Multiple nitrogen isotopic components coexisting in ureilites

被引:31
|
作者
Yamamoto, T [1 ]
Hashizume, K [1 ]
Matsuda, J [1 ]
Kase, T [1 ]
机构
[1] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
来源
METEORITICS & PLANETARY SCIENCE | 1998年 / 33卷 / 04期
关键词
D O I
10.1111/j.1945-5100.1998.tb01692.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
Nitrogen and noble gas isotopic compositions and C abundance of ureilites were analyzed using a stepwise combustion technique. Four Antarctic ureilites, ALHA77257, Asuka 881931, Yamato 791538 and Yamato 790981 were analyzed. Multiple N isotopic components were observed in these ureilites. The delta(15)N values of these N components ranged from +160 to -120 parts per thousand. The minimum delta(15)N values of typically -120 parts per thousand were observed at combustion temperatures at 700-900 degrees C where large amounts of C were released. A heavy N component was observed in only two ureilites, ALHA77257 and Asuka 881931. Silicate-enriched fractions and C-concentrated fractions were prepared for these two ureilites. We conclude that both the light N and the heavy N are trapped in the carbonaceous vein minerals. The lack of correlation between the NIC ratio and the Ar-36/C ratio suggests that the primary carrier phase of the light N does not correspond to that of the planetary noble gases. We consider that the isotopically heavy N, which was observed in this study, is related to the heavy N observed among polymict ureilites. Small amounts (<0.5 ppm) of light N with the minimum delta(15)N value of-120 parts per thousand were observed among the silicate fractions at the highest combustion temperature of 1200 degrees C, although the exact carrier phase of this light N is not known. We consider that the currently observed ureilites were produced by injection of several volatile-rich objects into volatile-poor ureilitic silicates.
引用
收藏
页码:857 / 870
页数:14
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