A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine to extensively aqueously altered CM chondrites, using SEM and EMP techniques

Bullock, E. S.

Gounelle, M.

Grady, Monica

Russell, S. S.

English

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Open Research OnlineThe Open University’s repository of research publicationsand other research outputsA study of the morphology, composition and mineralassociations of Fe-Ni sulphides in CM carbonaceouschondritesConference or Workshop ItemHow to cite:Bullock, E. S.; Gounelle, M.; Grady, Monica and Russell, S. S. (2004). A study of the morphology, compositionand mineral associations of Fe-Ni sulphides in CM carbonaceous chondrites. In: 35th Lunar and Planetary ScienceConference, 15-19 Mar 2004, Houston, Texas, USA.For guidance on citations see FAQs.c© [not recorded]Version: [not recorded]Link(s) to article on publisher’s website:http://www.lpi.usra.edu/meetings/lpsc2004/pdf/1653.pdfCopyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyrightowners. For more information on Open Research Online’s data policy on reuse of materials please consult the policiespage.oro.open.ac.ukA STUDY OF THE MORPHOLOGY, COMPOSITION AND MINERAL ASSOCIATIONS OF FE-NI SULPHIDES IN CM CARBONACEOUS CHONDRITES E. S. Bullock1, M. Gounelle1,2, M. M. Grady1, S. S. Russell1, 1 Department of Mineralogy, The Natural History Museum, Cromwell Road, London SW7 5BD, UK. e-mail e.bullock@nhm.ac.uk.  2 CSNSM - Université Paris 11, Bâtiment 104, 91 405 Orsay Campus, France.  Introduction: The CM chondrites are a large group that show a wide range of aqueous altera-tion features [1]. Whilst a lot of attention has been paid to primary and secondary phases in the CMs, such as phyllosilicates [e.g. 2], carbonates [3], sulphates [4] and chondrule olivines and py-roxenes [e.g. 5], much less attention has been given to the opaque phases in these chondrites. The sulphides in particular are very interesting, as they might be products of sulphuration of metal grains by H2S in the nebula [6]. Previous studies [e.g. 7] have tended to concentrate on sulphides in particular CMs; only one study [8] has looked for differences between the CM sul-phides. Our study looks at some of the CMs in-cluded in that study, plus an additional group of CMs, to assess whether the observations noted by [8] apply to these samples. Method: Five sections of the CM1 chondrite ALH88045 were studied, as well as a range of relatively pristine to extensively aqueously al-tered CM2’s. The samples were primarily studied in a Jeol 5900LV Scanning Electron Microscope operating at 20kV and 1nA, and a WD of 10mm. This allowed us to look at the morphology and size range of the grains, and to obtain major ele-ment analyses of the sulphides. Accurate analy-ses of the minor elements present in the sul-phides were obtained using a Cameca SX50 Elec-tron Microprobe operating at 20kV and 20nA.  Results: Results from the CM2s are pre-sented in order of increasing alteration according to [9]:  Murchison, the least altered CM2 of the group we studied, shows a range of Fe-Ni sul-phide compositions from pyrrhotite, through in-termediate sulphides to pentlandite   (Fig. 1). Stoichiometric FeS (troilite) is also present. Most of the sulphides are pyrrhotite. The sulphides are large (>40µm in diameter, up to >100µm). They range in shape from rounded, “blobby” grains to euhedral grains in the matrix, and also form dis-continuous rims around chondrules. Most are cracked across their surface, though not all. Some of the sulphides contain inclusions of matrix-like material: others have been partially oxidised to magnetite.    Bells, slightly more altered than Murchison, is less diverse in terms of its sulphide mineralogy. Again, both pyrrhotite and pentlandite are pre-sent, but there is no troilite, and no sulphide of an intermediate composition. (Fig. 1) The sulphides are rounded, cracked, and occur both as isolated grains in the matrix and as rims around chon-drules.  Pollen, in contrast to the previous two chon-drites, contains only pentlandite. The Ni content varies between 28 – 31wt% (Fig. 1). The grains in the matrix are around 10µm in diameter, rounded, and are dispersed sparsely throughout the matrix. Pentlandite is also found at one edge of a por-phyritic olivine chondrule, within the fine-grained rim.  Mighei, like the majority of CM2s in this study, contains a range of Ni-poor to Ni-rich pyr-rhotite grains, and Ni-poor and Ni-rich pentland-ites. Few grains of an intermediate composition are found (Fig. 1). Pyrrhotite and pentlandite of-ten occur within the same grain, but are not inter-grown. A distinct boundary can be seen between the phases.  Fe-Ni sulphide grains are rare in Mighei, but occur throughout the matrix as rounded, slightly cracked grains, and also as dis-continuous rims around chondrules. The matrix grains can be up to 100µm in diameter. Rarely, Fe-sulphides and Fe-oxides form thick rims around metal grains (Fig 2). Cold Bokkeveld, the most altered CM2, con-tains both pyrrhotite and pentlandite (Fig. 1). These two phases are rarely intergrown, and oc-cur as small (10 - 30µm), irregular grains in the matrix. Some grains show alteration at the edges, others show no alteration but are extensively cracked along the surface. Two of the Fe-Ni sul-phides show enrichment in Cu (0.15 and 0.38wt%) and Cr (0.13 and 0.12wt%) respectively. We have also included in our study some CM2s that were not included in the alteration index of [9]. These are given below. ALH81002: This chondrite, like Pollen, con-tains only pentlandite. The Ni content though is much more homogenous, between 31.5 – 33.7wt% (Fig. 1). The grains in the matrix are between 5 and 30µm, whilst the grains associated with chondrules are between 5 and 50µm.  Lunar and Planetary Science XXXV (2004) 1653.pdfEssebi: This unusually magnetite-rich CM2 also contains very interesting sulphide grains. Pyrrhotite and pentlandite (but not troilite or in-termediate sulphide) are present (Fig. 1). The grains occur as irregular masses around silicate grains, as discreet grains in the matrix and as as-sociated phases with chondrules. One interesting “flame-like” intergrowth of pyrrhotite and pent-landite has been noted (Fig. 3). QUE99355: Pyrrhotite, pentlandite and troilite are found in QUE99355 (Fig. 1). Clear boundaries can be seen between the pyrrhotite and pentland-ite where they occur in the same grain: the phases are not intergrown. The grains are found in the matrix, and associated with chondrules, where they are found inside the fine-grained rim.  The sulphides in the CM1 chondrite ALH88045 are the most diverse found in any sin-gle CM chondrite. The size of the sulphides ranges from <10µm to >300µm. They occur as rims around remnant chondrules and lumps of matrix, and also occur as isolated grains in the matrix. Some of the matrix grains are rounded: others are irregular, forming “tendrils” or “crosses” that taper out into the matrix (Fig. 4). The rims around Mg-rich matrix lumps and rem-nant chondrules are discontinuous and variable in thickness, between 10µm and 150µm. The grains are often porous. The composition of the sulphides in ALH88045 ranges from pyrrhotite ([Fe,Ni]1-xS) to pentlandite ([Fe,Ni]9S8) with sul-phides of an intermediate composition also ap-parently present (Fig. 1). The pyrrhotite and pent-landite are very finely intergrown. The intermedi-ate sulphides are probably a result of beam over-lap of the pyrrhotite and pentlandite in this case: high-magnification images show the level of inter-growth (Fig 5.) Discussion: We agree with [8] that the al-teration that has occurred to the Fe-Ni sulphides in the CM chondrites does not follow any simple direction. The number and texture of the sul-phides does not change with increasing altera-tion. This supports a nebula origin for CM sul-phides. Aqueous alteration of the sulphides has however had an effect on composition: the sul-phides that have undergone most alteration have a lower Ni content in their pyrrhotite.  References: [1] Zolensky, M. E. et al (1997) GCA 61 p5099-5115. [2] Grady, M. M. et al (1997) Workshop on Parent-body and nebular modification of chondritic materials, LPI technical report, p17-18. [3] Benedix, G. K. et al (2003) GCA 67 p1577-1588. [4] Lee, M. R. (1993) Meteoritics 28 p53-62. [5] Hanowsi, N. P & Brearley, A. J. (2001) GCA 65 495-518. [6] Zolensky, M. E. & Thomas, K. L. (1995) GCA 59 4707-4712. [7]Kerridge, J. F et al (1979) EPSL 43 p1-4 [8] Zolensky, M. E. & Loan, L. (2003) LPI XXXIV, 1235. [9] Browning, L. B et al (1996) GCA 60 p2621-2633. [10] Lauretta et al (1998) MAPS 33 p821-833.  Fig. 1. Triangular diagrams showing the composi-tional range of Fe-Ni sulphides in CM1 and CM2 car-bonaceous chondrites. Bottom row of diagrams shows increasing alteration, according to [8]; top row of dia-grams shows CM2s not included in the study by [8].   Fig. 2. Metal grain with Fe-oxide and Fe-Ni sulphide rims in Mighei. Scale bar is 30µm. Fig. 3. Intergrown pyrrhotite and pentlandite in Essebi. Fig. 4. BSE image of intergrown pyrrhotite and pentlandite (white) in matrix (grey) in ALH88045. Scale bar is 200µm. Fig. 5 High-contrast image of intergrown pyrrhotite and pentlandite in ALH88045. Scale bar is 5µm.  Lunar and Planetary Science XXXV (2004) 1653.pdf

A study of the morphology, composition and mineral associations of Fe-Ni sulphides in CM carbonaceous chondrites

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A study of the morphology, composition and mineral associations of Fe-Ni sulphides in CM carbonaceous chondrites

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