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Analysis of Lunar Terrain Altitudes and Correlation Links between the Terrain and Gravitational Field; Preliminary Conclusions on the Global Density Inhomogeneities of the Lunar Crust


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Abstract

The harmonic and statistical analysis of lunar terrain altitudes has been performed based on the procedure developed by the authors. The explanations for the displacements of the Moon's figure relative to the center of mass and for the shift of the major equatorial axis relative to the earthward direction have been given. The maps have been plotted for the density anomalies in the near-surface layers of the Moon that correspond to mascons (with negative correlation between the field and terrain mainly for N= 10, 11) and other variants of links between the gravitational field and terrain (with positive correlation between the field and terrain). It has been shown that the harmonics of the degree N= 5–9 mainly correspond to the isostatic compensation of the terrain in the near-surface layers of the crust; the low harmonics (N< 5) correspond to the isostatic compensation of the terrain in the deeper layers, while the harmonics of the degrees N > 11 may indicate the presence of tension in the crust generated by small structures of the terrain. Based on the maps, possible locations of deposits of volatile elements (mainly on the far side of the Moon and in the northern cir-cumpolar region) and other natural resources have been determined.

About the authors

N. A. Chuikova

Sternberg Astronomical Institute

Author for correspondence.
Email: jeanna@sai.msu.ru
Russian Federation, Moscow, 119234

Zh. F. Rodionova

Sternberg Astronomical Institute

Email: jeanna@sai.msu.ru
Russian Federation, Moscow, 119234

T. G. Maksimova

Sternberg Astronomical Institute

Email: jeanna@sai.msu.ru
Russian Federation, Moscow, 119234

E. A. Grishakina

Vernadsky Institute of Geochemistry and Analytical Chemistry

Email: jeanna@sai.msu.ru
Russian Federation, Moscow, 119991

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