Science. 1972 Jan 28;175(4020):363-75. doi: 10.1126/science.175.4020.363.
Samples returned from the Apollo 15 site consist of mare basalts and breccias with a variety of premare igneous rocks. The mare basalts are from at least two different lava flows. The bulk chemical compositions and textures of these rocks confirm the previous conclusion that the lunar maria consist of a series of extrusive volcanic rocks that are rich in iron and poor in sodium. The breccias contain abundant clasts of anorthositic fragments along with clasts of basaltic rocks much richer in plagioclase than the mare basalts. These two rock types also occur as common components in soil samples from this site. The rocks and soils from both the front and mare region exhibit a variety of shock characteristics that can best be ascribed to ray material from the craters Aristillus or Autolycus.
从阿波罗15号着陆点带回的样本包括月海玄武岩、角砾岩以及各种月海前火成岩。月海玄武岩至少来自两种不同的熔岩流。这些岩石的整体化学成分和结构证实了之前的结论,即月球月海由一系列富含铁且贫钠的喷出火山岩组成。角砾岩含有大量斜长岩碎屑,以及比月海玄武岩富含更多斜长石的玄武岩碎屑。这两种岩石类型也是该着陆点土壤样本中的常见成分。来自正面和月海区域的岩石和土壤都呈现出各种冲击特征,这些特征最有可能归因于来自阿里斯提卢斯或奥托吕科斯撞击坑的射线物质。