Abstract

Lunar gravity field is important information to reveal lunar internal structure and element composition, as well as one of the key scientific objects of lunar exploration mission. Using Chang'E-1 orbital tracking data, and in combination with orbital tracking data of SELENE, Lunar Prospector (LP) and historical spacecraft, a high accuracy lunar gravity field model CEGM02 is developed, improvements are shown compared to CEGM01 and other historical models. Analyses show that Chang'E-1 orbital tracking data contribute to long wavelength of lunar gravity field because of its higher orbit altitude than SELENE main orbiter. When compared CEGM02 with SGM100h, there are improvements by a factor of about 2 below degree 5, significant improvements up to degree 10, and contribution to all coefficients until degree 30. Lunar mean moment of inertia 0.393446 (±0.000006) is presented by combining degree 2 coefficients of CEGM02 with lunar laser range results, which can be served as a rather strong constraint in lunar internal structure research.

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