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Petrology and Oxygen Isotopic Compositions of Anomalous Achondrite NWA 011

Prinya Promprated, L. A. Taylor, M. Anand, D. Rumble, E. V. Korochantseva, M. A. Ivanova, C. A. Lorentz, М. А. Назаров

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Abstract

Introduction: Northwest Africa (NWA) 011 is a single stone of 40 g and has been discovered in the Moroccan Sahara desert in 1999 [1]. This pyroxeneplagioclase meteorite was classified as noncumulate eucrite, on the basis of petrography and geochemistry [1]. However, certain characteristics of this meteorite such as the high Fe/Mn values in pyroxene (~65) and particularly the bulk-rock oxygen isotopic compositions (δO = +2.54, δO = -0.48) are not of typical eucrites and may suggest a new type of basaltic meteorite [2]. In an attempt to resolve this issue, we have investigated mineral chemistry and oxygen isotopic compositions on portions of NWA 011. Trace-element chemistry and Ar-Ar age is presented in a companion paper [3]. Petrographic Description: Petrographic study of 2 polished thin-sections reveals that the sample is finegrained monolithic, unbrecciated achondrite [1]. The absence of primary breccia texture (i.e., relic plagioclase and augite grains [2]), even in our larger section (3 cm), suggests that NWA 011 may not be a recrystallized breccia. Modally, the sample consists mainly of pigeonite (58.50%) and plagioclase (39.56%), with minor amounts of opaque (0.71%), silica (0.67), and phosphate (0.54) minerals. Pigeonite (0.2-0.8 mm) is commonly subhedral and often has curve boundaries at the contacts with plagioclase (Fig. 1). All pigeonite grains contain exsolution lamellae of augite, usually a few microns wide but sometimes reach ~10 μm. Plagioclase (up to 0.1 mm) is anhedral and usually forms crystal aggregates (up to 2 mm) or straddles along grain boundaries or fractures of pigeonite grains. This texture may indicate recrystallization, possibly as a result of thermal metamorphism. Opaque minerals, occurring as small clusters, include ulvospinel, ilmenite, and small Fe metal-sulfide intergrowths (2-5 μm). Baddeleyite inclusions have also been found in some ilmenties. Olivine usually occurs in the same aggregates as oxides (Fig. 1). Ca-phosphates (whitlockite and Clapatite) are common but not evenly distributed. Mineral Chemistry: Compositions of pigeonite (Wo5.7-6.5 Fs63.2-65.1; Mg# = 32-33) and its lamella augite (Wo36.1-39.2 Fs35.2-38.3 ; Mg# = 38-43) are similar to those of Nuevo Laredo Trend eucrites (Fig. 2) [4] and some lunar metabasalts [5]. However, the Fe/Mn ratios (Pig = 67, Aug = 65) are significantly higher than those of typical eucrites (Fig. 3). Plagioclase is bytownite and low in K2O contents (An80.2-87.7Or0.7-0.2). Olivine is Ferich and its composition varies in a restricted range (Fa79.5-81.4). In ulvospinel, FeO and TiO2 contents are 55.3 and 24.2 wt%, resp.; ilmenite contains 45.1 and 52.7 wt%, resp.

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Introduction: Northwest Africa (NWA) 011 is a single stone of 40 g and has been discovered in the Moroccan Sahara desert in 1999 [1]. This pyroxeneplagioclase meteorite was classified as noncumulate eucrite, on the basis of petrography and geochemistry [1]. However, certain characteristics of this meteorite such as the high Fe/Mn values in pyroxene (~65) and particularly the bulk-rock oxygen isotopic compositions (δO = +2.54, δO = -0.48) are not of typical eucrites and may suggest a new type of basaltic meteorite [2]. In an attempt to resolve this issue, we have investigated mineral chemistry and oxygen isotopic compositions on portions of NWA 011. Trace-element chemistry and Ar-Ar age is presented in a companion paper [3]. Petrographic Description: Petrographic study of 2 polished thin-sections reveals that the sample is finegrained monolithic, unbrecciated achondrite [1]. The absence of primary breccia texture (i.e., relic plagioclase and augite grains [2]), even in our larger section (3 cm), suggests that NWA 011 may not be a recrystallized breccia. Modally, the sample consists mainly of pigeonite (58.50%) and plagioclase (39.56%), with minor amounts of opaque (0.71%), silica (0.67), and phosphate (0.54) minerals. Pigeonite (0.2-0.8 mm) is commonly subhedral and often has curve boundaries at the contacts with plagioclase (Fig. 1). All pigeonite grains contain exsolution lamellae of augite, usually a few microns wide but sometimes reach ~10 μm. Plagioclase (up to 0.1 mm) is anhedral and usually forms crystal aggregates (up to 2 mm) or straddles along grain boundaries or fractures of pigeonite grains. This texture may indicate recrystallization, possibly as a result of thermal metamorphism. Opaque minerals, occurring as small clusters, include ulvospinel, ilmenite, and small Fe metal-sulfide intergrowths (2-5 μm). Baddeleyite inclusions have also been found in some ilmenties. Olivine usually occurs in the same aggregates as oxides (Fig. 1). Ca-phosphates (whitlockite and Clapatite) are common but not evenly distributed. Mineral Chemistry: Compositions of pigeonite (Wo5.7-6.5 Fs63.2-65.1; Mg# = 32-33) and its lamella augite (Wo36.1-39.2 Fs35.2-38.3 ; Mg# = 38-43) are similar to those of Nuevo Laredo Trend eucrites (Fig. 2) [4] and some lunar metabasalts [5]. However, the Fe/Mn ratios (Pig = 67, Aug = 65) are significantly higher than those of typical eucrites (Fig. 3). Plagioclase is bytownite and low in K2O contents (An80.2-87.7Or0.7-0.2). Olivine is Ferich and its composition varies in a restricted range (Fa79.5-81.4). In ulvospinel, FeO and TiO2 contents are 55.3 and 24.2 wt%, resp.; ilmenite contains 45.1 and 52.7 wt%, resp.

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Available abstract

Introduction: Northwest Africa (NWA) 011 is a single stone of 40 g and has been discovered in the Moroccan Sahara desert in 1999 [1]. This pyroxeneplagioclase meteorite was classified as noncumulate eucrite, on the basis of petrography and geochemistry [1]. However, certain characteristics of this meteorite such as the high Fe/Mn values in pyroxene (~65) and particularly the bulk-rock oxygen isotopic compositions (δO = +2.54, δO = -0.48) are not of typical eucrites and may suggest a new type of basaltic meteorite [2]. In an attempt to resolve this issue, we have investigated mineral chemistry and oxygen isotopic compositions on portions of NWA 011. Trace-element chemistry and Ar-Ar age is presented in a companion paper [3]. Petrographic Description: Petrographic study of 2 polished thin-sections reveals that the sample is finegrained monolithic, unbrecciated achondrite [1]. The absence of primary breccia texture (i.e., relic plagioclase and augite grains [2]), even in our larger section (3 cm), suggests that NWA 011 may not be a recrystallized breccia. Modally, the sample consists mainly of pigeonite (58.50%) and plagioclase (39.56%), with minor amounts of opaque (0.71%), silica (0.67), and phosphate (0.54) minerals. Pigeonite (0.2-0.8 mm) is commonly subhedral and often has curve boundaries at the contacts with plagioclase (Fig. 1). All pigeonite grains contain exsolution lamellae of augite, usually a few microns wide but sometimes reach ~10 μm. Plagioclase (up to 0.1 mm) is anhedral and usually forms crystal aggregates (up to 2 mm) or straddles along grain boundaries or fractures of pigeonite grains. This texture may indicate recrystallization, possibly as a result of thermal metamorphism. Opaque minerals, occurring as small clusters, include ulvospinel, ilmenite, and small Fe metal-sulfide intergrowths (2-5 μm). Baddeleyite inclusions have also been found in some ilmenties. Olivine usually occurs in the same aggregates as oxides (Fig. 1). Ca-phosphates (whitlockite and Clapatite) are common but not evenly distributed. Mineral Chemistry: Compositions of pigeonite (Wo5.7-6.5 Fs63.2-65.1; Mg# = 32-33) and its lamella augite (Wo36.1-39.2 Fs35.2-38.3 ; Mg# = 38-43) are similar to those of Nuevo Laredo Trend eucrites (Fig. 2) [4] and some lunar metabasalts [5]. However, the Fe/Mn ratios (Pig = 67, Aug = 65) are significantly higher than those of typical eucrites (Fig. 3). Plagioclase is bytownite and low in K2O contents (An80.2-87.7Or0.7-0.2). Olivine is Ferich and its composition varies in a restricted range (Fa79.5-81.4). In ulvospinel, FeO and TiO2 contents are 55.3 and 24.2 wt%, resp.; ilmenite contains 45.1 and 52.7 wt%, resp.

Key concepts: Pigeonite, Achondrite, Augite, Plagioclase, Geology, Meteorite, Geochemistry, Petrography

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