Abstract
By landing unmanned or manned research stations on the surface of planets, moons, comets and asteroids in-situ characterization of these bodies becomes possible. Typically the scientific objective of lander missions includes measurements selected from the following list:
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• generation of images for studying morphological properties of the site and for obtaining mineralogical information (multispectral imaging)
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• chemical analysis of surface matter: bulk elemental abundance, isotopes, minerals, ices, carbonaceous compounds, organic, volatiles
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• determination of structure and physical properties of the surface: topography, texture, roughness, regolith scales, mechanical, electrical, optical, and thermal properties, temperatures.
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• measurements characterizing local depth structure (stratigraphy), and global internal structure.
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Wittmann, K., Ulamec, S., Richter, L. (1999). Lander Systems for Planetary Missions. In: Ehrenfreund, P., Krafft, C., Kochan, H., Pirronello, V. (eds) Laboratory Astrophysics and Space Research. Astrophysics and Space Science Library, vol 236. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4728-6_24
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DOI: https://doi.org/10.1007/978-94-011-4728-6_24
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