to sediment particles in non-acidic soils over the life-span of those soils. As such, meteoric 10 Be has the potential to be an excellent geochemical tracer of erosion and stability of surfaces in a diverse range of natural settings. Meteoric 10 Be has great potential as a recorder of first-order erosion rates and soil residence times. Even though this tracer was first developed in the late 1980s and showed great promise as a geomorphic tool, it was sidelined in the past two decades with the rise of the "sister nuclide", in situ 10 Be, which is produced at a known rate inside quartz minerals. Since these early days, substantial progress has been made in several areas that now shed new light on the applicability of the meteoric variety of this cosmogenic nuclide. Here, we revisit the potential of this tracer and we summarize the progress: (1) the atmospheric production and fallout is now described by numeric models, and agrees with present-day measurements and paleo-archives such as from rain and ice cores; (2) short-term fluctuations in solar modulation of cosmic rays or in the delivery of 10 Be are averaged-out over the time scale soils accumulate; (3) in many cases, the delivery of 10 Be is not dependent on the amount of precipitation; (4) we explore where 10 Be is retained in soils and sediment; (5) we suggest a law to account for the strong grain size dependence that controls adsorption and the measured nuclide concentrations; and (6) we present a set of algebraic expressions that allows calculation of both soil or sediment ages and erosion rates from the inventory of meteoric 10