Potential mineral resources of the Moon

Przylibski, Tadeusz A.; Szczęśniewicz, Mateusz; Blutstein, Konrad

doi:10.7306/gq.1804

Artykuł - szczegóły

Tytuł artykułu

Potential mineral resources of the Moon

Autorzy

Przylibski Tadeusz A. , Szczęśniewicz Mateusz , Blutstein Konrad

Treść / Zawartość

Pełne teksty:

Przylibski_T_Potential_GQ_Vol._69_No. 3_2025.pdf

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Identyfikatory

DOI

10.7306/gq.1804

Warianty tytułu

Języki publikacji

Abstrakty

Highlights: – The most geochemically and geophysically evolved layer is the regolith; – Lunar regolith should be treated as a multi-component, pre-crushed ore; – The first object of exploitation and processing on the Moon will be regolith; – Potential deposit zones include outcrops of ultrabasic igneous rocks enriched in metals: Cr, Ti, REE, and PGM; – The most promising deposit areas are the lunar maria, primarily the Procellarum KREEP Terrane, circumpolar areas, and regions on the far side with a regolith thickness > 10 m. The homogeneity of the chemical and isotopic compositions of the Earth and the Moon facilitates the identification of potential mineral resources present and exploitable on the Moon. Current knowledge of the geological structure of the Moon indicates that the greatest geochemical and geophysical activity of the surface layer of the Moon’s crust lies in the regolith, and it is this that promises the most promising lunar raw material resource base. The regolith contains increased concentrations of life-supporting raw materials (H2O and O2), fuels and energy raw materials (³He, U, Th, H₂, and O₂), metallic raw materials (Fe, Ti, Zr, Hf, Eu, other REEs, Cr, Ni, Co, Al, and Si), rock raw materials (regolith, breccias, basalts, anorthosites, and others) and chemical raw materials (K, P, Cl, and S). Lunar regolith should be treated as a multi-component, pre-crushed ore, in which there are local enrichments of selected raw materials, and so initially will form the target of exploitation and processing on the Moon. The next potential deposit zones are outcrops of basic and ultrabasic igneous rocks, which may be enriched in metals such as Cr, Ti, REEs and PGMs, or places where these rocks are covered by only a thin layer of regolith. Such zones also include areas of occurrence of acidic igneous rocks, enriched in quartz, and perhaps also in many other valuable metals and chemical raw materials. The most important prospective areas in terms of the occurrence of raw materials in the regolith are the lunar maria, primarily the Procellarum KREEP Terrane, circumpolar areas, as well as areas on the far side of the Moon characterized by a regolith thickness exceeding 10 m.

Słowa kluczowe

lunar resources space resources KREEP basalts lunar maria extraterrestrial resources lunar regolith

Wydawca

Państwowy Instytut Geologiczny - Państwowy Instytut Badawczy

Czasopismo

Geological Quarterly

Rocznik

2025

Tom

Vol. 69, No. 3

Strony

art., no. 31

Opis fizyczny

Bibliogr. 89 poz., rys., tab.

Twórcy

autor

Przylibski Tadeusz A.

Tadeusz.Przylibski@pwr.edu.pl

Wrocław University of Science and Technology, Faculty of Geoengineering, Mining and Geology, Laboratory of Geology and Mineral Engineering, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław, Poland

https://orcid.org/0000-0002-8094-7944+

autor

Szczęśniewicz Mateusz

Wrocław University of Science and Technology, Faculty of Geoengineering, Mining and Geology, Laboratory of Geology and Mineral Engineering, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław, Poland

https://orcid.org/0000-0003-2006-7950

autor

Blutstein Konrad

Graduate of the Wrocław University of Science and Technology, Faculty of Geoengineering, Mining and Geology, doctor of the team’s alumni of the Laboratory of Geology and Mineral Engineering, Wybrzeże S. Wyspiańskiego 27, Wrocław, Poland

https://orcid.org/0000-0003-1337-774X

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