Other
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28r.360h&link_type=abstract
Meteoritics, vol. 28, no. 3, volume 28, page 360
Other
Graphite Inclusion, Iab Iron Meteorite, Isotopes, Nitrogen
Scientific paper
Introduction: Iron meteorites are considered to have experienced a complex history, which is indicated by the variations in trace element chemistry (e.g., [1]). Among iron meteorite groups, the so called nonmagmatic groups, such as IAB, IIE, and IIICD, may have passed through different formation paths compared to others. Nitrogen isotopes can be a useful tool to understand the origin and formation processes of iron meteorites. Nikogen isotopes in a number of iron meteorites are measured [2,3], although trapping sites of nitrogen in iron meteorites are not yet clear. This is an important issue because nitrogen, a typical mobile element, may well reflect thermal history of their parent bodies (c.f., [4]). Generally, a major portion of nitrogen in iron meteorites is expected to be in a solid solution in Fe-Ni, especially in f.c.c. Fe-Ni (taenite). Franchi et al. [3] report that at least 25 to 35% of nitrogen in magmatic iron meteorites is in acid insoluble phases, however, not in those of non-magmatic meteorites. This result contradicts with the result [5] who report that a significant portion of nitrogen seems to be trapped in acid residues not only of magmatic meteorites but also of non- magmatic meteorites. To resolve the contradiction described above, and to identify the trapping site, we started measuring nitrogen isotopes in acid residues of iron metcorites. We report here preliminary results on acid residues of Canyon Diablo (IA). Procedures: Acid residues were prepared by Dr. J.-I. Matsuda and his colleagues. Different blocks of Canyon Diablo, "Can-1" and "Can-2" were treated by 14M HCl, 10M-HF + 1M-HCl, 1M-HCl, and by aqua regia, which destroyed Fe-Ni, sulfides, silicates, and shreibersite. Acid residues of these two blocks, "Can-1bn" and "Can-2b," yielded 0.102 wt% and 0.299 wt% of their original masses, respectively These residues seem to consist mostly of graphite No diamond was detected by powder X-ray analysis [6]. Preliminary Results: A predominant portion of nitrogen is released at 500 degrees C and 600 degrees C temperature fractions. Total nitrogen amounts and average delta^l5N values of the two acid residues are described in Table 1. Discussion and Summary: Sample "Can-1bn" is 3-4 times concentrated in nitrogen than "Call-2b," although its delta^15N value is within terrestrial range (0 < delta^15N < +20 per mil). Presently, we cannot deny the possibility that nitrogen in "Can-1bn" is dominated by terrestrial nitrogen, which may have been acquired during the acid treatment. Nevertheless, nitrogen isotope data of "Can-2b" suggests that indigenous nitrogen is indeed concentrated in the acid residue of Canyon Diablo. Bulk nitrogen isotope data of Canyon Diablo is reported to be delta^15N= -61.8 +- 10.4 per mil, N= 38.0 +- 155 ppm [2]. Therefore, delta^15N values of "Can-2b" can be resulted by a mixing of indigenous nitrogen and contaminating nitrogen. However, distinct delta^15N values of these two samples may indicate, in turn, that nitrogen isotopes in inclusions of Canyon Diablo are truly heterogeneous because carbon isotopes of graphite inclusions in IA iron meteorites seem to be heterogeneous [7]. Acknowledgments: We thank Dr. J.-I. Matsuda of Osaka University for providing samples and information on these samples. References: [1] Scott E. R. D. and Wasson J. T. (1975) Rev. Geophys. Space Sci., 13, 527-546. [2] Prombo C. A. and Clayton R. N. (1983) Meteoritics, 18, 377-379. [3] Franchi I. A. et al. (1988) Meteoritics, 22, 379-380. [4] Hashizume K. (1993) Doctor Thesis. [5] Murty S. V. S. et al. (1983) GCA, 47, 1061-1068. [6] Ogata Y. et al. (1990) In Abstract of the 1990 Annual Meeting of the Geochemical Society of Japan, 57. [7] Deines P. and Wickman F. E. (1973) GCA, 37, 1295-1319. Table 1 appears here in the hard copy.
Hashizume K.
Sugiura Norimasa
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