Science. 1967 Oct 13;158(3798):259-61. doi: 10.1126/science.158.3798.259.
Indium concentrations have been determined by neutron activation in four members of each of the L3, L4, L5, and L6 chondritic meteorite classes. The range of concentrations is found to be from 0.14 to 22 parts per billion, with the highest values in L3 chondrites and the lowest values in the L5 and L6 classes. Plots of indium concentration versus relative mean deviation of pyroxene iron content, total carbon concentration, and primordial argon-36 concentration show positive correlations to varying degrees. Indium concentration appears to be a valuable parameter relating to variable formation conditions of the chondritic meteorites during the early history of the solar system.
铟浓度已通过中子活化法在 L3、L4、L5 和 L6 球粒陨石类的每个成员中确定。发现浓度范围从 0.14 到 22 十亿分之一,在 L3 球粒陨石中最高,在 L5 和 L6 类中最低。铟浓度与辉石铁含量、总碳浓度和原始氩-36 浓度的相对平均偏差的关系图显示出不同程度的正相关。铟浓度似乎是一个有价值的参数,与太阳系早期球粒陨石形成条件的变化有关。