Sahara 03505 sulfide-rich iron meteorite: Evidence for efficient segregation of sulfide-rich metallic melt during high-degree impact melting of an ordinary chondrite

被引:18
作者
D'Orazio, Massimo [1 ]
Folco, Luigi [2 ]
Chaussidon, Marc [3 ]
Rochette, Pierre [4 ]
机构
[1] Univ Pisa, Dipartimento Sci Terra, I-56126 Pisa, Italy
[2] Univ Siena, Museo Nazl Antartide, I-53100 Siena, Italy
[3] Nancy Univ, CRPG, INSU, CNRS,UPR 2300, F-54501 Vandoeuvre Les Nancy, France
[4] Univ Aix Marseille 3, CEREGE, CNRS, F-13545 Aix En Provence, France
关键词
EARLY SOLAR-SYSTEM; OXYGEN-ISOTOPE; PARENT BODY; S SYSTEM; BULLETIN; FRACTIONATION; CHONDRULES; MINERALOGY; PETROLOGY; SULFUR;
D O I
10.1111/j.1945-5100.2009.tb00730.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Sahara 03505 meteorite is a 65 g sulfide-rich iron found in all undisclosed locality of the Sahara. It consists of roughly equal volumetric proportion of polycrystalline troilite (crystal size 1.5-7.5 mm) enclosing cellular/dendritic metallic Fe-Ni (width of the dendrite arms, similar to 100 mu m). The mineral assemblage is completed by sparse skeletal crystals of chromite, abundant droplets, 5100 pill in size, of anhydrous Fe-, Fe-Na-, and Fe-Mn-Mg-Ca-Na-K-phosphates, tiny crystals of schreibersite, and particles of metallic Cu. The medium- to fine-grained quench texture, and cooling modeling Suggest that Sahara 03505 formed through crystallization of a sulfur-rich metallic melt under rapid cooling conditions (1-4 degrees C s(-1)). The low troilite/metallic Fe-Ni ratio (similar to 0.6 by weight) shows that this liquid was generated at much higher temperatures (>1300 degrees C) with respect to the FeS-Fe,Ni cotectic liquids. Based oil bulk chemistry and oxygen isotope composition of chromite, we propose that Sahara 03505 formed by extensive impact melting of an ordinary chondrite lithology, followed by the efficient segregation of the immiscible silicate and metallic liquids. The sulfur-rich metallic liquid rapidly cooled either by radiation into space as a small lump, or by conduction to a chondrite country rock as a vein intruded into the walls of an impact crater. Sahara 03505 belongs to a small group of sulfide-rich iron meteorites which are characterized by medium- to fine-grained quench textures and by bulk chemistry that is different from the other iron meteorite groups. We propose here to use the descriptive term "sulfide-irons" for this meteorite group, by analogy with the stony-irons.
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页码:221 / 231
页数:11
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