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X-ray fluorescence for Moon exploration and exploitation
Carapelle, Alain; Lomax, Beth; Naito, Masayuki et al.
2022In Proceedings of International Astronautical Congress
Peer reviewed
 

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Keywords :
XRF; ISRU; PXG
Abstract :
[en] X-ray Fluorescence (XRF) is a spectroscopic method that allows detection and measurements of the amount of any atoms heavier than Na. XRF spectrometers are used in wide range of application and are paramount instruments for planetary science since the beginning of space exploration. Improvements of detectors and electronics allowed to improve capabilities of such planetary instruments. Up to now, all the XRF space instruments have used radioisotopes sources as excitation sources. The only exception is the very last PIXL instrument sent on Mars by NASA on-board Perseverance, which uses an X-ray tube. We propose to use XRF for three different instruments for the exploration and exploitation of the Moon. The first instrument will be placed on a rover for geological survey; this instrument will used pyroelectric X-ray generator as an excitation source. We reached an energy resolution of 121.17 eV using a Silicon Drift Detector and we have reduced measurement fluctuation from 25.2% to 3.7% thanks to renormalization process. The current development of this first instrument has reached a Technology Readiness Level of 6 (full-scale model demonstration in relevant environment). The second instrument will be used by astronauts in a handheld version and will use a miniature X-ray tube. The device will allow rapid sampling of rocks to allow the best choice of samples for earth return. The device will use machine learning and will present results on simple way to tell astronauts if a sample is worth collecting. The current Technology Readiness Level of this second instrument is 4 (Functional verification). The third instrument will be used to monitor the Oxygen production unit from lunar regolith. Oxygen extraction is taking place using a method called molten salt electrolysis, involving placing regolith in a metal basket with molten calcium chloride salt to serve as an electrolyte, heated to 950°C. At this temperature, the regolith remains solid. But passing a current through it causes the oxygen to be extracted from the regolith and migrate across the salt to be collected at an anode. As a bonus, this process also converts the regolith into usable metal alloys. XRF will be used to follow the concentration of atoms involved in the process and therefore to monitor the oxygen production. The current TRL level of this third instrument is 3 (Proof of concept).
Research Center/Unit :
CSL - Centre Spatial de Liège - ULiège
European Space Agency (ESA)
National Institutes for Quantum Science and Technology (Japan)
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Carapelle, Alain  ;  Université de Liège - ULiège > Centres généraux > CSL (Centre Spatial de Liège) ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Lomax, Beth;  European Space Agency
Naito, Masayuki;  National Institute for Quantum Science and Technology
Habraken, Serge  ;  Université de Liège - ULiège > Centres généraux > CSL (Centre Spatial de Liège) ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Language :
English
Title :
X-ray fluorescence for Moon exploration and exploitation
Alternative titles :
[fr] Fluorescence X pour l'exploration et l'exploitation lunaire
Publication date :
September 2022
Event name :
International Astronautical Congress
Event organizer :
International Astronautical Federaion
Event place :
Paris, France
Event date :
18-22/9/2022
Audience :
International
Main work title :
Proceedings of International Astronautical Congress
Publisher :
International Astronautical Federation
Peer reviewed :
Peer reviewed
Name of the research project :
ALEXIS
Funders :
BELSPO - Politique scientifique fédérale [BE]
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since 27 October 2022

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