dc.creator
Besse, Sebastien
dc.creator
Bogert, Carolyn H. van der
dc.creator
Bahia, Rickbir
dc.creator
Prissang, René
dc.creator
Ivanov, Mikhail A.
dc.creator
Hiesinger, Harald
dc.creator
Michael, Gregory
dc.creator
Pasckert, Jan Hendrik
dc.creator
Walter, Sebastian H. G.
dc.identifier
https://doi.org/10.35003/PI5HHE
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-41915
dc.description
Abstract: <p>
The South Pole-Aitken (SPA) basin is the oldest, largest visible impact structure on the Moon, making it a high priority science site for exploration missions. The 492 km diameter Apollo peak-ring basin is one of the youngest and largest basins within the SPA basin. We selected three Regions of Interest (ROI) in the Apollo basin for which the landing and operational hazards are minimized and evaluated
their science and in situ resource utilisation (ISRU) potential. We examined topography, slope, crater density, rock abundance, geologic mapping, mineralogy, and inferred subsurface stratigraphy within each ROI. The results show that the terrain is safe for landing without precision landing (within a few hundred meters). The mare materials have high ISRU potential with relatively high FeO
(~16-20 wt%) and TiO2 (~3-10 wt%) contents. Two robotic exploration mission architectures were examined for their scientific potential: <p>
(1) lander and rover with a dedicated payload suite, and <p>
(2) the same architecture with sample return capability. <p>
In-situ observations can address six of seven NRC concepts (1-3, 5-7) and Campaigns 1 and 5 of the European Space Agency's Strategy for Science at the Moon.
dc.subject
Astronomy and Astrophysics
dc.subject
South Pole-Aitken (SPA)
dc.subject
ISRU potentital
dc.subject
FeO, TiO2 contents
dc.subject
robotic exploration mission architectures
dc.subject
sample return capability
dc.subject
ESA Campaigns Moon
dc.title
Replication Data for: Characterization of high-priority landing sites for robotic exploration missions in the Apollo basin, Moon