Remote sensing data from lunar orbiters have revealed spectral features consistent with the presence of OH or HO on the lunar surface. Analyses of data from the Moon Mineralogy Mapper spectrometer onboard the Chandryaan-1 spacecraft have suggested that OH/HO is recycled on diurnal timescales and persists only at high latitudes. However, the spatial distribution and temporal variability of the OH/HO, as well as its source, remain uncertain.
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