Marsaalamite-(Y), Y(MoO<sub>4</sub>)OH, a new molybdate mineral from the Um Safi area, Marsa Alam District, Central Eastern Desert, Egypt

Abstract Marsaalamite-(Y), ideally Y(MoO 4 )OH, is a new molybdate mineral discovered in the greisenised Um Safi F-rich granite located in the Marsa Alam District, Central Eastern Desert, Egypt. It typically occurs as inclusions in or intergrowths with F-rich zinnwaldite. It forms micaceous aggregates, with sizes varying from 0.1 to 1 mm. Marsaalamite-(Y) is non-magnetic, white in colour, and has an earthy lustre and white streak. It is brittle (3–4 Mohs) and has basal cleavages {010}. The calculated density is 4.90 g.cm –3 based on the empirical formula and unit-cell parameters refined from powder X-ray diffraction data. Marsaalamite-(Y) is associated with arsenopyrite, baryte, bastnäsite-(Ce), cassiterite, chernovite-(Y), columbite-(Fe), fluocerite-(Ce), fluorite, iron oxy-hydroxides, löllingite, molybdenite, monazite-(Ce), pyrite, quartz, rutile, thorite, wolframite, wulfenite, xenotime-(Y) and several unidentified phases. The empirical formula is (Y 0.67 Er 0.10 Dy 0.08 Yb 0.08 Ho 0.02 Lu 0.02 Tm 0.02 Ca 0.01 ) Σ1.00 (Mo 0.95 S 0.03 As 0.01 P 0.01 ) Σ1.00 O 4.00 [(OH) 0.88 F 0.11 Cl 0.01 ] Σ1.00 ; the ideal end-member formula is Y(MoO 4 )(OH). The presence of a hydroxyl group has been confirmed by Raman and infrared spectroscopy, and its concentration has been calculated from the stoichiometry. Marsaalamite-(Y) is the natural (OH)-dominant analogue of synthetic Y(MoO 4 )F. It is monoclinic, space group P 2 1 /c , with unit-cell parameters a = 5.1863(7) Å, b = 12.3203(11) Å, c = 6.6953(7) Å, β = 114.173(8)°, V = 390.30(8) Å 3 , and Z = 4. Extreme fractionation of the parental halogen-rich, A-type granitic magma triggered the greisenisation of the granite. Marsaalamite-(Y) occurred simultaneously with or immediately after the crystallisation of F-rich zinnwaldite based on the textural relationship. Therefore, the crystallisation of marsaalamite-(Y) was most likely to have been controlled by fluid-induced processes rather than magmatic conditions. The new mineral has been approved by the Commission on New Minerals, Nomenclature and Classification of the International Mineralogical Association (IMA 2024-050) and named after the Marsa Alam District, Al-Bahr Al-Ahmer Governorate, Egypt.

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Journal
Mineralogical Magazine
Published
2024-12-27
DOI
https://doi.org/10.1180/mgm.2024.103
Primary Topic
Crystal Structures and Properties
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article
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article

Marsaalamite-(Y), Y(MoO4)OH, a new molybdate mineral from the Um Safi area, Marsa Alam District, Central Eastern Desert, Egypt

Cristian Biagioni, Jiří Sejkora, Martin Števko, Tomáš Mikuš et al.
Mineralogical Magazine
Crystal Structures and Properties
article

Marsaalamite-(Y), Y(MoO4)OH, a new molybdate mineral from the Um Safi area, Marsa Alam District, Central Eastern Desert, Egypt

Cristian Biagioni, Jiří Sejkora, Martin Števko, Tomáš Mikuš, Hans‐Jürgen Förster, Peter Bačík, Martin Ondrejka, Pavel Uher, Nasser M. Mahdy
article en

Abstract

Abstract Marsaalamite-(Y), ideally Y(MoO 4 )OH, is a new molybdate mineral discovered in the greisenised Um Safi F-rich granite located in the Marsa Alam District, Central Eastern Desert, Egypt. It typically occurs as inclusions in or intergrowths with F-rich zinnwaldite. It forms micaceous aggregates, with sizes varying from 0.1 to 1 mm. Marsaalamite-(Y) is non-magnetic, white in colour, and has an earthy lustre and white streak. It is brittle (3–4 Mohs) and has basal cleavages {010}. The calculated density is 4.90 g.cm –3 based on the empirical formula and unit-cell parameters refined from powder X-ray diffraction data. Marsaalamite-(Y) is associated with arsenopyrite, baryte, bastnäsite-(Ce), cassiterite, chernovite-(Y), columbite-(Fe), fluocerite-(Ce), fluorite, iron oxy-hydroxides, löllingite, molybdenite, monazite-(Ce), pyrite, quartz, rutile, thorite, wolframite, wulfenite, xenotime-(Y) and several unidentified phases. The empirical formula is (Y 0.67 Er 0.10 Dy 0.08 Yb 0.08 Ho 0.02 Lu 0.02 Tm 0.02 Ca 0.01 ) Σ1.00 (Mo 0.95 S 0.03 As 0.01 P 0.01 ) Σ1.00 O 4.00 [(OH) 0.88 F 0.11 Cl 0.01 ] Σ1.00 ; the ideal end-member formula is Y(MoO 4 )(OH). The presence of a hydroxyl group has been confirmed by Raman and infrared spectroscopy, and its concentration has been calculated from the stoichiometry. Marsaalamite-(Y) is the natural (OH)-dominant analogue of synthetic Y(MoO 4 )F. It is monoclinic, space group P 2 1 /c , with unit-cell parameters a = 5.1863(7) Å, b = 12.3203(11) Å, c = 6.6953(7) Å, β = 114.173(8)°, V = 390.30(8) Å 3 , and Z = 4. Extreme fractionation of the parental halogen-rich, A-type granitic magma triggered the greisenisation of the granite. Marsaalamite-(Y) occurred simultaneously with or immediately after the crystallisation of F-rich zinnwaldite based on the textural relationship. Therefore, the crystallisation of marsaalamite-(Y) was most likely to have been controlled by fluid-induced processes rather than magmatic conditions. The new mineral has been approved by the Commission on New Minerals, Nomenclature and Classification of the International Mineralogical Association (IMA 2024-050) and named after the Marsa Alam District, Al-Bahr Al-Ahmer Governorate, Egypt.

Mineralogical MagazineVol. 89(3)
University of Pisa (IT), Slovak Academy of Sciences (SK), National Museum (CZ), Nuclear Materials Authority (EG), Earth Science Institute of the Slovak Academy of Sciences (SK), GFZ Helmholtz Centre for Geosciences (DE), Comenius University Bratislava (SK)
Openalex Percentile: Top 85%
Crystal Structures and Properties
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