Compositional variation in the Hadley Apennine region
Compositional variation in the Hadley Apennine region
复制标题
哈德利亚平宁地区的成分变化
DOI：
--
复制
发表时间：
1982
期刊：
影响因子：
--
通讯作者：
B. Hawke
中科院分区：
文献类型：
--
作者：
P. Clark;B. Hawke
哈德利亚平宁地区的轨道地球化学数据与典型的岩石成分有关，并用于确定该地区发现的岩石类型所产生的土壤分布。轨道XRF Mg/Si和Al/Si强度是主要使用的轨道数据。这些数据是使用以前开发的方法的修改，假的轨道间的变化进行校正。从理论上考虑，校正值分别转换为% MgO和% Al 2 O3，并与阿波罗15号着陆点典型月球岩石和土壤的类似浓度进行比较。的XRF值的Fe，Ti和Th浓度，来自γ射线观测的关系，也被认为是。它是建立在该地区的轨道地球化学数据是一致的ANT套件和弗拉毛罗玄武岩成分的混合物的存在下，经常占主导地位的KREEP玄武岩成分向西和镁铁质火山碎屑成分向东。
Orbital geochemical data in the Hadley Apennine region are related to typical rock compositions and used in determining the distribution of soils derived from the rock types found in this region. Orbital XRF Mg/Si and Al/Si intensities are the orbital data that are used primarily. These data are corrected for spurious interorbit variation using a modification of a previously developed method. The corrected values are than converted to % MgO and % Al2O3, respectively, from theoretical considerations, and as such are compared with similar concentrations for typical lunar rocks and soils of the Apollo 15 landing site. The relationship of the XRF values to Fe, Ti, and Th concentrations, derived from gamma-ray observations, is also considered. It is established that the orbital geochemistry data for this region are consistent with the presence of a mixture of ANT suite and Fra Mauro basalt components frequently dominated by a KREEP basalt component toward the west and by a mafic pyroclastic component toward the east.