ABSTRACT
Early results showed that the Moon has practically no atmosphere and that it lost its thermal energy in the initial stages of formation. As a result, it has undergone minimal changes from its earlier formation unlike Earth, which has undergone drastic changes. In addition, the Moon is more heterogeneous and underwent prolonged igneous activity spanning hundreds of millions of years. This process led to varied and large-scale differentiation and fractionation during its early history. Therefore, long-standing questions such as lunar environments, origin, formation and evolution, magnetization of crustal rocks, internal structure, and possible life are of interest to the researcher.
