- 1PHAB, University of Oslo, Centre for Planetary Habitability, Oslo, Norway (stephanie.werner@geo.uio.no)
- *A full list of authors appears at the end of the abstract
Selene’s Explorer for Roughness, Regolith, Resources, Neutrons and Elements (SER3NE) is a small satellite mission performing gamma-ray and neutron spectroscopy (University of Oslo), near-infrared spectroscopy (Royal Observatory of Belgium and Royal Belgian Institute for Space Aeronomy) , and laser altimetry, roughness, and albedo observations (Institute for Planetary Reserch - DLR) at unprecedented spectral and ground resolution. The aim is to characterize the lunar surface to unravel its volatile origin and delivery processes, to uncover the geological processes that shaped the Moon, to prospect lunar resources for ISRU at future landing sites, to determine the exact neutron lifetime and the orbital evolution of the Earth-Moon system.
The instruments will be carried by the modular, single-failure tolerant TUBiX20 satellite platform (Technical University of Berlin). To ensure the desired global coverage and resolution for all instruments the satellite will orbit the Moon on a eccentric polar orbit with a slowly, naturally drifting argument of perilune over the mission lifetime of one year. This mission concept is a pre-Phase A Study led by University of Oslo under an ESA contract.
Christian Althaus, Julian Bartholomäus, Benedict Grefen, Matthias Grott, Lisa Hafemeister, Andre Henschke, Christian Hüttig, Ramsey Al Jebali, Clement Jonglez, Roland Kalms, Özgür Karatekin, Julian Klein, Elizabeth Klioner, Anja Kohfeldt, Agata Krzesinska, Kay Lingenauber, Manuel Ligges, Maria Meitinger, Jörg Neumann, Francois Poulet, Birgit Ritter, Séverine Robert, Alexander Stark, Enrico Stoll, Luis Filipe Alves Teodoro, Konstantinos Vasiliou, Rebecka Wahlén, Peter Weßels, Stephanie C. Werner
How to cite: Werner, S. C. and the The SER3NE Team: SER3NE - A small orbiter mission to the Moon, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8239, https://doi.org/10.5194/egusphere-egu25-8239, 2025.