Geologic characteristics of the Luna 17/Lunokhod 1 and Chang'E-3/Yutu landing sites, Northwest Mare Imbrium of the Moon. (November 2015)

• Record Type: Journal Article
• Authors: Basilevsky, A.T.; Abdrakhimov, A.M.; Head, J.W.; Pieters, C.M.; Wu, Yunzhao; Xiao, Long
• Is Part Of: Planetary and space science. Volume 117(2015)
• Page Start: 385
• Page End: 400
• Publication Date: 2015-11
• Subjects: Rover -- mare -- highland -- regolith -- crater -- ejecta; Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2015.08.006
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: We compared and assessed the results of measurements and observations by the Lunokhod 1 and Yutu rovers, both of which explored the northwestern part of Mare Imbrium. Both sites are within the distinctive Eratosthenian-aged lava flow geologic unit and our comparisons showed that the geologies of these exploration sites are very similar. As in the majority of other areas of the Moon, the dominant landforms in these sites are small impact craters, having various degrees of morphologic prominence and states of preservation, and rock fragments, mostly associated with the rims and interiors of fresh craters. The shape and the degree of preservation of the observed rock fragments in these two sites are similar. In both sites sporadic rock fragments were observed whose morphologies suggest that their source rocks had columnar jointing. Localization of these specific rocks on the rims of 450–470 m in diameter craters implies that the source rocks are at depths of 40–50 m. Regolith in the study areas is typically a few meters thick, but locally can be much thicker. The ground penetrating radar of the Yutu rover revealed the multilayer regolith structure, which is determined by superposition of crater ejecta; with some local variations, this type of the regolith stratigraphy should be typical of the majority of lunar mare sites. The physico-mechanical properties of the regolith in these two sites appear to be rather similar: the bearing capacity ranges from 0.04 to 1.44 kg/cm 2, with a modal value ∼0.45 kg/cm 2, and the shear strength ranges from 0.02 to 0.1 kg/cm 2, with a modal value ∼0.05 kg/cm 2 . Both these factors decrease by a factor of 3–4 with an increase of surface slope from ∼2 to 12°. The chemical composition of surface materials determined by the rover instruments at these two sites differ from those derived from the remote sensing data for the Eratosthenian-aged basalts on which the two sites are located. This could be partly due to low measurement accuracies, especially in the case of Lunokhod 1, but may also represent real variations in the composition of the surface materials compared to returned lunar samples. Difference in the spatial resolution of the in-situ and remote-sensing analyses should also be taken into account. Recommendations for future lunar rover missions are as follows: (1) to use ground penetrating radar and a robotic arm, and (2) to employ radial study tactics for impact crater documentation and analysis. Highlights: Results of observations of Lunokhod 1 and Yutu rovers in Mare Imbrium are described. Dominant landforms in both study areas are small impact craters and rock fragments. Morphologies of some rock fragments suggest that source rocks had columnar jointing. Ground penetrating radar and robotic arm are recommended for future rover missions. Radial study tactics for crater documentation and analysis is also recommended.