RESUMEN
Updated dataset based on the laser scanning of three specimens of lunar soil simulants representing highland regions (LHS-1, AGK-2010, CHENOBI) and three specimens of lunar soil simulants representing mare regions (LMS-1, JSC-1A, OPRL2N). In previous studies, only a specimen of ilmenite was used as a lunar soil simulants. Measurements were executed using phase-shift and time-of-fly terrestrial laser scanners (Z + F IMAGER 5016, FARO Focus3D, and Leica ScanStation C10). The stored data contain radiometric information of point clouds from the measurement of lunar soil simulants. The data provide information on the effect of different types of simulants (mare and highland) on the absorption and dispersion of the laser beam. In overall, the dataset presented in this work can be used in investigation of the application of the laser technology in the measurement of lunar structures made of mare and highlands lunar regolith. Lunar highlands and mare regions are characterized by different physicochemical parameters. Therefore, both types of soil scatter the laser beam differently, what affects the range and accuracy of the laser measurements.
RESUMEN
In the near future, permanent human settlements on the Moon will become increasingly realistic. It is very likely that the Moon will serve as a transit point for deep space exploration (e.g., to Mars). The key to human presence on the Moon is the ability to erect the necessary structures and habitats using locally available materials, such as lunar soil. This study explores the feasibility of using terrestrial laser scanning technology as a measurement method for civil engineering applications on the Moon. Three lunar soil simulants representing highland regions (LHS-1, AGK-2010, CHENOBI) and three lunar soil simulants representing mare regions (LMS-1, JSC-1A, OPRL2N) were used in this study. Measurements were performed using three terrestrial laser scanners (Z+F IMAGER 5016, FARO Focus3D, and Leica ScanStation C10). The research programme focused on the radiometric analysis of datasets from the measurement of lunar soil simulants. The advantages and limitations of terrestrial laser scanning technology for possible lunar applications are discussed. Modifications of terrestrial laser scanners that are necessary to enable their use on the Moon are suggested.
RESUMEN
The future construction effort on the Moon and Mars is increasingly discussed by the scientific community. In authors' opinion quick, precise and remote measuring technique will be essential for successful development of lunar and Martian construction projects. One of such techniques is terrestrial laser scanning (TLS). The dataset consists of results obtained using two different, commercially available, laser scanners. The measurements were conducted on Earth using lunar and Martian soil simulants. As a reference (Earth soil simulant) a standardized sand used for cement tests was utilized. Scans were performed from different distances. The acquired point clouds can be used for thorough analysis of a laser beam dispersion and absorption. The comparison with other results is enabled. One should also keep in mind that some of the characteristics of Earth, the Moon and Mars which will influence TLS technique and measurements (e.g. local atmosphere or lack of it, temperatures, radiation, light, distances and colours).
