ИСТИНА

It’s known that due to the lunar impact mascon basins have been dominated by an isosdetic processing of the mantle uploading and basalt filling at basin bottom, this evolution is directly connect with igneous activity. Identifying the mascon basins of various features will give more information to uncover the lunar dynamical evolution history. So, in result of Chang'e 3 mission we can investigate in situ such lunar features as structure of impact craters, near-surface magmatism, mechanisms and timing of deformation, cause(s) of crustal magnetization, estimation of upper-crustal density on intermediate zone between Sinus Iridum region and Mare Imbrium area.