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Analysis of data of “Clementine” and “KAGUYA” missions and “ULCN” and “KSC-1162” catalogues
Authors:Y.A. Nefedyev  S.G. Valeev  R.R. Mikeev  A.O. Andreev  N.Y. Varaksina
Affiliation:1. Engelhardt Astronomical Observatory, Kazan Federal University, Tatarstan, Zelenodolsk 422526, St. Observatory, EAO, Russia;2. Ulyanovsk Technological State University, Ulyanovsk 432027, St. Severny Venec, 32, Russia
Abstract:In this paper an analysis of data coordinate systems from selenographic catalogues and space missions was carried out. The lunar macrorelief models were made on basis of the software package ASNI USTU using method of the spherical harmonic expansion. These models accurately describe the global features of the lunar figure. To construct these models the following sources of topographic information were used: “Clementine” and “KАGUYА” (Selena, Japan mission) missions, “KSC-1162” (Kazan selenocentric catalogue), “Kiev” (selenodesic catalogue), “SAI” (Chuikova (1975)), “Bills, Ferrari”, “ULCN” (The Unified Lunar Control Network 2005). Direct comparison hypsometric information “KSС-1162” catalogue data with “Clementine” mission was carried out. These researches confirmed a good agreement of the hypsometric information of compared systems. The normalized coefficients were obtained on basis of the hypsometric information expansion for eight sources. The displacement of the lunar center of mass (LCM) relatively to the lunar center of figure (LCF) was obtained by using topographic data selenodetical catalogues and space missions.
Keywords:Selenodesy   Center masses   Center figure   Robust methods   Cosmic missions   Selenocentric catalogues
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