Feldman WC, Barraclough BL, Maurice S, Elphic RC, Lawrence DJ, Thomsen DR, Binder AB
W. C. Feldman, B. L. Barraclough, R. C. Elphic, D. J. Lawrence, D. R. Thomsen, Los Alamos National Laboratory, MS D-466, Los Alamos NM 87545, USA. S. Maurice, Observatoire Midi-Pyrenees, 14 avenue Ed Belin, 31400 Toulouse, France. A. B. Binder, L.
Science. 1998 Sep 4;281(5382):1489-93. doi: 10.1126/science.281.5382.1489.
Global maps of thermal and fast neutron fluxes from the moon suggest three end-member compositional units. A high thermal and low fast neutron flux unit correlates with the lunar highlands and is consistent with feldspathic rocks. The South Pole-Aitken basin and a strip that surrounds the nearside maria have intermediate thermal and fast neutron flux levels, consistent with more mafic rocks. There appears to be a smooth transition between the most mafic and feldspathic compositions, which correspond to low and high surface altitudes, respectively. The maria show low thermal and high fast neutron fluxes, consistent with basaltic rocks.
来自月球的热中子通量和快中子通量全球地图显示出三个端元成分单元。高热中子通量和低快中子通量单元与月球高地相关,且与长石质岩石相符。南极-艾特肯盆地以及近月面月海周围的一条带状区域具有中等热中子通量和快中子通量水平,与更多的镁铁质岩石相符。在最镁铁质成分和长石质成分之间似乎存在平滑过渡,这两种成分分别对应低和高的地表海拔。月海显示出低热中子通量和高快中子通量,与玄武岩相符。