Andrieslombaardite, RhSbS, a new platinum-group mineral from the platiniferous Onverwacht Pipe, Republic of South Africa

IF 1.2 4区 地球科学 Q2 GEOLOGY South African Journal of Geology Pub Date : 2023-05-09 DOI:10.25131/sajg.126.0011
L. Cabri, A. McDonald, T. Oberthür, N. Tamura, A. Vymazalová, K. C. Ross, F. Melcher
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Abstract

A hundred years after the discovery of the Merensky Reef in 1924, it is appropriate to present the new mineral andrieslombaardite in honour of Andries Frederik Lombaard who was instrumental in its discovery. Andrieslombaardite, RhSbS, was first described as an unknown mineral from placer deposits associated with the Tulameen Alaskan-Uralian type complex, British Colombia, Canada (Raicevic and Cabri, 1976) but has since been reported from several other deposits including the platiniferous Driekop, Mooihoek, and Onverwacht pipes in the eastern Bushveld Complex, South Africa. The mineral and the name were approved by the Commission on New Minerals Nomenclature and Classification (CNMNC) of the International Mineralogical Association (IMA no. 2022-076) based on data in the co-type samples from Onverwacht and a co-type sample from the Yubdo stream, Birbir River, Ethiopia. Andrieslombaardite in the Onverwacht sample is a single 8 x 20 μm grain attached to laurite in a matrix of altered silicate and Fe-oxyhydroxide minerals. In the Yubdo samples, there are many grains of pale brownish gray andrieslombaardite up to 25 x 55 μm in size, included in Pt-Fe alloys, some associated with erlichmanite, and others attached to bornite and chalcopyrite. The reflectance values (R%) measured in air and in oil at the COM wavelengths are 48.3 and 33.0 (470 nm), 49.3 and 34.0 (546 nm), 51.0 and 35.9 (589 nm), and 51.8 and 36.7 (650 nm). The colour values x, y, Y, λd, and Pe in air are 0.317, 0.322, 50.3, 580, and 3.2, and in oil are 0.319, 0.324, 35.6, 579, and 4.5. The composition of andrieslombaardite is ideally RhSbS, but it contains variable amounts of Fe, Pt, Pd, and Ir that may substitute for Rh. The mineral is cubic with unit-cell dimensions of a = 6.0278(4) Å, V = 219.01(6) Å3 and Z = 4. It was synthesised at 400 and 550°C using stoichiometric elemental amounts. It is a member of the cobaltite group. The mineralisation of the intrusive dunite pipes was probably introduced at high temperatures, under magmatic conditions. The primary assemblages were to a certain degree overprinted and redistributed by low-temperature hydrothermal fluids. The Pt-Fe alloys from Yubdo containing PGM inclusions such as andrieslombaardite in the Yubdo-Alaskan-type complex were formed at some post-magmatic stage owing to PGE remobilisation during hydrothermal or metamorphic episodes.
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Andrieslombaardite,RhSbS,一种来自南非共和国Onverwacht管道的新铂族矿物
1924年梅伦斯基礁被发现一百年后,为了纪念在其发现过程中发挥重要作用的安德里斯·弗雷德里克·隆巴德,我们可以将新矿物安德里斯·隆巴德(andrieslombaardite)赠送给大家。Andrieslombaardite,RhSbS,最初被描述为一种未知矿物,来自加拿大不列颠哥伦比亚省Tulameen Alaskan Uralian型杂岩的砂矿(Raicevic和Cabri,1976),但后来又被报道来自其他几个矿床,包括南非Bushveld杂岩东部的含铂Driekop、Mooihoek和Onverwacht管道。该矿物和名称由国际矿物学协会新矿物命名和分类委员会(CNMNC)(IMA编号:2022-076)根据Onverwacht的同型样品和埃塞俄比亚Birbir河Yubdo河的同型样本中的数据批准。Onverwacht样品中的Andrieslombaardite是一个8 x 20μm的颗粒,附着在蚀变硅酸盐和氧化铁矿物基质中的月桂石上。在Yubdo样品中,Pt-Fe合金中含有许多大小达25 x 55μm的浅棕灰色安德里斯洛姆巴rdite颗粒,其中一些与伊利石有关,另一些与斑铜矿和黄铜矿有关。在空气和油中测得的COM波长的反射率值(R%)分别为48.3和33.0(470 nm)、49.3和34.0(546 nm)、51.0和35.9(589 nm)以及51.8和36.7(650 nm)。在空气中的色值x、y、y、λd和Pe分别为0.317、0.322、50.3、580和3.2,在油中分别为0.319、0.324、35.6、579和4.5。andrieslombaardite的组成理想地为RhSbS,但它含有可替代Rh的可变量的Fe、Pt、Pd和Ir。该矿物为立方体,晶胞尺寸为a=6.0278(4)Å,V=219.01(6)Å3和Z=4。它是在400和550°C下使用化学计量元素量合成的。它是钴矿群的一员。侵入性纯橄榄岩管道的矿化作用可能是在高温、岩浆条件下引入的。初级组合在一定程度上被低温水热流体叠加和重新分布。Yubdo-Alaskan型杂岩中来自Yubdo的含有PGM包裹体的Pt-Fe合金,如andrieslombaardite,是在热液或变质过程中由于PGE的再活化而在岩浆后期形成的。
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来源期刊
CiteScore
3.60
自引率
5.60%
发文量
18
审稿时长
>12 weeks
期刊介绍: The South African Journal of Geology publishes scientific papers, notes, stratigraphic descriptions and discussions in the broadly defined fields of geoscience that are related directly or indirectly to the geology of Africa. Contributions relevant to former supercontinental entities such as Gondwana and Rodinia are also welcome as are topical studies on any geoscience-related discipline. Review papers are welcome as long as they represent original, new syntheses. Special issues are also encouraged but terms for these must be negotiated with the Editors.
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