Williams, J.-P., Paige, D., Greenhagen, B. On the effect of magnetospheric shielding on the lunar hydrogen cycle. Solar wind implantation into lunar regolith: hydrogen retention in a surface with defects. Hydrogen implantation in silicates: the role of solar wind in SiOH bond formation on the surfaces of airless bodies in space. Large negative lunar surface potentials in sunlight and shadow. Biogenic oxygen from Earth transported to the Moon by a wind of magnetospheric ions. Remote detection of widespread indigenous water in lunar pyroclastic deposits. Earth wind as a possible exogenous source of lunar surface hydration. Temperature regime and water/hydroxyl behavior in the crater Boguslawsky on the Moon. Effects of darkening agents and low-albedo materials. Estimating the water content of hydrated minerals using reflectance spectroscopy. The global albedo of the Moon at 1064 nm from LOLA. Sources and physical processes responsible for OH/H 2O in the lunar soil as revealed by the Moon Mineralogy Mapper (M 3). 48th Annual Lunar and Planetary Science Conference, 1831 (2017). Lunar water spatial distribution and its temporal variations. Formation timescales of amorphous rims on lunar grains derived from ARTEMIS observations. Variability of hydration across the Southern Hemisphere of the Moon as observed by Deep Impact. Solar wind‐induced water cycle on the Moon. M., Aleksandrov, A., Hibbitts, K., Dyar, M. Solar wind implantation into the lunar regolith: Monte Carlo simulations of H retention in a surface with defects and the H 2 exosphere. Diurnally migrating lunar water: evidence from ultraviolet data. Water on the surface of the Moon as seen by the Moon Mineralogy Mapper: distribution, abundance, and origins. Time-of-day-dependent global distribution of lunar surficial water/hydroxyl. Hydrogen abundance estimation and distribution on (101955) Bennu. A new in situ quasi-continuous solar-wind source of molecular water on Mercury. Solar wind contributions to Earth’s oceans. Evidence of hydrated and/or hydroxylated minerals on the surface of asteroid 4 Vesta. Rotationally-resolved spectroscopy of Vesta I: 2–4 μm region. Detection of widespread hydrated materials on Vesta by the VIR imaging spectrometer on board the Dawn mission. Direct measurement of hydroxyl in the lunar regolith and the origin of lunar surface water. Atom probe tomography of space-weathered lunar ilmenite grain surfaces. Detection of adsorbed water and hydroxyl on the Moon. Character and spatial distribution of OH/H 2O on the surface of the Moon seen by M 3 on Chandrayaan-1. ![]() Temporal and spatial variability of lunar hydration as observed by the Deep Impact spacecraft. Surface water at lunar magnetic anomalies. The behavior of volatiles on the lunar surface. We suggest that although we have confirmed the importance of the solar wind as a major source of fast water production on the Moon, hitherto unobserved properties of the plasma sheet properties may also play an important role. We find that the water abundance at lunar mid-latitudes substantially increases in the dusk and dawn magnetosheath when the solar wind flux increases, yet remains nearly constant across the central magnetotail. Here we report abundance observations of lunar surficial water on the nearside at different stages during the Moon’s passage through Earth’s magnetotail. However, no correlated decrease in surficial water content has yet been seen on the lunar nearside. ![]() ![]() The lunar nearside spends ~27% of its daytime in Earth’s magnetotail where the solar wind flux is reduced by as much as ~99%. ![]() Solar wind implantation is thought to be one of the primary mechanisms in the formation of water (OH/H 2O) on the surface of the Moon and possibly on the surface of other airless bodies.
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