کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
9951512 | 1646781 | 2018 | 40 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Chalcophile-siderophile element systematics of hydrothermal pyrite from martian regolith breccia NWA 7533
دانلود مقاله + سفارش ترجمه
دانلود مقاله ISI انگلیسی
رایگان برای ایرانیان
کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
ژئوشیمی و پترولوژی
پیش نمایش صفحه اول مقاله
![عکس صفحه اول مقاله: Chalcophile-siderophile element systematics of hydrothermal pyrite from martian regolith breccia NWA 7533 Chalcophile-siderophile element systematics of hydrothermal pyrite from martian regolith breccia NWA 7533](/preview/png/9951512.png)
چکیده انگلیسی
Unlike other martian meteorites studied so far, Martian regolith breccia NWA 7533 and paired meteorites that have sampled 4.4â¯Ga-old impact lithologies show only sulfides of hydrothermal origin (mostly pyrite (<1â¯vol.%) and scarce pyrrhotite). NWA 7533 pyrite has been analyzed for 25 chalcophile-siderophile trace elements with laser ablation-inductively coupled plasma mass spectrometer (LA-ICPMS). Micronuggets of highly siderophile elements-HSE (Os, Ir, Pt, Ru, Rh) along with occasional detection of Mo and Re were observed in half of the 52 analyzed crystals as random concentration spikes in time-resolved LA-ICPMS data. These nuggets are interpreted as variably altered remnants from repeated meteorite bombardment of the early martian crust, as are chondritic Ni/Co ratios of pyrite (10-20). Pyrite displays superchondritic S/Se (54,000-3300) and Te/Se (0.3 to >1). The reasonably good positive correlation (R2â¯=â¯0.72) between Se and Ni reflects a temperature control on the solubility of both elements. Apart from the chalcogens S, Se and Te, pyrite appears to be a minor contributor (<20%) to the whole-rock budget for both HSE (including Ni and Co) and chalcophile metals Ag, As, Au, Cu, Hg, Pb, Sb, Tl and Zn. This deficit can result from (i) high (>400â¯Â°C) temperature crystallization for NWA 7533 pyrite, as deduced from its Se and Ni contents, (ii) magmatic sulfide-depletion of brecciated early martian crust, (iii) precipitation from near neutral H2S-HS-H2O-rich hydrothermal fluids that did not provide halogen ligands for extensive transport of chalcophile-siderophile metals. It is suggested that the 1.4â¯Ga lithification event that precipitated hydrothermal pyrite left the chalcophile-siderophile element budget of the early martian crust nearly unmodified, except for S, Se and Te.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Geochimica et Cosmochimica Acta - Volume 241, 15 November 2018, Pages 134-149
Journal: Geochimica et Cosmochimica Acta - Volume 241, 15 November 2018, Pages 134-149
نویسندگان
J.-P. Lorand, R.H. Hewins, M. Humayun, L. Remusat, B. Zanda, C. La, S. Pont,