Si‐bearing metal and niningerite in Almahata Sitta fine‐grained ureilites and insights into the diversity of metal on the ureilite parent body. (October 2014)

• Record Type: Journal Article
• Authors: Horstmann, Marian; Humayun, Munir; Fischer‐Gödde, Mario; Bischoff, Addi; Weyrauch, Mona
• Is Part Of: Meteoritics & planetary science. Volume 49:Number 10(2014:Oct.)
• Page Start: 1948
• Page End: 1977
• Publication Date: 2014-10
• Subjects: Meteorites -- Periodicals; Planetology -- Periodicals; 523.4
• DOI: 10.1111/maps.12370
• Languages: English
• ISSNs: 1086-9379

Abstract

<abstract abstract-type="main" id="maps12370-abs-0001"> <title>Abstract</title> <p>A detailed mineralogical and chemical study of Almahata Sitta fine‐grained ureilites (MS‐20, MS‐165, MS‐168) was performed to shed light on the origin of these lithologies and their sulfide and metal. The Almahata Sitta fine‐grained ureilites (silicates <30 μm grain size) show textural and chemical evidence for severe impact smelting as described for other fine‐grained ureilites. Highly reduced areas in Almahata Sitta fine‐grained ureilites show large (up to ∼1 mm) Si‐bearing metal grains (up to ∼4.5 wt% Si) and niningerite [Mg<sub>>0.5, </sub>(Mn, Fe)<sub><0.5</sub>S] with some similarities to the mineralogy of enstatite (E) chondrites. Overall, metal grains show a large compositional variability in Ni and Si concentrations. Niningerite grains probably formed as a by‐product of smelting via sulfidation. The large Si‐Ni variation in fine‐grained ureilite metal could be the result of variable degrees of reduction during impact smelting, inherited from coarse‐grained ureilite precursors, or a combination of both. Large Si‐bearing metal grains probably formed via coalescence of existing and newly formed metal during impact smelting. Bulk and in situ siderophile trace element abundances indicate three distinct populations of (1) metal crystallized from partial melts in MS‐20, (2) metal resembling bulk chondritic compositions in MS‐165, and (3) residual metal in MS‐168. Almahata Sitta fine‐grained ureilites developed their distinctive mineralogy due to severe reduction during smelting. Despite the presence of E chondrite and ureilite stones in the Almahata Sitta fall, a mixing relation of E chondrites or their constituents and ureilite material in Almahata Sitta can be ruled out based on isotopic, textural, and mineral‐chemical reasons.</p> </abstract>