Science. 1975 Jun 27;188(4195):1297-300. doi: 10.1126/science.188.4195.1297.
A global lunar gravity field has been determined from data on the long-term motion of the Apollo 15 and Apollo 16 subsatellites and Lunar Orbiter 5. The nearside gravity map resolves major mascon basins and, in general, is in excellent agreemnent with the results of Muller and Sjogren. The farside gravity map is characterized by broad positive gravity in the highland regions with interspersed, localized, negative anomalies corresponding to major ringed basins. A comparison between global gravity and topography indicates that a thicker farside crust could be responsible for these gravitational differences between the two lunar hemispheres.
从阿波罗 15 号和阿波罗 16 号子卫星以及月球轨道器 5 号的长期运动数据中确定了一个全球月球重力场。近地侧重力图解析了主要的质量瘤盆地,并且总体上与 Muller 和 Sjogren 的结果非常吻合。远地侧重力图的特点是高地地区存在广泛的正重力,其中穿插着与主要环形盆地相对应的局部负异常。全球重力与地形的比较表明,较厚的远地侧地壳可能是造成这两个月球半球之间这些重力差异的原因。