Czy na Dolnym Śląsku występują naturalne analogi skał księżycowych?

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

doi:10.7306/2024.2

Artykuł - szczegóły

Tytuł artykułu

Czy na Dolnym Śląsku występują naturalne analogi skał księżycowych?

Autorzy

Przylibski Tadeusz A. , Szczęśniewicz Mateusz , Blutstein Konrad

Treść / Zawartość

Pełne teksty:

Przylibski_T_Czy na Dolnym_PG_Vol. 72_nr 1_2024.pdf

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Identyfikatory

DOI

10.7306/2024.2

Warianty tytułu

Are there natural analogues of Moon rocks in Lower Silesia?

Języki publikacji

Abstrakty

We describe the geological structure of the Moon and its evolution from the time of its joint formation with the Earth to the present. The common origin of both of these bodies justifies the search for analogues of the rocks that build the Earth andthe Moon. On this basis, we characterize the rocks that constitute the crust of the Moon. These comprise rocks of the primary planetary anorthosite crust: anorthosites and, subordinately, other gabbroid rocks (gabbros, troctolites, norrites). These rocks make up the lunar highlands and mainly build the far side of the Moon. On the near side, there are vast areas covered with basaltoids several hundred meters thick, of various ages: the lunarmaria. These two types of igneous rocks constitute the Moon's crust. Its surface is coveredwith materialproduced by impact metamorphism from incoming asteroids, meteoroids, micrometeoroids and interplanetary dust, as well as resulting from the crust's interaction with solar wind particles and cosmic radiation. This regolith comprises loose material a few to several meters thick. We compare the chemical composition of these lunar igneous rocks with the chemical composition of the igneous rocks of Lower Silesia. Basaltoids, anorthosites, gabbros and troctolites were included in our analysis. We conclude, unsurprisingly, that it is currently impossible to indicate the occurrence of natural analogues of lunar rocks in Lower Silesia. There are large differences between the chemical composition between the rocks constituting the primary planetary crust of the Moon and the igneous alkaline rocks of Lower Silesia, the latter representing strongly differentiated igneous rocks of the Earth's crust and upper mantle. Nevertheless, in the case of basaltoids, it will likely be possible in the near future to find rocks that can, with some approximation, be considered analogues of lunar basaltoids. At present, potential locations of lunar-like basalts and foidites include the Zaręba and Księginki quarries near Lubań. In the case of plutonie rocks, especially anorthosites, Lower Silesian analogues of lunar rocks will be very approximate. However, based on basaltoid rocks from Lower Silesia, and perhaps later also using gabbroid rocks, it should be possible to produce a natural analogue of the lunar regolith. Rock material from terrestrial analogues will have to be significantly processed both physically and chemically to obtain the composition and structure of this regolith material. These considerations, however, are not the purpose of this work. We focus primarily on analogies of chemical and mineral composition, as the basic features enabling the production of a lunar regolith analogue. We are particularly interested in pointing out analogies resulting from the composition of the parent magmas of these rocks, as reflected in the chemical composition of the rocks and their mineral composition. Due to significant differences in the age of crystallization of lunar magmas and their conditions of this crystallization compared to the rocks of Lower Silesia (on Earth), it is not presently possible to indicate Lower Silesian age-analogues of lunar rocks or structural and textural analogues.

Słowa kluczowe

księżyc bazalt anortozyt brekcja skaleniowa meteoryt księżycowy regolit synestia

moon basalt anorthosite feldspar breccia lunar meteorite regolith synestia

Wydawca

Państwowy Instytut Geologiczny - Państwowy Instytut Badawczy

Czasopismo

Przegląd Geologiczny

Rocznik

2024

Tom

Vol. 72, nr 1

Strony

26--46

Opis fizyczny

Bibliogr. 98 poz., fot., map., rys., tab., wykr.

Twórcy

autor

Przylibski Tadeusz A.

Tadeusz.Przylibski@pwr.edu.pl

Wydział Geoinżynierii, Górnictwa i Geologii, Politechnika Wrocławska, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław

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

autor

Szczęśniewicz Mateusz

Mateusz.Szczesniewicz@pwr.edu.pl

Wydział Geoinżynierii, Górnictwa i Geologii, Politechnika Wrocławska, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław

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

autor

Blutstein Konrad

Konrad.Blutstein@pwr.edu.pl

Wydział Geoinżynierii, Górnictwa i Geologii, Politechnika Wrocławska, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław

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

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