Science. 1970 Jan 30;167(3918):507-9. doi: 10.1126/science.167.3918.507.
A neuttron activation scheme for determining 25 elements in lunar samples weighing 20 milligrams is described and applied to a suite of Apollo 11 lunar materials. Concentrations of titanium, chromium, scandium, tantalum, hafnium, and rare earths are higher than in avercage basalt, whereas cobalt, nickel, and copper are lower. Chemical variations show groupings of elements possibly associated with the major phases, pyroxene, plagioclase, and ilmenite. The high concentration of "refractory oxides" and low volatile content implies that the raw material for the Apollo 11 samples was condensed from the primitive solar nebula at high temperatures.
描述了一种用于确定 20 毫克月球样本中 25 种元素的中子激活方案,并将其应用于阿波罗 11 号月球样本。钛、铬、钪、钽、铪和稀土元素的浓度高于平均玄武岩,而钴、镍和铜的浓度较低。化学变化显示出与主要相(辉石、斜长石和钛铁矿)可能相关的元素组合。“难熔氧化物”的高浓度和低挥发性含量表明,阿波罗 11 号样本的原始材料是在高温下从原始太阳星云中凝聚而成的。