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Mineralogy and petrology of the angrite Northwest Africa 1296
被引:42
|作者:
Jambon, A
Barrat, JA
Boudouma, O
Fonteilles, M
Badia, D
Göpel, C
Bohn, M
机构:
[1] Univ Paris 06, Lab Magie, UMR 7047, CNRS, F-75252 Paris, France
[2] CNRS, UMR 6538, IUEM, UBO, F-29280 Plouzane, France
[3] Univ Paris 06, UFR Sci Terre, Serv MEB, F-75252 Paris, France
[4] CNRS, UMR 7579, Inst Phys Globe, Lab Geochim & Cosmochime, F-75252 Paris, France
[5] IFREMER, Ctr Brest, CNRS, UMR 6538, F-29280 Plouzane, France
关键词:
D O I:
10.1111/j.1945-5100.2005.tb00388.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:
We report on a new angrite, Northwest Africa (NWA) 1296, a fine-grained rock with a magmatic texture of rapid cooling. Dendritic olivine (approximate to Fo50) crystallized first in association with anorthite microcrysts (An(98-100)) forming composite chains separated from one another by intergrown Al-Fe diopside-hedenbergite pyroxenes. In addition, some olivines with lower Mg# and increased CaO (up to 12%) are found between the chains as equant microphenocrysts. Pyroxenes and olivines are both normally zoned from Mg# = 0.52 to less than 0.01 in the rims. Ca-rich olivines are surrounded by, intergrown with, or replaced by subcalcic kirschsteinite. They appear after plagioclase crystallization stopped, at the end of the crystallization sequence. Minor phases are pyrrhotite, Fapatite, and titanomagnetite. Pyroxene is the last silicate phase to grow, interstitial to idiomorphic olivine-kirschsteinite. Numerous small vesicles and some channels are filled with microcristalline carbonate. The mode (vol%) is about 28% olivine, 3% kirschsteinite, 32% anorthite, 34% pyroxene, and 3% of the minor phases-close to that reported previously for D'Orbigny and Sahara (SAH) 99555. The bulk chemical composition of NWA 1296 is similar to D'Orbigny and SAH 99555; NWA1296 differs by its texture and mineralogy, which are interpreted as resulting from rapid crystallization-an evidence of impact melting. Angrites cannot be produced by partial melting of a CV source because segregation of a "planetary" core is necessary to explain the low FeO/MgO ratio of magnesian olivines. Neither the odd Ca/Al ratio nor the very low SiO2 content can be explained by conventional partial melting scenarios. We suggest that carbonate is the key to angrite genesis. This is supported by the striking similarities with terrestrial melilititeS (low SiO2, superchondritic Ca/Al ratio, presence of carbonate). The lack of alkalies could be the result of either loss after impact melting or absence of alkalies in the source.
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页码:361 / 375
页数:15
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