Abstract
The selection of a landing site on a planetary body is a multistep process that involves both the fulfillment of several engineering constraints and the accomplishment of scientific requirements. In this chapter, we will show how the simultaneous production and exploitation of different GIS maps depicting these criteria are pivotal in the landing site selection. Indeed, all of such constraints are presently evaluated through the use of GIS-based software. To show this, we will focus on the Martian site identification outline, providing multiple real examples taken from two ongoing study cases, i.e., the Simud Vallis landing site proposed by Pajola et al. (Icarus 268:355–381, 2016a) for the ESA ExoMars rover and the Eridania landing site proposed by Pajola et al. (Icarus 275:163–182, 2016b) for the NASA Mars 2020 landing site selection.
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Acknowledgements
We thank Dr. Henrik Hargitai and an anonymous reviewer for important comments and suggestions that highly improved the book’s chapter.
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Pajola, M., Rossato, S., Baratti, E., Kling, A. (2019). Planetary Mapping for Landing Sites Selection: The Mars Case Study. In: Hargitai, H. (eds) Planetary Cartography and GIS. Lecture Notes in Geoinformation and Cartography. Springer, Cham. https://doi.org/10.1007/978-3-319-62849-3_7
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