Petrology and chemistry of the basaltic shergottite North West Africa 480

被引:73
作者
Barrat, JA
Gillet, P
Sautter, V
Jambon, A
Javoy, M
Göpel, C
Lesourd, M
Keller, F
Petit, E
机构
[1] CNRS, UMR 6112, F-49045 Angers, France
[2] Univ Angers, Fac Sci, F-49045 Angers, France
[3] Ecole Normale Super Lyon, Lab Sci Terre, CNRS, UMR 5570, F-69364 Lyon, France
[4] Museum Natl Hist Nat, Lab Mineral, F-75005 Paris, France
[5] Univ Paris 06, CNRS, UMR 7047, Lab Magie, F-75252 Paris 05, France
[6] Inst Phys Globe, CNRS, UMR 5047, Lab Geochim & Isotopes Stables, F-75252 Paris 05, France
[7] Inst Phys Globe, CNRS, UMR 7579, Lab Geochim & Isotopes Stables, F-75252 Paris 05, France
[8] Univ Angers, UFR Med, SCIAM, Histol Lab, F-49045 Angers, France
[9] UJF, CNRS, UMR 5025, Maison Geosci, F-38400 St Martin Dheres, France
关键词
D O I
10.1111/j.1945-5100.2002.tb00835.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
North West Africa (NWA) 480 is a new martian meteorite of 28 g found in the Moroccan Sahara in November 2000. It consists mainly of large gray pyroxene crystals (the largest grains are up to 5 mm in length) and plagioclase converted to maskelynite. Excluding the melt pocket areas, modal analyses indicate the following mineral proportions: 72 vol% pyroxenes extensively zoned, 25% maskelynite, 1% phosphates (merrillite and chlorapatite), 1% opaque oxides (ilmenite, ulvospinel and chromite) and sulfides, and 1% others such as silica and fayalite. The compositional trend of NWA 480 pyroxenes is similar to that of Queen Alexandra Range (QUE) 94201 but in NWA 480 the pyroxene cores are more Mg-rich (En(77)-En(65)). Maskelynites display a limited zoning (An(42-50)Ab(54-48)Or(2-4)). Our observations suggest that NWA 480 formed from a melt with a low nuclei density at a slow cooling rate. The texture was achieved via a single-stage cooling where pyroxenes grew continuously. A similar model was previously proposed for QUE 94201 by McSween et al. (1996). NWA 480 is an Al-poor ferroan basaltic rock and resembles Zagami or Shergotty for major elements and compatible trace element abundances. The bulk rock analysis for oxygen isotopes yields Delta(17)O = +0.42parts per thousand, a value in agreement at the high margin, with those measured on other shergottites (Clayton and Mayeda, 1996; Romanek et al., 1998; Franchi et al., 1999). Its CI-normalized rare earth element pattern is similar to those of peridotitic shergottites such as Allan Hills (ALH)A77005, suggesting that these shergottites shared a similar parent liquid, or at least the same mantle source.
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收藏
页码:487 / 499
页数:13
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