Oxygen production from a lunar rock has been experimentally demonstrat
ed for the first time. A 10 g sample of high-Ti basalt 70035 was reduc
ed with hydrogen in seven experiments at temperatures of 900-1050-degr
ees-C and pressures of 14.7-150 psia. In all experiments, water evolut
ion began almost immediately and was essentially complete in tens of m
inutes. Oxygen yields ranged from 2.93 to 4.61% of the starting sample
weight, and showed weak dependence on temperature and pressure. Analy
sis of the solid samples demonstrated total reduction of Fe2+ in ilmen
ite and small degrees of reduction in olivine and pyroxene. TiO2 Was a
lso partially reduced to one or more suboxides. Data from these experi
ments provide a basis for predicting the yield of oxygen from lunar ba
salt as well as new constraints on natural reduction in the lunar rego
lith.