Meteoritics & Planetary Science 42, Nr 9, 1647–1694 (2007) Abstract available online at http://meteoritics.org

The Meteoritical Bulletin, No. 92, 2007 September

Harold C. CONNOLLY, JR.1, 2, 3*, Caroline SMITH4, Gretchen BENEDIX4, Luigi FOLCO5, Kevin RIGHTER6, Jutta ZIPFEL7, Akira YAMAGUCHI8, and Hasnaa CHENNAOUI AOUDJEHANE9

1Department of Physical Science, Kingsborough Community College and the Graduate School of the City University of New York, 2001 Oriental Boulevard, Brooklyn, New York 11235, USA 2Department of Earth and Planetary Science, American Museum of Natural History, Central Park West, New York, New York 10024, USA 3Lunar and Planetary Laboratory, Department of Planetary Sciences, The University of Arizona, Tucson, Arizona 85721, USA 4Department of Mineralogy, The Natural History Museum, Cromwell Road, London SW7 5BD, UK 5Museo Nazionale Antartide, Via Laterina 8, I-53100 Siena, Italy 6Code ST, NASA Johnson Space Center, Houston, Texas 77058, USA 7Sektion Meteoritenforschung, Forschungsinstitut und Naturmuseum Senckenberg, Senckenberganlage 25, D-60325, Frankfurt am Main, Germany 8Antarctic Meteorite Research Center, National Institute of Polar Research, 1-9-10 Kaga, Itabashi, Tokyo 173-8515, Japan 9Université Hassan II Casablanca, Faculté des sciences, Département de Géologie, BP 5366, Mâarif, Casablanca, Morocco * Corresponding author. E-mail: [email protected] (Received 04 September 2007)

Abstract–In this edition of The Meteoritical Bulletin, 1394 recognized meteorites are reported, 27 from specific locations within Africa, 133 from Northwest Africa, 1227 from Antarctica (from ANSMET, PNRA, and PRIC expeditions), and 7 from Asia. The Meteoritical Bulletin announces the approval of four new names series by the Nomenclature Committee of the Meteoritical Society, two from Africa and one from Asia, including Al Haggounia, from Al Haggounia, Morocco, which is projected to be on the order of 3 metric tons of material related to enstatite chondrites and aubrites. Approved are two falls from Africa, Bassikounou (Mauritania) and Gashua (Nigeria). Approved from areas other than Antarctica are one lunar, two Martian, 32 other achondrites, three mesosiderites, two pallasites, one CM, two CK, one CR2, two CV3, one CR2, and four R chondrites. The Nomenclature Committee of the Meteoritical Society announces 48 newly approved relict meteorites from two new name series, Österplana and Gullhögen (both from Sweden).

AFRICA larger lithic clasts (up to 0.3 mm) and vesicular glassy matrix and veins. Minerals identified include pyroxene, Libya plagioclase, olivine, ilmenite, kamacite, and troilite. Lithic clasts include gabbro (composed of plagioclase and Dar al Gani 1048 27°12.10′N, 16°18.67′E pigeonite) and very fine grained, ophitic-textured basalt Libya (composed of plagioclase and olivine with accessory Find: June 28, 2001 orthopyroxene, troilite, metal, and rutile). Several glassy Achondrite (lunar, feldspathic breccia) spheres were found. History: A tiny complete individual stone was recovered by Geochemistry: Olivine (Fa19.6–49.6, FeO/MnO = 93–98), an anonymous finder in June 2001 and purchased by pigeonite (Fs20.2–61.9Wo5.3–7.2, FeO/MnO = 54.8–66.5), and N. Classen in 2003 in Vienna, Austria. plagioclase (An97–98Or0). Physical characteristics: A single 0.801 g medium gray Classification: Achondrite (lunar, feldspathic breccia). This stone with some diffuse whitish clasts. About 70% of the stone is likely paired with Dar al Gani 262 and Dar al Gani stone is covered by fusion crust. 996. Petrography: (A. Irving and S. Kuehner, UWS) Type specimens: A total of 0.33 g of sample is on deposit at Predominantly very fine-grained mineral debris with some UWS. Classen holds the main mass.

1647 © The Meteoritical Society, 2007. Printed in USA. 1648 H. C. Connolly, Jr., et al.

Mauritania samples potentially from this area varies, ranging from EL3 chondrite to aubrite. Bassikounou 15°47′N, 5°54′W Bassikounou, Hodh Ech Chargui, Mauritania Al Haggounia 001 27°30′N, 12°30′W Fall: 16 October 2006, 04:00 UTC Al Haggounia, Morocco Ordinary chondrite (H5) Find: 2006 History: A fireball was witnessed in the area, but no records Achondrite (aubrite) of the direction of movement were recorded. A single stone of History: Several tons of this material have been found on 3165 g was found by A. Salem El Moichine, a local resident, the ground or by digging near Al Haggounia, Morocco on the same day at 13:00 h local time, 11 km SE of (see Chennaoui et al. 2007 for description of the strewn Bassikounou. The sample for classification was provided to field), and sold to several dealers. The coordinates are NMBE by M. Ould Mounir, Nouakchott, who obtained it given for the center of the strewn field, which extends from his cousin who recovered the meteorite. According to ~40 km. S. Buhl (Hamburg, Germany), more than 20 specimens were Physical characteristics: It is impossible to precisely later recovered by locals and meteorite finders. These finds assess the amount of material already (and to be) define an 8 km long strewn field. The total recovered mass is recovered, but according to dealers, collectors, and Jambon, 46.00 kg. it is about 3 metric tons composing many samples of varied Physical characteristics: The 3165 g specimen is largely sizes (from a few g to 50 kg). The largest stones were covered by black fusion crust. The interior is light gray. On recovered after excavating them from the ground. The outer the surface of the fusion crust there is some adherent soil surface is rusty brown due to severe alteration and looks material, some of which is bright red. Shortly after recovery, like a sedimentary breccia cemented by iron oxide and the stone was cut into two pieces of 1200 and 1950 g. The carbonate. Color changes from bluish gray to rusty brown larger piece has a rectangular shape and shows indications of closest to the fractures are observed. Yellow patches of flow lines in the fusion crust. sulfur (alteration) are widespread. The rocks are Petrography: (E. Gnos, MHNGE; B. Hofmann, NMBE, significantly porous, with pore sizes from several M. Eggimann, Bern/NMBE): Mean chondrule size centimeters to hundreds of microns. 0.35 mm (n = 53). Metal abundance is 8 vol%, troilite Petrography: (A. Jambon, O. Boudouma, and D. Badia. 6.6 vol%. Mean plagioclase grain size is ~20 μm. Troilite UPVI) Dominated by enstatite and plagioclase. Troilite, is polycrystalline, rich in silicate inclusions, and shows graphite daubreelite, oldhamite, kamacite rich in Si, and diffuse boundaries to metal. Metal is partly rich in schreibersite are present. μ silicate and troilite inclusions. Rare metallic Cu (10 m) Mineral compositions: Enstatite (En98Fs1Wo1) and occurs at kamacite-taenite boundaries and in troilite. plagioclase (Ab78An16Or5). Some shock veins and no weathering products were Classification: Achondrite (aubrite); extensive weathering. observed. Similar to and likely paired with NWA 002, 1067, 2736, 2828, Mineral compositions: Olivine (Fa18.6), pyroxene (Fs16.3 2965. Wo1.1), and plagioclase (An13.7). Type specimens: A total of 50 g of sample and three polished Cosmogenic radionuclides: (P. Weber, PPGUN) Gamma- sections are on deposit at UPVI. spectroscopy performed in December 2006 and January 2007 Main masses: Beroud, 3886 g (26 pieces from 1185 g to showed the presence of the following radionuclides: 48V, 46Sc, 5.8 g); P. Thomas, 4497 g (33 pieces from 11 to 1507 g); 56Co, 54Mn, 58Co, 7Be, 51Cr, 57Co, 22Na, 26Al, and 60Co. Hmani, about 500 kg; Ouzrou, about 500 kg. Recalculated to 12 October 2006 22Na was 38.0 ± 2.2 and 26Al 31.5 ± 2.1 (both dpm/kg), the activity ratio of 1.21 is The Meteoritical Bulletin announces a new name series fully consistent with a fall on that date. approved by the Nomenclature Committee of the Classification: Ordinary chondrite (H5); S2, W0. Meteoritical Society, Istifane, located in the Istifane region of Type specimens: A total of 115 g are on deposit at NMBE. Morocco. Boudreaux holds the main mass. Istifane 001 31°29.911′N, 5°43.045′W Morocco Morocco Find: 24 July 2005 The Meteoritical Bulletin announces a new name series Ordinary chondrite (H4) approved by the Nomenclature Committee of the Meteoritical Physical characteristics: It consists of three separate pieces Society from a dense collection area near Al Haggounia, of 68.0, 51.8, and 11.8 g, with a total mass of 131.6 g. The Morocco (Chennaoui et al. 2007), comprising approximately three pieces fit together documenting that they are fragments 3 tons of material. It should be noted that the classification of of a single stone. The Meteoritical Bulletin, No. 92 1649

Petrography: (A. Ibhi and H. Nachit IZU, H. Chennaoui Nigeria Aoudjehane UHAC) It is severely weathered with a dark orange-brown color. Metallic Fe-Ni and/or troilite grains are Gashua 12°51′N, 11°02′E frequently replaced by iron oxide. Plagioclase grains are up to Dapchi, Nigeria 100 μm in size. Fall: April 1984 Mineral compositions: Olivine (Fa18.4–19.2), orthopyroxene Ordinary chondrite (L6) (Fs16.2–17.5). History: The meteorite fall was reported by anonymous Classification: Ordinary chondrite (H4); S3, W4. eyewitnesses to have occurred around April 1984 (about the Type specimens: Three polished thin sections and three time of the nearby Gujba fall) near the tiny desert settlement fragments totalling 104 g are on deposit at IZU. Kolomari close to the town of Gashua, Dapchi district, Nigeria. Istifane 002 31°29.909′N, 5°43.044′W Physical characteristics: A single stone of 4162 g was Morocco recovered and broken by villagers into many pieces at the Find: 17 August 2005 place of the fall. The pieces were stored by villagers until they Ordinary chondrite (H5) were collected in 2005 and sent to E. Twelker. Physical characteristics: One 40 g stone, brownish in color. Petrography: (A. Greshake, NHB) The meteorite is a weakly Mineral compositions: (A. Ibhi and H. Nachit IZU, weathered ordinary chondrite with recrystallized texture and H. Chennaoui Aoudjehane UHAC) Olivine (Fa15.5±0.5) and few poorly defined chondrules. Opaque and often low-Ca pyroxene (Fs16.8±0.6). interconnecting shock veins are present. Classification: Ordinary chondrite (H5); S5, W3. Mineral compositions: Olivine (Fa23.8) and pyroxene (Fs20). Type specimens: One thin section and the main mass are on Classification: Ordinary chondrite (L6); S4, W1. deposit at IZU. Type specimens: A total of 40.4 g plus one polished thin section are on deposit at MNB. Twelker holds the main mass. Istifane 003 31°29.150′N, 5°43.027′W Morocco A list of all meteorites recognized from countries and regions Find: 17 August 2005 in Africa other than the northeast and the northwest is Ordinary chondrite (L5) provided in Table 1. Physical characteristics: It is an 18.5 g stone partly covered by dark-brown fusion crust. Northwest Africa Mineral compositions: (A. Ibhi and H. Nachit IZU, H. Chennaoui Aoudjehane UHAC) Olivine (Fa24.9±0.7), Northwest Africa 801 orthopyroxene (Fs21.4±0.6), feldspar (An11Or6), high-Ca Morocco pyroxene (Fs10.6Wo41). Find: 2001 Classification: Ordinary chondrite (L5); S3, W2. Carbonaceous chondrite (CR2) Type specimens: Three thin sections and three fragments History: M. Farmer and G. Hupé recovered a total of totaling 10.4 g are on deposit at IZU. approximately 5 kg of many individuals and fragments from Zagora, Morocco. Many whole and sliced specimens Istifane 004 31°30.165′N, 5°42.916′W have been sold over the last several years. Morocco Physical characteristics: Many whole stones and fragments, Find: 19 May 2006 all with desert varnish and brown/orange color. Numerous Ordinary chondrite (H5) chondrules, many on the order of ~1 mm in apparent History: A. Ibhi and M. El Mansouri found this meteorite diameter, are visible. while prospecting with a metal detector. Petrography: (G. Benedix and C. Smith, NHM) The thin Physical characteristics: It is a 10.8 g stone. section studied is dominated by millimeter-sized type I PO Petrography: (A. Ibhi and H. Nachit IZU, H. and POP chondrules, which are often rimmed with and/or Chennaoui Aoudjehane UHAC) The meteorite is contain metallic Fe-Ni blebs. Metallic Fe-Ni also occurs as dominated by olivine and low-Ca pyroxene. Plagioclase, rounded, millimeter-sized grains within the matrix. Interstitial troilite, and metallic Fe-Ni are also noted as major and to chondrules and metal is a fine-grained matrix rich in minor minerals. phyllosilicate. Two type II chondrules were also observed. Mineral compositions: Olivine (Fa19.1±0.5), low-Ca pyroxene Pervasive veins of rust occur throughout. (Fs15.4±0.9), feldspar (An2.5±0.3). Mineral compositions: Type 1 chondrule olivine (Fo98.2±1.3), Classification: Ordinary chondrite (H5); S2, W2. low-Ca pyroxene (En96.2±0.9Wo2.0±2.2), and high-Ca pyroxene Type specimens: One thin section and the main mass are on (En45.7±11.5Wo35.9±4.7). Type II chondrule olivine (Fo77.4±7.7) deposit at IZU. and low-Ca pyroxene (En73.8±1.8Wo2.1±2.4). 1650 H. C. Connolly, Jr., et al.

Classification: Carbonaceous chondrite (CR2); moderate to Northwest Africa 2044 extensive weathering. Morocco or Algeria Type specimens: A total of 77.4 g of sample and two Find: August 2003 sections are on deposit at NHM. Farmer holds several Carbonaceous chondrite (CV3) grams, KCCU holds approximately 10 g, and AMNH holds History: Purchased in 2003 August in Erfoud, Morocco, for several grams. D. Gregory. Physical characteristics: A single stone weighing 661 g. Northwest Africa 1461 Petrography: (A. Irving and S. Kuehner, UWS) Sparse, well- Algeria or Morocco formed ovoid chondrules in a black matrix. Olivine, Find: March 2002 orthopyroxene, clinopyroxene with accessory troilite and Achondrite (diogenite) metal. Sparse CAI consisting mainly of Mg-Al spinel, History: D. Gregory purchased the 252 g stone in Erfoud, gehlenite and perovskite, with rims of Al-Ti-rich Morocco, in March 2002. clinopyroxene. Veins of anorthite present. Physical characteristics: A single pale gray-green, broken Geochemistry: Mafic silicates are very Mg-rich (mg > stone. 97), metal (5 wt% Ni). Oxygen isotopes: (D. Rumble, Petrography: (A. Irving and S. Kuehner, UWS): Coarse- CIW) Analyses of two whole rock fragments by laser grained (clasts up to 7 mm) with a partly cataclastic texture. fluorination gave δ18O = −1.12, −2.71; δ17O = −4.45, Predominantly orthopyroxene (with diffuse grain boundaries) −6.36; Δ17O = −3.860, −4.934 (all ‰). and accessory chromite. Minor calcite is present along some Classification: Carbonaceous chondrite (CV3); S1, minimal grain boundaries. weathering. Mineral compositions and geochemistry: Orthopyroxene Specimens: A total of 22.4 g of sample and one polished thin (Fs13.5–13.7Wo0.7–0.9; FeO/MnO = 32.0–33.8). This specimen is section are on deposit at UWS. Gregory holds the main mass. distinctive in the magnesian pyroxene it exhibits. Oxygen isotopes: (D. Rumble, CIW) Replicate analyses by laser Northwest Africa 3157 fluorination yielded δ18O = 3.177, 3.584; δ17O = 1.410, 1.634; Morocco or Algeria Δ17O = −0.2609, −0.2505 (all ‰). Find: September 2004 Classification: Achondrite (diogenite). Ordinary chondrite (Type 3) Type specimens: A total of 23 g of sample is on deposit at History: Purchased from a Moroccan dealer at the Denver UCLA. One polished thin section and 1.3 g are on deposit at Mineral Show by A. Hupé in September 2004. UWS. Gregory holds the main mass. Physical characteristics: A single 51.7 g light brown stone lacking fusion crust and with abundant, large chondrules. Northwest Africa 1924 Petrography: (A. Irving and S. Kuehner, UWS) Closely Morocco or Algeria packed PO and POP chondrules (mean diameter 1.0 mm); Find: January 2001 some are ovoid. The matrix is a “lacework” of porous olivine Carbonaceous chondrite (CV3) and pyroxene with accessory kamacite, taenite and troilite. The History: Purchased in January 2001 in Erfoud, Morocco for content of metal (+minor Fe hydroxide) is very low (mode D. Gregory. determined by BSE imaging of a whole thin section is 1 vol%). Physical characteristics: A single stone weighing 255 g. Geochemistry: Olivine (Fa0–60); orthopyroxene Petrography: (A. Irving and S. Kuehner, UWS) Separated (Fs0.5–30Wo1.5). Oxygen isotopes: (D. Rumble, CIW) Analyses olivine-rich chondrules (mostly micro-porphyritic) and of two acid-washed whole rock fragments by laser sparse CAI (containing Al-Ti-rich clinopyroxene, Fe-rich fluorination gave, respectively, δ18O = 5.30, 4.85; δ17O = spinel, and anorthite) in a dark, relatively magnetite-rich 3.48, 3.29; Δ17O = 0.693, 0.742 (all ‰). Although these Δ17O matrix. Olivine, Cr-bearing magnetite, ilmenite, values are within the range for H chondrites, this specimen is intermediate plagioclase, orthopyroxene, clinopyroxene, and poorer in metal than typical H chondrites. pentlandite. Classification: Ordinary chondrite (Type 3); S2, W1/2. Geochemistry: Olivine (Fa29.1), Ti-rich pyroxene Specimens: A total of 10.6 g of sample and one polished thin (Wo70.3Fs0.05) with TiO2 = 16.2, Al2O3 = 17.8 (both wt%). section are on deposit at UWS. G. Hupé holds the main mass. Oxygen isotopes: (D. Rumble, CIW) Laser fluorination analyses of two samples (all ‰) δ18O= −3.01, −3.61; δ17O Northwest Africa 3221 = −6.46, −7.04; Δ17O = −4.879, −5.139. Morocco Classification: Carbonaceous chondrite (CV3); S1, minimal Find: 2002 weathering. Achondrite (ureilite, polymict) Specimens: A total of 20.4 g of sample and one polished thin History: B. Fectay purchased a single stone of 38.5 g in section are on deposit at UWS. Gregory holds the main mass. Rissani, Morocco, in 2002. The Meteoritical Bulletin, No. 92 1651

Physical characteristics: A fragment with 45% fresh black Physical characteristics: The sample is a subrounded stone fusion crust with a typical polymict ureilite texture. with 60% fusion crust and soft when cut. Petrography: (H. Takeda, Chiba and A. Yamaguchi, NIPR). Petrography and mineral compositions: (H. Takeda, Chiba The sample is a fragmental breccia with lithic clasts and and A. Yamaguchi, NIPR). It is composed of medium to subrounded mineral fragments embedded in a cataclastic coarse (up to 1.6 × 1.2 mm in size) olivine (Fo77–80, CaO = matrix of predominantly ureilitic material. One large clast is a 0.3–0.4; Cr2O3 = 0.65–0.9 [both wt%; cores]) and pigeonite fine-grained carbonaceous chondrite 2.3 × 1.5 mm in size and grains (Fs18.0Wo7.5; Cr2O3 = 1.1–1.3 wt%). Carbonaceous another is very heavily shocked ureilite. Mineral fragments veins typical of ureilites are observed at parts of the thin include olivine up to 1.8 × 1.2 mm, pyroxene, Na-rich section and dusty patches of fine-grained opaque minerals plagioclase, rare K, Na-rich glassy grain. decorate the rims of grains. Mineral compositions: Pyroxene (Fs8Wo8-Fs44Wo10- Classification: Achondrite (ureilite, polymict); minimal Fs13Wo34; Cr2O3 of pigeonite = 0.8–1.2 wt%; augite = 1.8 = shock with rare mosaicism in olivine. 2.0 wt%), olivine (Fo74–90; CaO = 0.25–0.47 wt%; Cr2O3 = Type specimen: A total of 9.8 g of sample and one thin 0.42–0.83 wt% [cores]) and plagioclase (An6–60). High K, Na- section are on deposit at NIPR. Fectay hold the main mass. rich glassy materials (SiO2 = 66.5, Al2O3 = 11.3, FeO = 8.5, Na2O = 4.2, K2O = 2.1 [all wt%] observed). Coexistence of Northwest Africa 3340 unshocked olivine and a very heavily shocked ureilite clast Algeria or Morocco 4.4 × 3.2 mm in size (PTS 090,8) as in Dar al Gani 1023 with Find: April 2006 granoblastic texture. Clast olivines (Fo70–78 [cores]). Carbonaceous chondrite (CM2, anomalous) Classification: Achondrite (ureilite, polymict). History: Purchased by F. Kuntz in April 2006 in Erfoud, Type specimen: A total of 7.7 g of sample and a thin section Morocco, and subsequently acquired for the DuPont are on deposit at NIPR. Fectay hold the main mass. Collection at PSF. Physical characteristics: Two pieces from a very fresh, Northwest Africa 3222 broken, black, porous stone (total weight 12.7 g) with shiny Morocco fusion crust on one side. Find: 2000 Petrography: (A. Irving and S. Kuehner, UWS; T. Bunch, Achondrite (ureilite, monomict) NAU) Sparse mineral grains, carbon-rich objects, dust- History: An anonymous finder recovered 79 g. armored chondrules and rare refractory inclusion occur in a Physical characteristics: A flattened individual stone with heterogeneous, very fine grained, porous matrix composed sandblasted crust on 80% of the surface. mainly of bladed phyllosilicates with some pentlandite and Petrography and mineral compositions: (H. Takeda, Chiba calcite (clearly visible under incident UV light). Olivine and A. Yamaguchi, NIPR). The texture shows slightly grains (up to 2 mm across) are commonly armored by fine, rounded angular fragments (up to 2.5 × 1.2 mm) of olivine polycrystalline “dust” and contain inclusions of Ni-rich (Fo87–89 [cores]; Fo92–96[rims]) in a comminuted matrix. troilite, chromite, millerite, kamacite and taenite. Both Small rounded to oval orthopyroxene (Fs11.2Wo4.8) and augite pentlandite and magnesian olivine occur as separate smaller, μ (Fs7Wo37) grains are poikilitically enclosed in olivine angular grains. The carbon-rich objects (up to 50 m across) crystals. Carbonaceous material with iron oxide-hydroxide consist of either pure graphite or a chlorine-rich organic occur as narrower, intergranular veins in a crystalline clast (4 phase. Chondrules consist of PO and POP olivine, many × 4 mm). The olivine grains in this clast show mosaicism with having a fine-grained polycrystalline “dust” rims. One small tilt boundaries, but the olivine fragments in the breccia matrix refractory inclusion is composed of Mg-Al spinel with are not shocked. This meteorite contains mostly olivine with inclusions of perovskite. minor inclusions of orthopyroxene and augite. Many olivine Mineral compositions and geochemistry: Larger zoned fragments in the matrix do not contain carbonaceous veins. olivine grains (e.g., Fa17.9-33.9, Fa39.9–66); smaller Classification: Achondrite (ureilite, monomict); S2, homogeneous olivine grains (e.g. Fa1.5, Fa19.9); pentlandite moderate weathering. (Ni = 26.2 wt%). Matrix phyllosilicate material could not be Type specimen: A total of 15.8 g of sample and one thin analyzed quantitatively, but has very consistent proportions of section are on deposit at NIPR. Fectay hold the main mass. Mg, Fe, Si and S. The chlorine-rich organic phase contains ~17 wt% Cl and ~32 wt% C, but no detectable N and minor Northwest Africa 3223 O. Oxygen isotopes: (D. Rumble, CIW) Replicate analyses by Morocco laser fluorination gave, respectively, δ18O = 0.494, 1.166; Find: 2002 δ17O = 6.224, 7.049; Δ17O = −2.780, −2.542 (all ‰). Achondrite (ureilite, polymict) Classification: Carbonaceous chondrite (CM2, anomalous); History: An anonymous finder recovered a single stone of minimal weathering. The presence of chlorine-rich carbon 51 g. compounds, which may be enigmatic chlorinated 1652 H. C. Connolly, Jr., et al. hydrocarbons, makes this specimen potentially unique among Specimens: A total of 20.1 g of sample, one polished thin CM chondrites. section and a polished mount are on deposit at UWS. GHupé Specimens: A total of 2.7 g of sample is on deposit at UWS holds the main mass. and the remainder of the mass (10 g) is at PSF. Northwest Africa 4232 Northwest Africa 4223 Northwest Africa Algeria Find: December 2005 Find: December 2005 Enstatite chondrite (EL3) Achondrite (diogenite, olivine-bearing) History: G. Hupé purchased the specimens in December 2005 History: G. Hupé purchased the stones in December 2005 in in Tagounite, Morocco. Tagounite, Morocco. Physical characteristics: The meteorite consists of two dark Physical characteristics: The meteorite comprises two brown stones weighing 105 and 19 g. Cut surfaces have dense, dark brown and partly fusion crusted stones with a sparse grains of fresh metal, and there are multiple subparallel total weight of 329 g. and anastomosing thin veinlets filled with iron oxides/ Petrography: (A. Irving and S. Kuehner, UWS) The hydroxides and some calcite from terrestrial weathering. meteorite is coarse-grained (≤4 mm) with a primarily Petrography: (A. Irving and S. Kuehner, UWS) protogranular texture, and some areas of cataclasis. Olivine Predominantly granular texture with mostly equant and some (50 vol%) and orthopyroxene (45 vol%) are the dominant bladed grains (0.5 to 1.5 mm). Composed mainly of pure minerals with accessory chromite, troilite and metal enstatite with subordinate altered kamacite, altered troilite, (kamacite). Some veinlets of terrestrial calcite crosscut the plagioclase and accessory schreibersite and daubreelite (as specimen. blades in altered troilite). Sparse RP chondrules (0.2–0.8 mm Mineral compositions and geochemistry: Olivine in diameter) composed of radiating (and some subparallel) (Fa30.0–31.2; FeO/MnO = 44.8–48.2), orthopyroxene enstatite grain clusters. (Fs24.2–25.2Wo2.8–3.2; FeO/MnO = 28.8), chromite (Cr/[Cr + Mineral compositions: Enstatite (En97.9–98.4Wo1.3–1.4) and Al] = 0.703–0.715; Fe/[Fe+Mg] = 0.69–0.73, mean TiO2 = plagioclase (An15.2–16.0Or4.3–4.4). 1.02 wt%). Oxygen isotopes: (D. Rumble, CIW) Analyses of Classification: Enstatite chondrite (EL3); S1, W4/5. This two aliquots by laser fluorination gave, respectively, δ18O = specimen is similar to NWA 002, NWA 1067, NWA 2736, 3.08, 3.22; δ17O = 1.44, 1.48; Δ17O = −0.180, −0.214 (all ‰). NWA 2965, and NWA 4295. It may also be related to Al Classification: Achondrite (diogenite, olivine-bearing). Haggounia 001. Type specimens: A total of 20.4 g of sample, one polished Specimens: A total of 20 g of sample and one polished thin thin section and a polished mount are on deposit at UWS. section are on deposit at UWS. GHupé holds the main mass. GHupé holds the main mass. Northwest Africa 4255 27°51′00′′N, 7°48′00′′W Northwest Africa 4230 Hamada du Draa, southwest Algeria Algeria Find: September 2002 Find: December 2005 Achondrite (diogenite) Mesosiderite History: Nomads found the meteorite in September 2002 in History: G. Hupé purchased this stone in December 2005 in Hamada du Draa, southwest Algeria. Rissani, Morocco. Physical characteristics: The total mass is 6000 g and is Physical characteristics: The meteorite is a single 134 g fragmented into hundreds of pieces, some of which are partly stone containing abundant metal. covered with fusion crust. Petrography: (A. Irving and S. Kuehner, UWS) In thin Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine, section, the meteorite is texturally heterogeneous, mostly J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. Lorand, fragmental with variable grain size (0.5–4 mm), but some MNHNP). Predominantly composed orthopyroxene with regions have triple junctions among silicate grains. Abundant scarce inclusions of troilite, ilmenite, spinel, olivine, and metal (kamacite with taenite), orthopyroxene, plagioclase metallic Fe-Ni. (some with included grains of silica polymorph and Mineral compositions and geochemistry: Orthopyroxene clinopyroxene), schreibersite, merrillite, and troilite. One (Fs25.3Wo1.5; Fe/Mn = 23–28 [atomic]), spinel (Cr = rounded clot composed of clinopyroxene, merrillite and 0.92 wt%), olivine (Fa30), Fe, Ni-rich metal (NiO = <1 wt%). kamacite was observed. Oxygen isotopes: δ18O = 3.25, δ17O = 1.31, Δ17O = −0.38 Mineral compositions: Orthopyroxene (Fs30.9Wo2.7–2.9, FeO/ (all ‰). MnO = 23.9–26.2), plagioclase (An89.5–94.8Or.0.2), kamacite (Ni Classification: Achondrite (diogenite); S2, minor = 5.4–5.9 wt%), and taenite (Ni = 36–49 wt%). weathering. Classification: Mesosiderite. Type specimens: A total of 21 g of sample is on deposit at The Meteoritical Bulletin, No. 92 1653

MNHNP. Two thin sections are on deposit at UJM. An fragments: plagioclase (An88.4), diogenitic pyroxenes anonymous finder holds the main mass. (En67.4–75.9, Wo2.0–3.0), spinel (cr# = 0.89), olivine (Fa67–80). Basaltic fragments: plagioclase (An85.8–93.6), Northwest Africa 4269 27°59′N, 7°35′W pigeonite (En37.2,Wo7.7), pigeonite with augite lamellae δ18 Hamada du Draa, southwest Algeria (En39.6,Wo41.4). Oxygen isotopes: (R. Greenwood, OU) O Find: September 2004 = 3.34 and δ17O = 1.25, Δ17O = −0.48 (all ‰). Achondrite (eucrite, monomict) Classification: Achondrite (eucrite, polymict); moderate History: Nomads found a complete stone in September 2004 shock and minor weathering. in Hamada du Draa (southwest Algeria). Type specimens: A total of 2.55 g of sample is on deposit at Physical characteristics: The complete stone is fusion MNHNP. One thin section, one inclusion and a powder aliquot crusted and weighs 54 g. (430 mg) are on deposit at UJM. An anonymous finder holds Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine, the main mass. J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. Lorand, MNHNP). The rock is compact, fine-grained and contains Northwest Africa 4272 mm-sized metal grains. A heterogeneous granulitic matrix Northwest Africa with plagioclase and recrystallized pyroxene, associated with Find: December 2003 silica, fayalite, Ca phosphate, iron metal (Ni% <0.1), sulfide, Achondrite (diogenite) spinel, and ilmenite is observed. Some clasts display residual History: An anonymous collector recovered a single, ophitic texture (lath plagioclase with granular exsolved complete stone in the western part of the Sahara in December pigeonite). Pyroxenes occur as ferro-pigeonites exsolved in 2003. ferro-augite and ferro-hypersthene. Individual augite grains Physical characteristics: The individual is 6768 g and are also observed in the matrix. displays a partial fusion crust and regmaglypts. Mineral compositions and geochemistry: Augite (En26–27 Petrography: (A. Seddiki, Ud’OEA and UJM; Wo34–41), hypersthene (En29–30Wo6–5), and matrix augite M. Messaoudi, USTHB, Algeria; B. Moine, J. Y. Cottin, UJM; grains (En26Wo40). Pyroxene Fe/Mn (27 to 42 [atomic]), B. Devouard, UBP; M. Denise, V. Sautter, J. P. Lorand, spinel (Fe-rich chromite, cr# = 0.91). Oxygen isotopes: MNHNP). The sample is composed of Ca-poor pyroxene (R. Greenwood, OU) δ17O = 1.718, δ18O = 3.762, Δ17O = containing small opaque inclusions of spinel, troilite, and 0.238 (all ‰). metallic Fe-Ni (Ni 0.3 wt%). Specimen is crosscut by thin Classification: Achondrite (eucrite, monomict); S3, minor veins (50 μm) of plagioclase and displays small weathering. concentrations of Ca-rich pyroxene. Type specimens: A total of 19.2 g of sample is on deposit at Mineral compositions: Ca-poor pyroxene (Fs21.6–22.2 MNHNP. Two inclusions and one powder aliquot (1.690 g) Wo1.6–2.9), spinel inclusions (cr# = 0.85). Vein material: are on deposit at UJM. An anonymous finder holds the main plagioclase (An81.5–86.3), Ca-rich pyroxene (Fs7.75–8.1, mass. Wo45.3–4537). Pyroxenes (Fe/Mn = 24.7 to 31.9 [atomic]). Oxygen isotopes: (R. Greenwood, OU) δ 18O = 3.78 and δ17O Northwest Africa 4271 27°57′N, 7°50′W = 1.50, Δ17O = −0.46 (all ‰). Hamada du Draa, southwest Algeria Classification: Achondrite (diogenite); minor shock and Find: February 2003 weathering. Achondrite (eucrite, polymict) Type specimens: A total of 20 g of sample is on deposit at History: The meteorite found by nomads in Hamada du Draa, MNHNP. One thin section is on deposit at UBP. An southwest Algeria. anonymous finder holds the main mass. Physical characteristics: The stone displays a fine fusion crust and weighs 6 g. Northwest Africa 4294 Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine, Morocco or Algeria J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. Lorand, Find: February 2006 MNHNP). The stone has a fine- to medium-grained, Ordinary chondrite (type 3) brecciated texture containing mineral fragments of History: Purchased from a Moroccan dealer at the Tucson plagioclase, diogenitic pyroxenes, spinel, olivine, and silica. Gem and Mineral Show by A. Hupé in February 2006. The rock also contains some basaltic fragments displaying Physical characteristics: A single 84.2 g light brown stone both ophitic and subophitic textures, formed by plagioclase lacking fusion crust and with abundant, large chondrules. and pigeonite; some pigeonite grains also display augite Petrography: (A. Irving and S. Kuehner, UWS) Closely exsolution lamellae. Diogenitic fragments are low in packed PO and POP chondrules with a mean diameter of abundance (<10%). 1.2 mm. Chondrules contain accessory phases including Cr- Mineral compositions and geochemistry: Mineral bearing clinopyroxene, chromite, partially altered kamacite, 1654 H. C. Connolly, Jr., et al. taenite, troilite, and terrestrial barite. The content of metal Mineral compositions and geochemistry: Orthopyroxene (+minor Fe hydroxide) is very low (mode determined by BSE (Fs25.2–25.4Wo3.4–3.7; FeO/MnO = 30.4–33.5), olivine (Fa29.7, imaging of a whole thin section is 3 vol%). FeO/MnO = 48.1), and plagioclase (An89.8Or0.4). Geochemistry: Olivine (mostly Fa2–25, with rim Classification: Achondrite (diogenite). compositions up to Fa95) Oxygen isotopes: (D. Rumble, CIW) Type specimens: A total of 9.3 g of sample and one polished Analyses of two acid-washed whole rock fragments by laser thin section are on deposit at UWS. GHupé holds the main fluorination gave, respectively, δ18O = 5.38, 5.31; δ17O = mass. 3.34, 3.23; Δ17O = 0.508, 0.443 (all ‰). These oxygen isotopic compositions are closer to the TFL than to those of H Northwest Africa 4304 chondrites and far removed from those of LL chondrites. Northwest Africa Classification: Ordinary chondrite (type 3); S1, W2. Find: 2004 Specimens: A total of 22 g of sample and one polished thin Achondrite (ureilite, polymict) section are on deposit at UWS. AHupé holds the main mass. History: An anonymous finder recovered the specimen in the western part of the Sahara. C. Anger purchased the meteorite Northwest Africa 4298 in Baden, Austria, in 2004. Morocco or Algeria Physical characteristics: Eighteen small fragments totaling Find: September 2005 22.97 g were recovered. Ordinary chondrite (type 3) Petrography: (A. Greshake, MNB and M. Kurz, Kurz) History: Purchased from a Moroccan dealer in Erfoud by The meteorite is a polymict breccia with lithic and A. Hupé in September 2005. mineral clasts set into a ureilitic matrix dominated by Physical characteristics: A single 18 g light brown stone large olivine and pigeonite crystals. Lithic clasts include lacking fusion crust and with abundant, large chondrules. ureilite material and chondritic lithologies with Petrography: (A. Irving and S. Kuehner, UWS): Very well recognizable chondrule fragments. The meteorite contains formed and closely packed chondrules (mean diameter diamonds. 1.5 mm). Chondrules (PO and POP) contain euhedral olivine Mineral compositions and geochemistry: Ureilite material: or orthopyroxene crystals with Fe-enriched rims enclosed in Olivine (Fa1.1–22.4), pyroxene (Fs17.8Wo5.3). Chondritic glassy groundmass. Accessory kamacite (some as spherical lithologies: Olivine (Fa13.6–20.4), pyroxene (Fs12.9–14.4). grains in chondrules), taenite and troilite. The content of Classification: Achondrite (ureilite, polymict); extensive metal (+minor Fe hydroxide) is very low (mode determined shocked, moderate weathering. by BSE imaging of a whole thin section is 2 vol%). Type specimens: A total of 4.6 g plus one polished thin Geochemistry: Olivine (Fa0–46) Oxygen isotopes: section are on deposit at MNB. Anger holds the main (D. Rumble, CIW) Analyses of two acid-washed whole rock mass. fragments by laser fluorination gave, respectively, δ18O = 5.96, 5.57; δ17O = 3.78, 3.51; Δ17O = 0.639, 0.573 (all ‰). Northwest Africa 4360 Although these Δ17O values are within the range for H Northwest Africa chondrites, this specimen is much too poor in metal to be an H Find: 2005 chondrite. Rumuruti chondrite (R3.6) Classification: Ordinary chondrite (type 3); S1, W1/2. History: The meteorite was recovered by an anonymous Specimens: A total of 4 g of sample and one polished thin finder in the western part of the Sahara and purchased by the section are on deposit at UWS. AHupé holds the main mass. main mass holder in Erfoud, Morocco, in 2005. Physical characteristics: Approximately 100 fragments Northwest Africa 4302 totaling 308.5 g were found. Algeria Petrography: (A. Greshake, MNB) Clearly defined Find: December 2005 chondrules and chondrule and mineral fragments, all Achondrite (diogenite) embedded into a fine-grained matrix. In thin section the History: G. Hupé purchased the meteorite in December 2005 meteorite appears unbrecciated. in Tagounite, Morocco. Mineral compositions: Olivine (Fa34±11; range Fa0.3–39.8), Physical characteristics: The sample is composed of two low-Ca pyroxene (Fs16.1±5.6; range Fs9.3–24.7), augite very fresh, yellowish-green, partly crusted stones (36 g and (Fs9.2Wo46.7). 10.2 g) containing visible metal in cut slices. Classification: Rumuruti chondrite (R3.6); S4, moderate Petrography: (A. Irving and S. Kuehner, UWS) The weathering. meteorite is coarse-grained and has a partly cataclastic Type specimens: A total of 23.2 g plus one polished thin texture. It is composed mostly of orthopyroxene with minor section are on deposit at MNB. HSSH holds the main olivine, plagioclase, troilite, and kamacite. mass. The Meteoritical Bulletin, No. 92 1655

Northwest Africa 4362 low-Ca pyroxene, Ca-pyroxene, olivine, plagioclase, metallic Morocco Fe-Ni, and troilite. Silicate grains are often euhedral and Find: 2005 display an equigranular texture with abundant triple Carbonaceous chondrite (CK5/6) junctions. History: An anonymous finder collected the meteorite in Mineral compositions and geochemistry: Olivine (Fa4.4), the western part of the Sahara. The main mass holder low-Ca pyroxene (Fs5Wo1.5), Ca-pyroxene, (Fs2.3Wo46.2). purchased the sample in 2005 in Erfoud, Morocco. Oxygen isotopes: (I. A. Franchi and R. C. Greenwood, OU) Physical characteristics: One oriented stone of 60.1 g Mean of two replicates δ17O = 2.74, δ18O = 5.88, covered with fresh fusion crust was recovered. Δ17O= −0.31 (all ‰). Petrography: (A. Greshake, MNB) The meteorite shows a Classification: Primitive achondrite (winonaite); minimal fine-grained texture with recrystallized matrix dominating shock, moderate weathering. over rare and mostly poorly defined chondrules and mineral Type specimens: A total of 3.9 g of sample plus one polished fragments. Feldspar is abundant in the matrix and minor thin section are on deposit at MNB. HSSH holds the main phases include Cr-rich magnetite and Ca pyroxene. mass. Mineral compositions and geochemistry: Olivine (Fa29.9), low-Ca pyroxene (Fs25.5). Oxygen isotopes (I. A. Franchi and Northwest Africa 4380 R. C. Greenwood, OU): δ17O = −4.72, δ18O = −0.63, Δ17O = Northwest Africa −4.39 (all ‰). Find: 2006 Classification: Carbonaceous chondrite (CK5/6); minimal Achondrite (diogenite) shock, moderate to extensive weathering. History: An anonymous finder recovered the meteorite in the Type specimens: A total of 14.4 g plus one polished thin western part of the Sahara. The main mass holder acquired the section are on deposit at MNB. HSSH holds the main mass. sample in Erfoud, Morocco, in 2006. Physical characteristics: A total of 42 small fragments with Northwest Africa 4372 a combined mass of 211.2 g were recovered. Northwest Africa Petrography: (A. Greshake, MNB). The meteorite is Find: 2005 composed of large blocky orthopyroxene crystals. Minor Carbonaceous chondrite (CK4) phases include FeS and Mg-Al-chromite. History: An anonymous finder recovered the meteorite in the Mineral compositions: Low-Ca pyroxene (Fs22.9Wo1.5). western part of the Sahara. The main mass holder purchased Classification: Achondrite (diogenite); moderate shock, the sample at a mineral fair in Munich, Germany, in 2005. moderate to extensive weathering. Physical characteristics: One stone of 64.8 g was recovered. Type specimens: A total of 22.5 g of sample plus one Petrography: (A. Greshake, MNB). The meteorite consists of polished thin section are on deposit at MNB. HSSH holds the sharply defined chondrules, mineral fragments, and large main mass. CAIs set into a fine-grained matrix. Minor phases include feldspar, Cr-rich magnetite, and Ca-pyroxene. Northwest Africa 4391 Mineral compositions: Olivine (Fa24.6–28.8); low-Ca Northwest Africa pyroxene (Fs1.2–24.1). Oxygen isotopes: (I. A. Franchi and Find: 2005 R. C. Greenwood, OU) δ17O = −3.26, δ18O = 0.40, Achondrite (eucrite, polymict) Δ17O= −3.46 (all ‰). History: An anonymous finder recovered the meteorite in Classification: Carbonaceous chondrite (CK4); minimal northwest Africa. The main mass holder acquired the shock, extensive weathering. specimen in 2005 in Midelt, Morocco. Type specimens: A total of 13.5 g plus one polished thin Physical characteristics: A single stone weighing 54.8 g section are on deposit at MNB. HSSH holds the main mass. with a grayish color and little fusion crust present was recovered. Northwest Africa 4375 Petrography: (A. Greshake, MNB). The meteorite is a Northwest Africa polymict breccia consisting of coarse basaltic and mineral Find: 2005 clasts set into an abundant fine-grained groundmass. Primitive achondrite (winonaite) Mineral fragments are dominantly large plagioclase and History: An anonymous finder collected the meteorite in the exsolved low-Ca pyroxene. Minor phases include silica, western part of the Sahara. The main mass holder purchased ilmenite, and Al,Ti-rich chromite. the sample at a mineral fair in Munich, Germany, in 2005. Mineral compositions: Plagioclase (An85.5–95.9) and Physical characteristics: A small oval stone of 12.2 g was pyroxene (Fs41.7–54Wo2.6–20.1). recovered. Classification: Achondrite (eucrite, polymict); moderate Petrography: (A. Greshake, MNB). The meteorite consists of shock, moderate weathering. 1656 H. C. Connolly, Jr., et al.

Type specimens: A total of 11.4 g of sample plus one finder in northwest Africa and purchased by the main mass polished thin section are on deposit at MNB. Ralew holds the holder in Midelt, Morocco. main mass. Physical characteristics: A single stone of 228 g was recovered. Northwest Africa 4396 Petrography: (A. Greshake, MNB). The meteorite Northwest Africa displays a largely unbrecciated basaltic texture with Find: 2006 calcic plagioclase and exsolved low-Ca pyroxene Achondrite (eucrite, polymict) being the major phases. Minor phases include History: An anonymous finder recovered the meteorite in silica, ilmenite, and Al,Ti-rich chromite. northwest Africa. The main mass holder purchased the Mineral compositions: Plagioclase (An78.2–87.2) and sample in Tagounite, Morocco. pyroxene (Fs31.2–61.1Wo4.6–40.5). Physical characteristics: A single stone of 680 g, partly Classification: Achondrite (eucrite, monomict); moderate covered with fusion crust, was recovered. shock, minimal weathering. Petrography: (A. Greshake, MNB). The meteorite is a Type specimens: A total of 20.3 g of sample plus one polymict breccia consisting of coarse- and fine-grained polished thin section are on deposit at MNB. Ralew holds the basaltic and mineral clasts set in a fine-grained clastic main mass. groundmass. Mineral fragments are mostly large plagioclase and exsolved low-Ca pyroxene. Minor phases include silica, Northwest Africa 4399 ilmenite, and troilite. Northwest Africa Mineral compositions: Plagioclase (An58.9–92.7) and Find: 2005 pyroxene (Fs26.8–59.3Wo2.4–42.6). Achondrite (acapulcoite) Classification: Achondrite (eucrite, polymict); minimal History: The meteorite was recovered in northwest Africa by shock, moderate to extensive weathering. an anonymous finder and purchased by Stefan Ralew in Type specimens: A total of 20 g of sample plus one polished Midelt, Morocco, in 2005. thin section are on deposit at MNB. Ralew holds the main Physical characteristics: Many small fragments totaling mass. 210 g were recovered. Petrography: (A. Greshake, MNB) The meteorite consists Northwest Africa 4397 dominantly of low-Ca pyroxene, olivine, augite, troilite, Northwest Africa metallic Fe-Ni and plagioclase; minor phases include Find: 2006 chromite and phosphates. It displays a completely Achondrite (eucrite, polymict) recrystallized texture with abundant 120° triple junctions. History: The meteorite was recovered by an Mineral compositions: Olivine (Fa7.3; range Fa6.5–7.8), anonymous finder in northwest Africa and purchased low-Ca pyroxene (Fs8.7–9.2Wo2.2–3.2), augite, (Fs3.7– by the main mass holder in Tagounite, Morocco. 4.4Wo41.3–44.3; up to Cr2O3 = 1.7 wt%). Oxygen isotopes: (I. Physical characteristics: A single stone of 34 g was A. Franchi and R. C. Greenwood, OU) δ17O = 1.61, δ18O recovered. = 4.87, Δ17O = −0.92 (all ‰). Petrography: (A. Greshake, MNB) The meteorite consists of Classification: Achondrite (acapulcoite); minimal shock, coarse- and fine-grained basaltic and mineral clasts extensive weathering. The sample may be paired with NWA embedded in a fine-grained clastic matrix. Mineral fragments 2627. are mostly plagioclase and exsolved Ca-pyroxene. Minor Type specimens: A total of 20.3 g of sample plus one phases include silica, ilmenite, and troilite. polished thin section are on deposit at MNB. Ralew holds the Mineral compositions: Plagioclase (An68.1–92.7) and main mass. pyroxene (Fs36.7–58.8Wo8–28). Classification: Achondrite (eucrite, polymict); minimum Northwest Africa 4470 shock, moderate to extensive weathering. Algeria Type specimens: A total of 6.8 g of sample plus one polished Find: July 2006 thin section are on deposit at MNB. Ralew holds the main Achondrite (eucrite, basaltic, anomalous) mass. History: G. Hupé purchased the specimen in July 2006 in Rissani, Morocco. Northwest Africa 4398 Physical characteristics: The sample is made up of a total of Morocco 48 broken gray stones with a combined weight of 631 g. Find: 2005 Petrography: (A. Irving and S. Kuehner, UWS) The Achondrite (eucrite, monomict) meteorite is composed mainly of large, distinctively zoned History: The meteorite was recovered by an anonymous low-Ca pyroxene grains (≤0.8 mm) and interstitial The Meteoritical Bulletin, No. 92 1657 plagioclase, with minor silica (associated with blebby troilite), augite, chromite, and ilmenite. No metal was observed. Many pigeonite grains consist of multiple subgrains, with narrow zones of ferroan olivine along their boundaries. Mineral compositions and geochemistry: Orthopyroxene cores (Fs31.3–33.9Wo4.6–5.2, FeO/MnO = 26.8–27.4) have sharply defined boundaries against wider, much more Fe-rich mantles of exsolved pigeonite (host orthopyroxene Fs59.1–60.3Wo2.9–3.9, FeO/MnO = 31.9–33.9); olivine along subgrain boundaries in pyroxene (Fa81.7, FeO/MnO = 42.3); plagioclase (An88.9Or0.3). Classification: Achondrite (eucrite, basaltic, anomalous). Fig. 1. An image of a handsample of Northwest Africa 4473. The ferroan olivine along grain boundaries and the gap in pyroxene compositions requires that this sample be classified Petrography: (A. Irving and S. Kuehner, UWS) This as anomalous. specimen is composed of large mineral and polycrystalline Type specimens: A total of 20.1 g of sample and one polished lithologies (up to 8 mm across) with interstitial fine-grained thin section are on deposit at UWS. GHupé holds the main material of the same phases. The large minerals consist of mass. either olivine or orthopyroxene (with clinopyroxene exsolution lamellae associated with blebs of Ni-free iron Northwest Africa 4473 metal). The polycrystalline lithology consists mainly of Northwest Africa interlocking olivine grains (up to 3 mm across) and sparse Find: July 2006 large chromite grains with interstitial clinopyroxene, Achondrite (diogenite) orthopyroxene, kamacite, pyrrhotite, pentlandite, and troilite. History: G. Hupé purchased a total of 32 dark stones in July The modal abundance of metal (+limonite after primary 2006 in Laâyoune, Morocco. metal) is 5 vol%. Plagioclase is absent. Olivine grains contain Physical characteristics: Cut-surfaces of the stones show numerous blebby to worm-like polycrystalline inclusions, and pale yellowish-green angular clasts (see Fig. 1) and have a clinopyroxene grains contain similar inclusions; some combined weight of 7020 g. No fusion crust was noted for any examples exhibit symplectitic intergrowths of these various of the specimens. phases. Some olivine grains contain multiple blade-like Petrography: (A. Irving and S. Kuehner, UWS) Breccia lamellae of olivine of a different composition. Narrow composed of polycrystalline clasts (≤2 cm) set in a matrix elongate zones or discontinuous veinlets of metal are present derived from several different diogenite precursors. No within clinopyroxene, and adjacent to such metal the basaltic eucrite clasts were observed. The sample is modally pyroxene has a more magnesian composition. dominated by orthopyroxene with subordinate olivine, augite, Mineral compositions and geochemistry: Olivine chromite, silica polymorph, rare calcic plagioclase, troilite, (Fa10.6–10.9; FeO/MnO = 22.1–23.9), clinopyroxene pyrrhotite, and kamacite. (Fs3.9Wo41.9; FeO/MnO = 10.2), orthopyroxene lamella in Mineral compositions: Orthopyroxene compositions fall clinopyroxene (Fs9.1Wo1.3; FeO/MnO = 11.9) and chromite into at least three distinct populations (median compositions) (Cr/[Cr + Al] = 0.822–0.825; Mg/[Mg + Fe] = 0.506–0.520, Fs17.2Wo1.0, FeO/MnO = 34.4; Fs21.6Wo2.1, FeO/MnO = 29.3; TiO2 = 0.31–0.37 wt%). Oxygen isotopes: (D. Rumble, CIW) Fs37.2Wo3.5, FeO/MnO = 32.6). Olivine (Fa24.5, FeO/MnO = Quadruplicate analyses by laser fluorination gave, 50.2). respectively, δ18O = 2.23, 2.43, 2.23, 2.40; δ17O = 0.14, Classification: Achondrite (diogenite). 0.30, 0.07, 0.11; Δ17O = −1.034, −0.984, −1.107, −1.147 Specimens: A total of 20.1 g of sample and one polished (all ‰). mount are on deposit at UWS. GHupé holds the main mass. Classification: Achondrite (lodranite). Type specimens: A total of 20.1 g of sample and one polished Northwest Africa 4478 thin section are on deposit at UWS. GHupé holds the main Algeria mass. Find: September 2006 Achondrite (lodranite) Northwest Africa 4480 History: G. Hupé purchased the sample in September 2006 in Algeria Zagora, Morocco. Find: Summer 2006 Physical characteristics: Two dense, brown stones (298 g Achondrite (Martian, basaltic shergottite) and 146 g) lacking fusion crust. History: The sample was recovered in Algeria in the summer 1658 H. C. Connolly, Jr., et al. of 2006. G. Hupé purchased it in Tagounite, Morocco, in this specimen is almost entirely weathered to iron September 2006. hydroxides. Physical characteristics: The meteorite is a single, very Specimens: A total of 20.1 g of sample, one polished thin fresh 13 g ellipsoidal stone, mostly coated by dark brown section and one polished mount are on deposit at UWS. fusion crust. Maskelynite, yellow-green olivine and tan- GHupé holds the main mass. colored pyroxene are visible on cut face. Petrography: (A. Irving and S. Kuehner, UWS) The stone is Northwest Africa 4484 mostly a relatively fine-grained (mean grain size 0.15 mm) Algeria basaltic rock, but with several coarser grained, Find: June 2006 glomerocrystic regions. The dominant matrix consists of Achondrite (eucrite, basaltic) plagioclase laths (maskelynite), olivine and complexly zoned History: S. Ralew purchased the specimens in June 2006 in clinopyroxene with accessory Ti-chromite, ilmenite, Mg-Fe– Rissani, Morocco. bearing merrillite and rare Si-rich glass or silica polymorph. Physical characteristics: The meteorite consists of seven Glomerocryst regions are composed of coarser (0.5–0.8 mm) broken fragments of a dark gray stone with a combined plagioclase (maskelynite) and olivine with interstitial weight of 140 g. pigeonite and ilmenite. Petrography: (A. Irving and S. Kuehner, UWS) The thin Mineral compositions and geochemistry: Matrix- section studied shows an ophitic texture, with large clinopyroxene is patchily zoned from augite cores (≤1.3 mm) pyroxene grains (composed of orthopyroxene with (Fs24.9–31.2Wo35.3–31.1, FeO/MnO = 30–32) to pigeonite rims fine augite exsolution lamellae or patchy intergrowths of (Fs55.4–56.4Wo17.5–15.4, FeO/MnO = 36); olivine (Fa67.9–79.2, orthopyroxene with augite) and distinctive, thin plagioclase FeO/MnO = 49–52); plagioclase (An58.40–61.0 Or1.6). laths (commonly in radiating clusters). Interstitial mesostasis Plagioclase in glomerocryst regions is consistently more regions contain silica, ilmenite, troilite, and minor Ni-free calcic (An66.3–68.5Or0.3). Bulk composition (R. Korotev, kamacite (partly altered to brown iron hydroxides). WUSL): INAA of two ~37 mg whole fragments of matrix Mineral compositions and geochemistry: Augite gave Na 1.40 wt%, Fe 15.8 wt%, and (in ppm) Sc 39.7, Cr (Fs32.4–32.8Wo41.2–41.3; FeO/MnO = 32.7–36.7), orthopyroxene 1027, Ni <60, La 1.85, Sm 2.69, Eu 0.86, Tb 1.05, Yb 4.16, (Fs64.9Wo2.9; FeO/MnO = 32.2) and plagioclase Hf 3.16, Th 0.24; the REE pattern shows moderate light REE (An86.0–90.5Or0.2–0.5). depletion, elevated heavy REE abundances and a negative Eu Classification: Achondrite (eucrite, basaltic). anomaly. Type specimens: A total of 20 g of sample and one polished Classification: Achondrite (Martian, basaltic shergottite). thin section are on deposit at UWS. Ralew holds the main Type specimens: A total of 2.6 g of sample is on deposit at mass. UWS. PSF holds the main mass (6.63 g). Northwest Africa 4486 Northwest Africa 4482 Morocco or Algeria Algeria Find: September 2005 Find: August 2006 Ordinary chondrite (type 3) Pallasite (main group) History: Purchased at the Denver Mineral Show by A. Hupé History: G. Hupé purchased the sample in August 2006 in in September 2004. Tagounite, Morocco. Physical characteristics: A single 21.3 g light brown stone Physical characteristics: The meteorite consists of a total of lacking fusion crust and with abundant, small chondrules. 30 dark, magnetic fragments containing yellowish-green Petrography: (A. Irving and S. Kuehner, UWS): Closely silicate in a dark brown matrix. The fragments have a packed, round PO and POP chondrules (mean diameter combined weight of 5816 g. 0.8 mm) with accessory, partially altered kamacite, troilite Petrography: (A. Irving and S. Kuehner, UWS) Large olivine and pentlandite. The content of metal (+minor Fe hydroxide) grains (up to 8 mm across) with interstitial, porous, banded is very low (mode determined by BSE imaging of a whole iron hydroxides enclosing sparse angular grains of terrestrial thin section is 2 vol%). quartz, and accessory chromite, schreibersite and fresh metal Geochemistry: Olivine (Fa5–29), orthopyroxene (both kamacite and taenite). (Fs0.5–30Wo1.6). Oxygen isotopes: (D. Rumble, CIW) analyses Mineral compositions and geochemistry: Olivine of two acid-washed whole rock fragments by laser 18 17 (Fa12.2–13.0, FeO/MnO = 41.1–42.5). Oxygen isotopes: fluorination gave, respectively, δ O = 5.11, 5.51; δ O = (D. Rumble, CIW) analysis of acid-washed handpicked 3.15, 3.29; Δ17O = 0.465, 0.400 (all ‰). These oxygen olivine by laser fluorination gave δ18O = 3.65, δ17O = 1.72, isotopic compositions are closer to the TFL than those of H Δ17O = −0.198 (all in ‰). chondrites and far removed from those of LL chondrites. Classification: Pallasite (main group). The original metal in Classification: Ordinary chondrite (type 3); S1, W1/2. The Meteoritical Bulletin, No. 92 1659

Specimens: A total of 4.6 g of sample and one polished thin (Fs18.5Wo4.6). Microscopic observations and Raman analyses section are on deposit at UWS. AHupé holds the main mass. (T. Nakamuta, KyuU) show tiny diamond crystals occurring in blade-shaped graphite crystals. Northwest Africa 4506 Classification: Achondrite (ureilite); minimum weathering, Northwest Africa minimum shock. Find: October 2006 Type specimen: A total of 17.22 g of sample and one thin Pallasite (main group) section are on deposit at NSMT. Hori holds the main History: Michael Farmer purchased the sample in Denver, mass. Colorado, in October 2006. Physical characteristics: The meteorite was a fragment with Northwest Africa 4508 a total mass of 23.12 g. The exterior color of the meteorite Northwest Africa was orange and contains numerous by dark veins, as it was Find: 2001 mainly olivine with veins of oxidized metallic Fe-Ni. Achondrite (ureilite) Petrography: (D. Schrader, M. Killgore, and D. Lauretta, History: Purchased in Rissani, Morocco in April 2001. UAz) The meteorite contains olivine, Fe, Ni-rich metal, Physical characteristics: One subrounded blocky mass (5 × chromite, sulfide, and FeO. The olivine (2.2–3.2 mm) grains 3 × 2 cm) of 182 g and covered with dark brown, moderately are surrounded by weathered remnant metal veins. weathered fusion crust. Mineral compositions and geochemistry: (D. Schrader, Petrography: (H. Takeda, Chiba and A. Yamaguchi, NIPR). M. Killgore, D. Lauretta, K. Domanik, and D. Hill at UAz) The sample contains fine-grained, granoblastic olivine, partly Olivine (Fo86.3–86.8; average = Fo86.5±0.2), kamacite (average darkened pyroxene with carbonaceous (graphite) veins at Ni = 4.96 ± 1.60 [3.47 to 7.76] and average Co = 0.86 ± 0.04 grain boundaries. Minor weathering and heavily shocked. A [0.81–0.92] all wt%) and one taenite analysis (Ni = 20.75 and few grains of pyroxene or olivine crystals form larger grains Co = 0.54 [both wt%]). Reliable analyses on chromite and (0.7 × 0.4 to 3 × 1 mm). An original olivine crystal is broken troilite were not possible due to weathering. into many very fine crystallites to show a granoblastic texture. Classification: Pallasite (main group). There is an unusual texture of pyroxene crystals found in one Type specimens: A total of 8.17 g of sample is on deposit at of the sections studied. UAz (UA2059). Farmer holds the main mass. Mineral compositions and geochemistry: Olivine (Fo83–86 [cores], up to Fo89 [rims]); pigeonite (Fs14Wo7; Wo6– δ17 Northwest Africa 4507 10 range). Oxygen isotopes: (M. Kusakabe, OkaU) O = Morocco 2.97, δ18O = 7.66 (both ‰). Find: 2005 Classification: Achondrite (ureilite). Achondrite (ureilite) Type specimen: A total of 20.2 g of sample and one thin History: Purchased in 2006 at the Tucson Gem and Mineral section are on deposit at NIPR. Fectay holds the main Show. mass. Physical characteristics: Total mass, 85.0 g, a deformed parallel piped piece with smaller top surface, 68 × 24 × Northwest Africa 4519 24 mm in size, external color is dark brown and no fusion Morocco crust is apparent. Find: 2001 Petrography: (H. Takeda, Chiba). The sample consists of Achondrite (ureilite) olivine (up to 2.3 × 1.7 mm in size) and pyroxene. One PTS History: Purchased in Zagora, Morocco in 2001. shows a typical ureilite texture with carbonaceous veins, in Physical characteristics: The deformed conical shaped mass which Fe metal and sulfide are present. Approximately one- (114 g; 6.5 × 3.5 cm) is partially fusion-crusted. third of mafic silicates are pigeonite. A part of carbonaceous Petrography: (H. Takeda, Chiba and A. Yamaguchi, NIPR). veins intrudes into an olivine crystal as a plate. Olivine crystals It contains olivine and pyroxene with carbonaceous veins at have minor cracks, but shock effect is minor. Some pigeonite grain boundaries. Mafic silicate crystals seem to show a grains show a twin texture. preferred orientation, two to three crystals up to 4.2 × 1.4 mm Mineral compositions: Olivine Fo79–82 (core) and >Fo90 in size are joined with common elongation direction without (rims). Major pyroxenes have pigeonite compositions carbonaceous veins to form a large aggregate (~4.2 × 3.8 mm) (Fs19Wo10). A large olivine crystal contains a small ellipsoidal with carbonaceous materials around it. inclusion of pigeonite, 0.26 × 0.20 mm, with small regions of Mineral compositions and geochemistry: Olivine high-Ca (Fs14Wo35) and low-Ca (Fs17.3Wo4.8). Pyroxenes (Fo83–80 [cores]; Fo89 [rims]), pyroxene (Fs16.7Wo8.6). Oxygen enclosed in thick rims of the small ellipsoidal inclusion of isotopes: (M. Kusakabe, OkaU), δ17O = 3.29, δ18O = 8.20 pigeonite within the olivine grain; another ellipsoidal (both ‰). inclusion (0.16 × 0.09 mm) has low-Ca pyroxene composition Classification: Achondrite (ureilite); minimal weathering. 1660 H. C. Connolly, Jr., et al.

Type specimen: A total of 20 g of sample and two thin Petrography: (A. Irving and S. Kuehner, UWS) Olivine sections are on deposit at NIPR. Fectay holds the main mass. occurring with either prismatic low-Ca pyroxene phenocrysts or chromite microphenocrysts is set in a matrix of pigeonite, Northwest Africa 4523 maskelynite, Ti-chromite, ilmenite, merrillite, and pyrrhotite. Al Nif, Morocco Minor veinlets of calcite and barite are present. Find: April 2001 Mineral compositions: Olivine phenocrysts are zoned from Achondrite (eucrite, basaltic) Fa19.8–22.4 (cores) to Fa49.2–50.9 (rims) (FeO/MnO = 41–56); History: Carine and Bruno Fectay purchased the rock in Al pyroxene phenocrysts are zoned from orthopyroxene cores Nif, Morocco in April 2001. (Fs22.8Wo4.1, FeO/MnO = 40) to pigeonite rims (Fs40.1Wo11.9, Physical characteristics The very fresh stone weights 174 g FeO/MnO = 40); olivine microphenocrysts Fa32.7 (FeO/ and is nearly covered with fusion crust. The interior of the MnO = 51); maskelynite (An53.7–66.4 Or0.7–0.1); matrix stone is light gray in color and displays a brecciated texture chromite is relatively Ti-rich, whereas chromite occurring as with dark clasts ranging from a few mm to about 1.5 cm. microphenocrysts and as inclusions in olivine phenocrysts is Petrography: (J. A. Barrat and M. Bohn, IUEM; Ti-poor and Mg-rich. A. Yamaguchi, NIPR) Two types of clasts are found in a fine- Classification: Achondrite (Martian, basaltic shergottite). grained recrystallized matrix: medium-grained ophitic/ Type specimens: A total of 2.1 g of sample and one thin subophitic and fine-grained clasts. Medium-grained clasts section are on deposit at UWS. GHupé holds the main mass. (~1–2 mm) display a subophitic texture, and are composed of plagioclase, pyroxene (pigeonitic core and augitic rim), silica, Northwest Africa 4531 ilmenite, chromite, and recrystallized mesostasis. Fine- Morocco or Algeria grained clasts consist of pyroxene phenocrysts (~150 μm in Find: September 2005 diameter) in a fine-grained groundmass that consists of Ordinary chondrite (type 3) plagioclase, pigeonite, augite, silica, ilmenite, troilite, and History: Purchased at the Denver Mineral Show by A. Hupé K-feldspar. in September 2005. Geochemistry: (J. A. Barrat, M. Benoit, J. Cotton, IUEM and Physical characteristics: Three light brown stones (total A. Yamaguchi, NIPR). Mineral phases in clasts and matrix weight 38.9 g) lacking fusion crust and with abundant large have identical composition; pyroxenes (Mg35.9Ca4.7Fe59.4 to chondrules. En30.2Wo43.3Fs26.5; FeO/MnO = 34 [n = 265]) and plagioclase Petrography: (A. Irving and S. Kuehner, UWS) Closely (An90–71). Bulk composition: FeOtotal/MgO = 2.84 (ICP-AES) packed PO and POP chondrules with a mean diameter close to typical main group eucrites but exhibits the highest 1.0 mm. Chondrules contain accessory phases such as concentrations in K2O = 0.15 wt% measured in eucrites. partially altered kamacite, taenite, and troilite. The content of Moreover, it is richer in TiO2 = 1.35 wt% (ICP-MS) and metal (+minor Fe hydroxide) = 2 vol%. incompatible trace elements relative to Stannern. Its REE Geochemistry: Olivine (Fa4–27) Oxygen isotopes: element pattern is flat (Lan/Ybn = 1.29) and displays a marked (D. Rumble, CIW) Analysis of an acid-washed whole rock negative Eu anomaly (Eu/Eu* = 0.62). Bulk oxygen isotopic: sample by laser fluorination gave δ18O = 5.25, δ17O = 3.47, (R. C. Greenwood, I. A. Franchi, OU) composition is δ17O = Δ17O = 0.709 (all ‰). Although these Δ17O values are within 1.757 ± 0.004, δ18O = 3.791 ± 0.013, Δ17O = −0.230 ± 0.003 the range for H chondrites, this specimen is much too poor in (all ‰). metal to be an H chondrite. Classification: Achondrite (eucrite, basaltic) and lies on the Classification: Ordinary chondrite (type 3); S1, W1/2. Stannern trend. Specimens: A total of 7.8 g of sample and one polished thin Type specimens: A total of 21 g of sample and one thick section are on deposit at UWS. AHupé holds the main mass. section are on deposit at IUEM. Fectay holds the main mass. Northwest Africa 4587 Algeria Northwest Africa 4527 Find: September 2006 Algeria Achondrite (ungrouped) Find: Summer 2006 History: G. Hupé purchased the rock in September 2006 in Achondrite (Martian, basaltic shergottite) Erfoud, Morocco. History: The stones were recovered in Algeria in summer Physical characteristics: The meteorite comprises a single, 2006, and G. Hupé purchased them in M’Hamid, Morocco, in dense stone (530 g) without fusion crust. The main July 2006. constituent (pyroxene) is a distinctive deep brown color and Physical characteristics: The meteorite consists of two several large opaque grains are visible. broken, brown stones weighing 10.06 g. The stones have Petrography: (A. Irving and S. Kuehner, UWS) Granular weathering rinds ~2 mm thick. texture with large pyroxene grains (pigeonite with numerous The Meteoritical Bulletin, No. 92 1661 fine, parallel exsolution lamellae of clinopyroxene), and grains; these films of glass + daughter minerals truncate interstitial polycrystalline plagioclase (with rims of silica kirschsteinite exsolution lamellae in adjacent olivine. This against pyroxene). Accessory minerals are skeletal ilmenite, angrite is unlike other known specimens, having neither a merrillite, Ni-bearing pyrrhotite and rare kamacite. One large fine-grained quench or ophitic/intersertal basaltic texture nor a oikocryst of ilmenite + Ti-chromite contains numerous coarse metamorphic texture. chadacrysts of plagioclase and has narrow rims of fayalitic Mineral compositions and geochemistry: Clinopyroxene olivine adjacent to surrounding pyroxene. (Fs20.8–33.3Wo53–54.9; FeO/MnO = 85–278), olivine host Mineral compositions: Pyroxene consists of host pigeonite (Fa72.6–74.7Ln3.5–3.6; FeO/MnO = 70–87), kirschsteinite (Fs63.4Wo6.9 FeO/MnO = 67.6, TiO2 = 0.49 wt%) and lamellae lamellae (Fa44.7–45.4Ln46–47.2; FeO/MnO = 73–82), of clinopyroxene (Fs35.4Wo38.9, FeO/MnO = 69.4, TiO2 = kirschsteinite host (Fa46.6–47.5Ln43.6–45.5; FeO/MnO = 63–68), 0.90 wt%); plagioclase (An85); olivine rim adjacent to olivine lamellae (Fa75–76.7Ln2.7–2.8; FeO/MnO = 71–74). ilmenite (Fa81.9, FeO/MnO = 112). Oxygen isotopes: (D. Rumble, CIW) Analyses of two aliquots Classification: Achondrite (ungrouped). This very fresh of acid-washed mineral fragments by laser fluorination gave, stone is essentially identical to NWA 011, NWA 2400, and δ18O = 3.845, 3.881; δ17O = 1.927, 1.967; Δ17O = 0.0956, NWA 2976, and evidently is paired with them. 0.0745 (all ‰). Specimens: A total of 20 g of sample is on deposit at UWS. Classification: Achondrite (angrite). GHupé holds the main mass. Specimens: A total of 20.01 g of sample, two polished thin sections and two polished mounts are on deposit at UWS, and Northwest Africa 4590 30°19.025′N, 4°56.573′W 4 g at PSF. GHupé holds the main mass. Morocco/Algeria Find: June 2006 Northwest Africa 4615 Achondrite (angrite) Northwest Africa History: Scattered fragments from a small stone which Find: 2006 appears to have shattered upon landing recently were Rumuruti chondrite (R3.4) recovered from an area of ~40 m2 in the Morocco-Algeria History: The meteorite was recovered by an anonymous border zone, 21 km SSW of Tamassint oasis and 18 km S of hunter in the western part of the Sahara and purchased by Agoult, Morocco. G. Hupé purchased all the recovered J. Nauber in Morocco in 2006. material in June 2006 in Tagounite, Morocco. He then Physical characteristics: A 10.5 g stone. traveled to Tamassint and was shown the location by the Petrography: (A. Greshake, MNB) Various textural types of original find and measured GPS coordinates. chondrules with clearly defined outlines as well as chondrule Physical characteristics: Fragments totaling 212.8 g of a and mineral fragments, all embedded in a dark, fine-grained very friable specimen composed of coarse yellow-green, matrix. The meteorite appears unbrecciated in the thin section black and white grains; very fresh with preserved shiny, black studied. fusion crust on some pieces, and minor pale orange terrestrial Mineral compositions: Olivine (Fa23.9±14.7; range Fa2.4–41.5), weathering coatings on some broken surfaces. low-Ca pyroxene (Fs14.5±6.9; range Fs3.8–25.3). Petrography: (A. Irving and S. Kuehner, UWS) Coarse- Classification: Rumuruti chondrite (R3.4); S2, moderate grained (mostly 0.6–1.6 mm, but some olivine grains up to weathering. 12 mm) with a cumulate texture and composed of Type specimens: A total of 2.9 g of sample plus one polished clinopyroxene (33 vol%, with rare pigeonite exsolution thin section are on deposit at MNB. JNMC holds the main lamellae), pure anorthite (28 vol%), olivine (14 vol%, with mass. prominent subparallel exsolution lamellae 10–50 microns wide of kirschsteinite), kirschsteinite (5 vol%, with thin Northwest Africa 4619 exsolution lamellae of olivine), ulvöspinel (18 vol%), and Northwest Africa accessory glass, troilite merrillite, Ca silicophosphate, and Find: 2006 kamacite (making up the remaining 5 vol%). Some anorthite Rumuruti chondrite (R3–5) occurs as subhedral grains partially enclosed within large History: The meteorite was collected by an anonymous ulvöspinel grains, but most occurs as intercumulus aggregates. finder in the western part of the Sahara and bought by Clinopyroxene is strongly zoned with paler-colored, corroded J. Nauber in Morocco in 2006. cores surrounded by darker purple-brown mantles and distinct Physical characteristics: A 704 g stone. rims. Thin (5–50 μm wide) discontinuous, curvilinear zones of Petrography: (A. Greshake, MNB) A brecciated chondrite glass are present on some grain boundaries (notably those with dark and brighter lithologies ranging from petrological between anorthite and ulvöspinel, but also around and cutting type 3 to 5. across troilite grains), and are associated with secondary Mineral compositions: Olivine (Fa36; range Fa23–39), low-Ca clinopyroxene, kirschsteinite, olivine, anorthite, and troilite pyroxene (Fs18.2; range Fs9.7–29.6). 1662 H. C. Connolly, Jr., et al.

Classification: Rumuruti chondrite (R3–5); S2, moderate Northwest Africa 4677 weathering. Northwest Africa Type specimens: A total of 20.8 g of sample plus one Find: July 2006 polished thin section are on deposit at MNB. JNMC holds the Achondrite (eucrite, monomict) main mass. History: F. Béroud purchased the meteorite in July 2006 at Ste Marie-aux-Mines, France. According to the Moroccan Northwest Africa 4624 seller, the meteorite was found in the Sahara and other pieces Northwest Africa had been previously sold. Find: 2006 Physical characteristics: A single, complete, partially Achondrite (eucrite) crusted stone weighing 156.4 g. History: The meteorite was recovered by an anonymous Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine, collector in the northern part of the Sahara and bought by J. Y. Cottin, UJM; B. Devouard, UBP and M. Denise, Jürgen Nauber in Ensisheim, France, in 2006. MNHNP). The rock is brecciated and transected by impact Physical characteristics: Two stones totaling 175 g. melt veins. Undeformed clasts mostly consist of pyroxene Petrography: (A. Greshake, MNB). An unbrecciated and plagioclase grains (1–4 mm) with a cumulative texture. achondrite mainly consisting of exsolved pyroxene and calcic The pyroxenes are pigeonites with very fine (<1 μm) plagioclase displaying a cumulate texture. Minor phases exsolution lamellae. These clasts are embedded in a finer include chromite, pyrrhotite, troilite, and SiO2. The meteorite grained clastic matrix of the same nature. Accessory phases contains several dark shock veins. include spinel and taenite-kamacite-troilite assemblages and Mineral compositions: Pyroxene (Fs35.5–43.3Wo2.7–15.6) and silica. plagioclase (An91.1–93). Mineral compositions and geochemistry: Spinel (Fe,Ti-rich Classification: Achondrite (eucrite); extensive shock; chromite, Cr2O3 = 45 wt%), plagioclase (An91), pigeonite moderate weathering. (Fs41.20–42.40Wo7–10), pyroxene (Fe/Mn = 27–32). Kamacite Type specimens: A total of 21.5 g of sample plus one (Ni = 4.9) and taenite (Ni = 38.5–44.6, both wt%). polished thin section are on deposit at MNB. JNMC holds the Classification: Achondrite (eucrite, monomict); S3, minimal main mass. weathering. The meteorite is similar to Dhofar 007 and EET 92023. Northwest Africa 4636 Type specimens: A type specimen of 20.2 g is on deposit at Northwest Africa MNHNP and two sections are kept at UBP. Béroud holds the Find: 2005 main mass. Mesosiderite History: The meteorite was collected by an anonymous Northwest Africa 4678 finder in the western part of the Sahara and bought by the Morocco main mass holder at a meteorite fair in Germany from two Find: August 2006 different dealers. Achondrite (diogenite) Physical characteristics: Several dark stones totaling History: F. Béroud purchased the meteorite in August 2006 in 2850 g. Rissani, Morocco. Petrography: (A. Greshake, MNB and M. Kurz, Kurz). The Physical characteristics: A 3.60 g individual, oriented, stony portion of the meteorite consists of dominant pyroxene, nearly complete stone with black fusion crust over plagioclase, and phosphates. Minor phases include troilite, approximately 90% of the specimen. silica, and small metallic Fe-Ni grains. Metal is mostly Petrography: (A. Seddiki, UO and UJM; B. Moine, J. Y. kamacite. Cottin, UJM; B. Devouard, UBP; M. Denise, MNHNP). The Mineral compositions and geochemistry: Pyroxene stone is composed predominantly of Ca-poor pyroxene with (Fs31.1–35.0 Wo4.8–9.1), plagioclase (An94.5; range An91.8–95.5). small inclusions of spinel and troilite. Oxygen isotopes: (I. A. Franchi and R. C. Greenwood, OU) Mineral compositions and geochemistry: Ca-poor δ17 δ18 Δ17 The mean of two replicates O = 2.09, O = 4.38, O = pyroxene (Fs29.8–28.6Wo3.5–4.1), pyroxene (Fe/Mn = 26.4– −0.19 (all ‰). 31.8 [atomic]). Spinel Ti-poor chromite (Cr2O3 = Classification: Mesosiderite; minimal shock and moderate 56 wt%). weathering. Classification: Achondrite (diogenite); minimum shock and Type specimens: A total of 29 g of sample plus one polished weathering. thin section are on deposit at MNB. The anonymous purchaser Type specimens: The main mass of 3.34 g is deposited at holds the main mass. MNHNP and one thin section is kept at UBP. The Meteoritical Bulletin, No. 92 1663

Northwest Africa 4693 synonym for Richland. The new mass may be referred to as Morocco “Richland (Fredericksburg).” A total of 213 g is on deposit at Find: 2006 UCLA. Rumuruti chondrite (R3–6) History: The meteorite was recovered by an anonymous South America finder in western part of the Sahara and bought by the main mass holder in Erfoud, Morocco, in 2006. Peru Physical characteristics: One stone weighting 866.2 g. Petrography: (A. Greshake, MNB). A brecciated chondrite Cerro La Tiza 14°31′59.56′′S, 75°46′30.40′′W with pronounced dark and brighter lithologies ranging from Cerro La Tiza, Ica, Peru petrological type 3 to 6. Find: September 14, 2002 Mineral compositions: Olivine (Fa24.3; range Fa4.6–39.2) and Ordinary chondrite (H4) low-Ca pyroxene (Fs30; range Fs2.3–34.7). History: K. Hönninger and N. Diaz Zegarra recovered this Classification: Rumuruti chondrite (R3–6); S2, moderate meteorite in the course of an expedition. weathering. Physical characteristics: The meteorite consists of three Type specimens: A total of 24.3 g of sample plus one pieces with a total mass of 3740 g (3475 g, 235 g, and 30 g). polished thin section are on deposit at MNB. HSSH holds the Fragments are irregularly formed, shiny and of brownish main mass. color with very small black patches of fusion crust left. Petrography: (S. P. Schwenzer, MPI and J. Zipfel, SNG) Northwest Africa 4747 Sharply defined chondrules up to 0.8 cm in diameter. In rare Morocco chondrules turbid glass is observed. Fragments are fractured. Find: 2001 Along cracks weathering is more pronounced. Mesosiderite Mineral compositions and geochemistry: Olivine History: Purchased in Alnif, Morocco, in 2001 by B. Fectay. (Fa17.9±0.2) and pyroxene (Fs15.9±0.4), both homogeneous. Physical characteristics: A single rounded stone of 1.2 kg Classification: Ordinary chondrite (H4); S3, W3. with no fusion crust. Type specimens: A total of 97 g of sample and one thin Petrography: (A. Yamaguchi, NIPR). The thin section section on deposit at MPI. The finders hold the main mass. reveals a breccia composed of silicate fragments (<1 mm) (~80 vol%) in a matrix of Fe, Ni-rich metal and minor troilite. ANTARCTICA There are a few large nodules of metallic Fe-Ni (iron meteorite was reportedly found near Fredericksburg, Texas. Chemical analysis (Wasson et al. PNRA 2007) showed that it is indistinguishable from Richland, a 13.6 kg IIAB iron that was found ~300 km away. It is likely Table 4 lists meteorites collected by the Italian team, that these meteorites are paired and that one (or both) masses Programma Nazionale Ricerche in Antartide (PNRA) were transported by humans from their original find locations. recovered from the Allan Hills blue ice field (Victoria Land, Henceforth, the name Fredericksburg shall be an unofficial Antarctica) in November 2006. Mineralogy and classification 1664 H. C. Connolly, Jr., et al. performed by L. Folco (MNA-SI) and P. Rochette (CEREGE). Mineral compositions and geochemistry: Olivine Magnetic classification was conducted according to Rochette (Fa27.9±3.1; FeO/MnO = 37 ± 3), low Ca-pyroxene (Fs29.5±3.8; et al. (2003) and Folco et al. (2006) using a SM30 FeO/MnO = 22 ± 2), and plagioclase (An88.7–90.3Ab9.0–11.1). susceptivimeter. All main masses and type specimens are on Classification: Mesosiderite; minimal weathering. deposit at MNA-SI. Type specimens: The entire sample is on deposit at PRIC. PRIC ASIA Table 5 lists meteorites collected by the Chinese Antarctic Expedition to Grove Mountains, Antarctica, in 2006 and Arabian Peninsula submitted through the Polar Research Institute of China The Meteoritical Bulletin announces a new name series, (PRIC). Arabian Peninsula (AP), approved after considerable debate by the Nomenclature Committee of the Meteoritical Society. Grove Mountains 052049 72°46′23′′N, 75°20′8′′E Grove Mountains, Antarctica The five approved meteorites listed below, along with Find: January 16, 2006 reportedly 18 ordinary chondrites, were recovered near the Ordinary chondrite (L5) Rub al-Khali Desert (Empty Quarter) by workers in 2005 and History: X. Liu recovered the stone in a large moraine west to 2006. They were all sent to an anonymous American collector the northern part of Gale Escarpment in Grove Mountains. for verification in August 2006. Physical characteristics: It is a round stone mostly covered with fusion crust. The meteorite weights 96.7 g. Magnetic Arabian Peninsula 001 susceptibility: logχ = 4.60 × 10−9 m3/kg. United Arab Emirates Petrography: (Y. Lin, B. Miao, S. Hu, and L. Feng, Find: 2006 IGGCAS). It contains large melt veins (>3 mm thick) with Achondrite (diogenite) abundant rounded silicate clasts embedded in History and physical characteristics: This 145 g stone is microcrystalline matrix. Olivine grains in the melt veins very fresh with black crust and flow ridges. common have FeO-rich ringwoodite rims and FeO-poor Petrography: (T. Bunch and J. Wittke, NAU) Unbrecciated wadsleyite interiors. Chondrules in the unmolten parts are medium-grained orthopyroxenite with inclusions of euhedral recognized. chromite crystals. Contains 94 vol% orthopyroxene, 4 vol% Mineral compositions: olivine (Fa24.0±0.4); low Ca-pyroxene chromite, 2 vol% FeS, and trace olivine. Orthopyroxene (Fs20.6±0.5). exhibits heavy undulatory extinction, shear zones show Classification: Ordinary chondrite (L5); S6, W1 intense granulation and distortion of minerals. Type specimen: All of the mass is on deposit at PRIC. Mineral compositions and geochemistry: Orthopyroxene (Fs21.6Wo2.0; FeO/MnO = 29), olivine (Fa27.3, FeO/MnO = 45) Grove Mountains 055364 72°59′36′′N, 75°13′6′′E and chromite (Cr/[Cr + Al] = 79). Grove Mountains, Antarctica Classification: Achondrite (diogenite); moderate shock, Find: January 9, 2006 minimum weathering. Mesosiderite Type specimen: A 21 g sample is on deposit at NAU. The History: X. Chen recovered the meteorite in a large moraine main mass holder is anonymous. west of the middle of the Gale Escarpment in Grove Mountains. Arabian Peninsula 002 Physical characteristics: A 396.4 g meteorite with a round United Arab Emirates shape and many concaved areas. Part of the black fusion crust Find: 2006 remains. Achondrite (eucrite) Petrography: (Y. Lin, B. Miao, S. Hu, and L. Feng, Physical characteristics: A dark, 54 g completely crusted IGGCAS). It contains 23.9 vol% metallic Fe-Ni. The silicate stone. part consists mainly of low-Ca pyroxene (61.8 vol%), Petrography: (T. Bunch and J. Wittke, NAU). Eucrite plagioclase (32.3 vol%), and silica (5.9 vol%), with minor breccia with ophitic to subophitic textures. Contains olivine, chromite, and phosphates. Olivine occurs as clasts pigeonite, augite, plagioclase, FeS, metal, and SiO2. with embayed outlines and is surrounded by layers of low-Ca Pigeonite cores are rimmed by subcalcic augite. Pigeonite pyroxene and fine-grained chromite. Low-Ca pyroxene grains basal sections show well-developed twinning and are nearly homogeneous, without exsolved lamellae of Ca- plagioclase has extensive Carlsbad-albite twinning. pyroxene. Phosphates commonly occur along the boundaries Mesostasis pockets consist of fine-grained intergrowths of of Fe,Ni-rich metal with minor schreibersite. plagioclase, SiO2, and FeS. The Meteoritical Bulletin, No. 92 1665

Mineral compositions and geochemistry: Pigeonite cores with no fusion crust, partially desert-etched by (Fa41.4Wo8.2; FeO/MnO = 30), subcalcic augite rims sandblasting. (Fs46Wo21.6; FeO/MnO = 29) and plagioclase (An84.2–92.2). Petrography: (J. Wittke and T. Bunch, NAU) Porphyroclastic Classification: Achondrite (eucrite); minimal shock, minimal texture of relict cumulate basalt clasts surrounded by a fine- weathering with minor carbonate/ iron oxide veins. grained matrix of recrystallized basalt. Thin, shock-melt veins Type specimen: A 10.8 g sample is on deposit at NAU. The transcend the sample. Prominent iron oxide staining main mass holder is anonymous. surrounds metal grains. Mineral characteristics and geochemistry: Pigeonite Arabian Peninsula 003 (Fs52.5Wo8.7; FeO/MnO = 33), augite (Fs42.8Wo27.2), chromite United Arab Emirates (Cr/[Cr + Al] = 75), and plagioclase (An90.5). Find: 2006 Classification: Achondrite (eucrite, monomict breccia); Achondrite (diogenite) moderate shock and weathering. Physical characteristics: A 56 g stone that has been heavily Type specimen: A 21 g sample is on deposit at NAU. The sandblasted, no crust remains. main mass holder is anonymous. Petrography: (J. Wittke and T. Bunch, NAU) Unbrecciated with well-developed preferred orientation of orthopyroxene. Arabian Peninsula 006 Large chromite crystals (<2 mm) are surrounded by a corona- United Arab Emirates like “necklace” of very small orthopyroxene and olivine Find: 2005 grains. Chromite also has very tiny (<0.01 mm) inclusions of Achondrite (eucrite, monomict breccia) pigeonite, diopside, plagioclase, and FeS. Small grains of Physical characteristics: A 67 g stone that has somewhat FeS, metal, and clusters of olivine occur as inclusions in weathered fusion crust and desert staining. cumulate orthopyroxene. Petrography: (J. Wittke and T. Bunch, NAU) A fine-grained, Mineral compositions and geochemistry: Orthopyroxene eucrite monomict breccia. Ophitic- to subophitic-textured, (Fs23.5Wo2.3; FeO/MnO = 28), orthopyroxene inclusions plagioclase contains numerous, tiny (<0.02 mm) oriented (Fs21Wo2.7; FeO/MnO = 28), olivine (Fa25.5; FeO/MnO = 43), euhedral pyroxene crystals. Has a moderate degree of diopside inclusions (Fs11.1Wo42), and chromite (Cr/[Cr + Al] undulatory extinction in plagioclase and pyroxenes. Contains = 0.76). orthopyroxene, pigeonite, augite, plagioclase, ilmenite, Classification: Achondrite (diogenite); minimal shock, chromite, FeS, and metal. weathering in the interior is minimal. Mineral compositions and geochemistry: Orthopyroxene Type specimen: A 11.2 g sample is on deposit at NAU. The host (Fs56.6Wo2.2; FeO/MnO = 29), augite exsolution lamellae main mass holder is anonymous. (Fs28.8Wo43.6), pigeonite (Fs52Wo8.7; FeO/MnO = 33), and chromite (Cr[Cr + Al] = 84). Arabian Peninsula 004 Classification: Achondrite (eucrite, monomict breccia); United Arab Emirates minimal shock and weathering. Find: 2006 Type specimen: A 13.5 g sample is on deposit at NAU. The Achondrite (diogenite) main mass holder is anonymous. Physical characteristics: A 31 g stone that is partially covered with a dull black fusion crust. China Petrography: (T. Bunch and J. Wittke, NAU) Protogranular texture with several poikilitic grains of orthopyroxene host Weikengquan 40°16′N, 99°49′E and rounded olivine inclusions. Mineral modes (vol%): Jiuquan City, Gansu Province, China orthopyroxene = 94, olivine = 4, chromite, metal, and FeS = 2. Find: November 2, 2006 Mineral compositions and geochemistry: orthopyroxene Ordinary chondrite (H5, breccia) (Fs24.3Wo3.7; FeO/MnO = 28), olivine (Fa30.3; FeO/MnO = History: The stone lay on sand close to dunes at the 45), chromite (Cr/[Cr + Al] = 66), metal (Ni = 3.1 wt%). northwestern boundary of the Badanjilin Desert. H. Zang Classification: Achondrite (diogenite); minimal shock, recovered the stone on the way from the base to minimal weathering. Weikengquan. Type specimen: A 7 g sample is on deposit at NAU. The main Physical characteristics: The stone is 665 g, roughly ball- mass holder is anonymous. shaped and ~10 cm in diameter. It has a complete fusion crust with many cracks penetrating inside. Sand grains adhere on Arabian Peninsula 005 the crust. United Arab Emirates Petrography: (Y. Lin, B. Miao and S. Hu, IGGCAS) It is a Find: 2005 brecciated chondrite, consisting of numerous almond-like Achondrite (eucrite, monomict breccia) clasts cemented by fine-grained impact melt. In the clasts Physical characteristics: A brownish 146 g stone, chondrules are readily recognized, and troilite is much more 1666 H. C. Connolly, Jr., et al.

Kiel. A 1.7 g slice and one thin section are on deposit at Bart. The anonymous finder holds the main mass.

Sayh al Uhaymir 290 21°04′31.6′′N, 57°08′49.3′′E Oman, Al Wusta Find: February 13 and November 6, 2004 Carbonaceous chondrite (CH3) History: Sixty-four fragments were discovered within a distance of ~10 m by Rainer and Claudia Bartoschewitz during a natural science expedition on a gravel plateau of Miocene fresh-water limestone of Middle Fars group about 35 km SSW of Ghaba Resthouse (Adam County). Physical characteristics: Sixty-four fragments weighing between 0.2 to 888 g amount to a total of 1.796 kg. Petrography: The meteorite is mostly composed of small chondrules (<20 μm) of various textural types, ~15% fine- Fig. 2. An image of Österplana 002. grained metal, few small “matrix lumps,” and rare refractory inclusions. abundant than metallic Fe-Ni. In the melt breccias, metallic Mineral composition and geochemistry: (R. Bartoschewitz, Fe-Ni and troilite occur as small spheres, and there are Bart, P. Appel and B. Mader, Kiel, M.I. Prudêncio, ITN, nodule-like clasts with ringwoodite rims and wadsleyite U. Krähenbühl, Bern) Pyroxene (Fs3.99–5.16 Wo3.01–1.80; Al2O3 interior. = 1.90, Cr2O3 = 0.62 [wt%]), Ti-rich pyroxene (Fs2.88Wo19.66; Mineral compositions: Olivine (Fa19.4±0.4) and low Ca- Al2O3 = 10.40, Cr2O3 = 1.27 [wt%]), olivine (Fa1.88–0.83, CaO pyroxene (Fs17.1±0.2) are homogeneous, but plagioclase shows = 0.43–0.27, Al2O3 = 0.27, Cr2O3 = 0.47 [all wt%]), sulfide variation An11.7–20.6Ab69.8–85.5Qr1.5–10.6). Magnetic (Ni = 0.4–21.7 [wt%]), kamacite (Ni = 3.7–8.0, Co = 0.35– susceptibility: logχ = 4.45 × 10−9 m3/kg. 0.56, Si = 0.02–0.15, Cr = 0.08–0.40 [all wet%]), tetrataenite Classification: Ordinary chondrite (H5, breccia); S6, W3. (Ni = 59.2, Co = 1.45 [wt%]). Whole rock siderophile, Type specimens: A sample of 359 g is on deposit at IGGCAS. chalcophile, and lithophile element abundances similar to The finder holds 306 g. other CHs. Magnetic susceptibility: logχ = 5.2 × 10−9 m3/kg. Noble gas isotopes (J. Park and K. Nagao, UTokE, Japan, Oman R. Okazaki, KyuU) high concentrations of solar noble gases. O isotopes (M. Kusakabe, OkaU) 17O = 1.91‰, 18O = 5.71‰. Dhofar 1427 19°6.771′N, 54°49.126′E Classification: Carbonaceous chondrite (CH3); moderate Qitbit, Dhofar, Oman weathering. Find: January 17, 2001 Type specimens: A total of 20.1 g are on deposit UTokE. Bart Achondrite (ureilite) holds 1500 g and one thin section. History: A meteorite was found by an anonymous finder in the Omani desert about 34 km ESE of Qitbit on January 17, Table 6 lists all approved meteorites from Asia. 2001. Physical characteristics: The meteorite is a single dark EUROPE brown stone of 12.92 g with a magnetic susceptibility of logχ = 4.57 × 10−9 m3/kg. Sweden Petrography: (Bartoschewitz, Bart) Coarse-grained texture with triple junctions and curved grain boundaries formed by The Nomenclature Committee has recognized the new large (1–2 mm) elongated recrystallized olivines and minor category of relict meteorites. From the Guidelines for pyroxenes (<1 mm). Grain boundaries are outlined by dark Meteorite Nomenclature, http://www.meteoriticalsociety.org/ carbonaceous matrix material with finely dispersed metal. bulletin/nc-guidelines.htm#s77, a relict meteorite is defined Mineral composition and geochemistry: (Bartoschewitz, in such a fashion that special provisions are made for highly Bart and P. Appel, B. Mader, Kiel) Olivines (Fo74.2–79.8, CaO altered materials that may have a meteoritic origin, = 0.34, and Cr2O3 = 0.64 [all in wt%], Fe/Mn = 51); and designated relict meteorites, which are dominantly (>95%) pyroxenes, Fs13.0–21.6, Wo1.4–9.1, Cr2O3 = 0.97 (in wt%). composed of secondary minerals formed on the body on Classification: Achondrite (ureilite) with mosaicised typical which the object was found. Examples of such material may texture. include some types of “meteorite shale,” “fossil meteorites,” Type specimens: A total of 2.6 g of sample is on deposit at and fusion crust (as defined in section 1.2 of the guidelines). The Meteoritical Bulletin, No. 92 1667

The naming of relict meteorites is defined in section 7.7 of the main mass as located at the SWML. The correct mass is guidelines. A special type of name should be assigned to relict 3280 g and Tobin holds the main mass. meteorites. The documentation required for these names must include a description of the material, the location and date of In Table 7, NWA 2738 and 2739 are reported as being the find, the approximate mass or size, the location of the classified by Ted Bunch with the type specimen at NAU. It main mass, and the type of meteoritic material it is suspected should read that V. Moggi-Cecchi and G. Pratesi of MSP as to represent. The name must conform to all applicable parts of classifiers with the type specimen at MSP. sections 2–6 of the guidelines, and must be approved by the Nomenclature Committee prior to publication. Relict The Meteoritical Bulletin, No. 90, 2006 meteorite names may be converted to formal meteorite names by a second vote of the committee, subject to the requirements In Table 2, NWA 2457 is classified as an impact melt clast but of section 7.1 of the guidelines. it should be listed as an impact melt breccia. Furthermore, the follow additions to NWA samples should be printed within Reported in Table 7 are two new name series, Österplana and the comment column of Table 2: NWA 3347: breccia; NWA Gullhögen. Both are relict of ordinary chondrites recovered 3349: shock veins; NWA 3351: breccia, impact-shock breccia from strata of Ordovician age. clasts; NWA 3352: calcite veins; NWA 3353: shock veins, ringwoodite, partly S6; NWA 3355: calcite vein; NWA 3356: ERRATA shock veins; NWA 3357: shock veins, breccia, shock darkening; NWA 3359: An79±6, shock veins, breccia, Errata to previous editions of The Meteoritical Bulletin. polymict, impact-melt clasts, impact melt breccia clasts; NWA 3360: breccia, impact-melt clasts; NWA 3361: shock The Meteoritical Bulletin, No. 85, 2001 veins, breccia, impact melt breccia clasts; NWA 3362: shock veins, breccia, shock darkening; NWA 3363: shock veins, In Table 4, NWA 265 is listed with coordinates of recovery. breccia, shock darkening; NWA 3364: breccia; NWA 3365: However, these coordinates should be disregarded and, as shock veins, breccia; NWA 3367: breccia, shock veins. published, they are unknown. In Table 5, Dhofar 1301 is printed on June 15, 2006; however, The Meteoritical Bulletin, No. 88, 2004 this sample was shown to be the same as Dhofar 1286. Dhofar 1301 is thus not a valid name and is not official. In Table 5, Dhofar 607 is listed with coordinates of recovery as 10°43.728′N, 54°11.432′E. The correct coordinates are In Table 6, Minas Gerais b is incorrectly listed. It should be 18°43.728′N, 54°11.432′E. listed as Minas Gerais (b).

The description for Maromandia reports coordinates of The Meteoritical Bulletin, No. 91, 2007 recovery as 48.1°S 14.2°E. The correct coordinates of recovery should be 14.2°S 48.1°E. In Table 1, Tanezrouft 88 and 89 should be 088 and 089.

The Meteoritical Bulletin, No. 89, 2005 In Table 2, NWA 969 is listed as an LL7. It should be LL6/7.

In Table 2, Little Spring Creek is listed as having a mass of In Table 2, NWA 2748 is listed as L 3.4. It should be listed as 29,500 g. The correct mass is 2950 g. LL 3.4.

To Table 5, the following changes are made: Dhofar 543: H6, In Table 2, NWA 2954 is listed as having a 145 g. This should S3, W2; Fa19.7±0.14; Fs17.2±0.25, Wo1.13±0.02; Chromite (Al2O3 = be 1246 g. The main mass is listed as being held by Reed; 7.8, 2.6% MgO = 2.6, MnO = 0.9 [all wt%]). Whitlockite is however, Martinez holds the main mass. observed. Dhofar 545: LL4 (breccia), S2, W2; Fa31.4±1.02; Fs25.6±0.73; Wo2.45±0.08. In Table 3, Santa Vitoria do Palmar is incorrectly spelled as Santa Vitorio do Palmar. It is also listed with a mass of In Table 7, NWA 774 is listed with a mass of 523 g, purchased 5910.0 g but this should be 50,360 g. The correct coordinates in Tucson in 2001, and the main mass is located at the SWML. of recovery, both in the write-up and in Table 3, are The correct mass is 1440 g, it was purchased from an 33°30′34′′S, 53°24′39′′W. anonymous collector in 2000, and Tobin holds the main mass. In Table 5, Dhofar 962 was recovered on January 6, 2004. In Table 7, NWA 775 is listed with a mass of 1440 g and the Dhofar 969, 971, 973, and 975 were all recovered on 1668 H. C. Connolly, Jr., et al.

January 7, 2004. Dhofar 985 and 987 were recovered on LundU-2: Classified: B. Schmitz and M. Tassinari, LundU. Type January 10, 2004. Dhofar 1400 was recovered on specimen: LundU. Main mass: Undisclosed. November 25, 2003. UAE 001 was recovered on January LundU-3: Classified: B. Schmitz. Type specimen: LundU. Main mass: LundU. 18, 2005. MNA-SI-1: Classified: L. Folco, MNA-SI. Type specimen: OAM. Main mass: OAM. REFERENCES MNHNP-1: Classified: M. Bourot-Denise, MNHNP. Type specimen: MNHNP + 120.8 g. Main mass: Goueslain and Parodi. MNHNP-2: Classified: M. Bourot-Denise, MNHNP. Type specimen: Chennaoui Aoudjehane H., Jambon A., and Rjimati E. 2007. Al MNHNP. Main mass: Goueslain and Parodi. Haggounia (Morocco) strewn field (abstract #5329). Meteoritics MNHNP-3: Classified: M. Bourot-Denise, MNHNP. Type specimen: & Planetary Science 42:A30. MNHNP. Main mass: P. Thomas. Folco L., Rochette P., Gattacceca J., and Perchiazzi N. 2006. In situ MNHNP-4: Classified: M. Bourot-Denise, MNHNP. Type specimen: identification, pairing, and classification of meteorites from MNHNP. Main mass: Giessler. Antarctica through magnetic susceptibility measurements. MSP-1: Classified: V. Cecchi Moggi and G. Pratesi MSP. Type Meteoritics & Planetary Science 41:343–353. specimen: MSP. Main mass: MSP. Irving A. J., Kuehner S. M., Korotev R. L., and Hupé G. M. 2007a. MNB-1: Classified: A. Greshake, MNB. Type specimen: MNB. Main Petrology and bulk composition of primitive enriched olivine mass: Anonymous. basaltic shergottite Northwest Africa 4468 (abstract #1526). 38th MNB-2: Classified: A. Greshake, MNB. Type specimen: MNB. Main Lunar and Planetary Science Conference. CD-ROM. mass: Stehlik. Kuehner S. M. and Irving A. J. 2007. Grain boundary glasses in the MNB-3: Classified: A. Greshake, MNB. Type specimen: MNB. Main Tamassint plutonic angrite: Evidence for rapid decompressive mass: HSSH. partial melting and cooling on Mercury (abstract #1522)? 38th MNB-4: Classified: A. Greshake, MNB. Type specimen: MNB. Main Lunar and Planetary Science Conference. CD-ROM. mass: Ralew. Kuehner S. M., Irving A. J., Korotev R. L., Hupé G. M., and Ralew S. NAU-1: Classified: T. Bunch, NAU. Type specimen: NAU. Main 2007. Zircon-baddeleyite-bearing silica + K-feldspar mass: Farmer. granophyric clasts in KREEP-rich lunar breccias Northwest NAU-2: Classified: T. Bunch, NAU. Type specimen: NAU. Main Africa 4472 and 4485 (abstract #1516). 38th Lunar and Planetary mass: Aaronson. Science Conference. CD-ROM. NAU-3: Classified: T. Bunch, NAU. Type specimen: NAU. Main Rochette P., Sagnotti L., Bourot-Denise M., Consolmagno G., mass: Cimala. Folco L., Osete M. L., and Pesonen L. 2003. Magnetic NAU-4: Classified: T. Bunch, NAU. Type specimen: NAU. Main classification of stony meteorites: 1. Ordinary chondrites. mass: Hall. Meteoritics & Planetary Science 38:251–268. NAU-5: Classified: T. Bunch, NAU. Type specimen: NAU. Main Wasson J. T., Huber H., and Malvin D. J. 2007. Formation of IIAB mass: Boswell. iron meteorites. Geochimica et Cosmochimica Acta 71:760– NAU-6: Classified: T. Bunch, NAU. Type specimen: NAU. Main 781. mass: Reed. NAU-7: Classified: T. Bunch, NAU. Type specimen: NAU. Main ABBREVIATIONS mass: Oaks. NAU-8: Classified: T. Bunch and Wittke, NAU. Type specimen: NAU. Main mass: Boswell. Classifiers, Type Specimen Locations, Finders, and NAU-9: Classified: T. Bunch and Wittke, NAU. Type specimen: Holders of Main Masses NAU. Main mass: Aaronson. NIPR-1: Classified: A. Yamaguchi, NIPR. Type specimen: NIPR. A key to abbreviations for addresses used in the Meteoritical Main mass: Fectay. Ud’OEA-1: Classified: A. Seddiki, Ud’OEA and UJM; Bulletin is found at our web site, http://tin.er.usgs.gov/ B. Moine, J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. meteor/MetBullAddresses.php. Lorand, MNHNP. Type specimen: MNHNP and UJM. Main mass: Anonymous. Listed throughout most of the tables within the “Info” column UWS-1: Classified: A. Irving, UWS. Type specimen: UCLA and are relevant data on who classified the samples, where the UWS. Main mass: Gregory. UWS-2: Classified: A. Irving, UWS. Type specimen: UWS. Main type specimen is located, etc. Below is a key to the mass: Gregory. abbreviations used within this edition. UWS-3: Classified: A. Irving, UWS. Type specimen: UWS. Main mass: PSF. AMSA-1: Pickard, Williams, and McKinnon. Type specimen, UWS-4: Classified: A. Irving, UWS. Type specimen: UWS. Main AMAS. Main mass: Bessy. mass: GHupé. AMSA-2: Classified: Pickard, Williams, and McKinnon, AMAS. UWS-5: Classified: A. Irving, UWS. Type specimen: UWS. Main Type specimen, AMAS. Main mass: Bathurst. mass: AHupé. AMSA-3: Classified: Pickard, Williams and McKinnon, AMAS. UWS-6: Classified: A. Irving, UWS. Type specimen: UWS. Main Type specimen, AMAS. Main mass: Anonymous. mass: Ralew. IZU-1: Classified: A. Ibhi, H. Nachit, IZU; H. Chennaoui UWS-7: Classified: A. Irving, UWS. Type specimen: UAz. Main Aoudjehane, UHAC. Main mass: IZU. mass: Farmer. LundU-1: Classified: B. Schmitz and M. Tassinari, LundU. Type UWS-8: Classified: A. Irving, UWS. Type specimen: UAz. Main specimen: LundU. Main mass: LundU. mass: Jirasek. The Meteoritical Bulletin, No. 92 1669

Additional Abbreviations Used in the Text ALH = Allan Hills, CRS = Mount Cranfield, CMS = Cumulus Hills; DOM = Dominion Range; GRO = Grosvenor Mountains; For chondrule textural types: PO = porphyritic olivine, POP = LAP = LaPaz Icefield; LAR = Larkman Nunatak; MAC = porphyritic olivine pyroxene, PP = porphyritic pyroxene. MacAlpine Hills; MCY = MacKay Glacier; MIL = Miller Range; PRA = Mount Pratt, RBT = Roberts Massif, SAN = Sandford Abbreviations for the location meteorites recovered by ANSMET: Cliffs, and TYR = Taylor Glacier. 1670 H. C. Connolly, Jr., et al. entry entry entry breccia with fine-grained chondritic lithologies See separate entry entry See separate entry entry ) Info Comments χ Magnetic sus (log 4.64 MNHNP-1 Wo (mol%) Fs (mol%) 1.22–27.46 (5.36 ± 10.86) Fa (mol%) (10.36 ± 12.19) Type Type specmen mass (g) SS WG No. of pieces Class Many Aub 1.5 1 H5 1.4 S4/5 W3 18.5 16.2 MSP-1 Brecciated 7.8 1 H5 7.6 S2 W1 18.8 16.5 MSP-1 0.9 1 H6 0.7 S2 W2 19.2 16.8 MSP-1 10.9 1 L5 10.9 S3 W3 23.8 20.1 MSP-1 235 2 LL5 235 S3 W1 29.1 23.9 MNA-SI-1 397578 3 1971 H5 H4 21.8 4 22.3 2 L5 2 2 20.8 1 18.6 19.4 3 4 16.4 25.1 20.4 1.2 21.1 1.1 1.4 MSP-1 MSP-1 MSP-1 200177 1 6 L5 H4-6 20.4 22.8 3 3 2 3 24.5 18.5 21.7 14.0 1.4 1.2 MSP-1 MSP-1 Brecciated Total Total known mass (g) 1072 110632995 H4 7 24 24.6 H5 LL6 1 21.5 23.8 3 2 1 18.9 2 4 18.6 30.7 14.7 16.6 24.9 1.2 1.4 2.1 MSP-1 MSP-1 MSP-1 tons 49.8 1 Ure 10.2 Mod Mod 3.6–22.4 3.7–22.4 MNB-1 Polymict W 10.8 1 H5 10.8 S2 W2 19.1 15.4 See separate W 18.5 1 L5 18.5 S5 W2 24.9 21.4 See separate W 40 1 H5 40 S5 W3 15.5 16.8 See separate 0.801 1 LunarW 0.33 259.3 2 LL3.2 21 S4 W2 0.72–36.8 W 224 1 H4 20.53 S3 W2 19.89 ± 0.48 17.3 ± 0.31 MNHNP-2 W 131.6 3 H4 104 S3 W4 18.4–19.2 16.2–17.5 separate See W 13266 1 LL6 61 S1 W1 25.70 ± 0.28 21.86 ± 0.48 MNHNP-2 ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′′ ′′ W 383 1 LL6 20 S2 W2 25.81 ± 0.39 22.3 ± 0.56 MNHNP-2 ′ 32.1 1 LL6 30 S2 W4 30.1 26.1 MNA-SI-1 07 W~3 metric metric W~3 30 ′ ′ ′ ′ ′ ′ ′ ′ W 29560 >20 H5 115 S2 W0 18.6 16.3 See separate ′ 25°40 25°36.50 25°42.37 25°40 Longitude (E) 03°52 04°09 03°40.90 03°41.58 01°31.45 00°42.37 5°42.916 03°42.00 04°00.90 5°43.027 16°23 16°18.67 10°09.22 5°43.044 10°10.49 9°56.41 5°43.045 14°42.98 12°30 ′ ′ ′ 16°11 ′ ′ ′ ′ ′ ′ ′ ′ ′ ′′ ′′ ′ ′ ′ ′ ′ 16°00 02 09 5°54 ′ ′ ′ ′ ′ ′ ′ ′ ′ Latitude (N) Find/ Fall Jan-2004 Find 22°47 Date of recovery 19-May-2006 Find 31°30.165 17-Aug-2005 Find 31°29.150 28-Jan-2005 Find 22°59.61 12-Oct-2006 Fall 15°47 27-Jan-2005 Find 23°17.55 25-Jan-2005 Find 23°23.44 17-Aug-2005 Find17-Aug-2005 31°29.911 Find 31°29.909 10-Feb-2005 Find 24°38.18 2006 Find 27°30 geriageria Jan-2004 Jan-2004 Find Find 27°30.24 27°30.15 geriageria Jan-2004 Jan-2004 Find Find 27°21.61 27°33.48 Algeria Jan-2004 Find 27°37 , Libya 12-Dec-2005 Find 27°26 , Libya 16-May-1999 Find 27°02 , Libya 28-Jun-2001 Find 27°12.10 ni, Libya Nov-2006 Find 27°27 Mauritania (see Adrar, AlgeriaAdrar, (Rocky desert) Jan-2004 Find 27°22.22 southeastern Morocco southeastern Morocco (see IGN map 1/200000 feuille NF-29-XIV) Bassikounou, Hodh Ech Mauritania Chargui, Mauritania (see IGN map 1/000000 Ouadane NE-29-30) Mauritania (see IGN map 1/000000 Ouadane NE-29-30) southeastern Morocco southeastern Morocco IGN Map 1/1000000 Cap Bojador NG 28) Morocco 1 Haggounia, All A list of meteorites recovered from specific locations within Africa. of list A

Great Sand Sea 024 al Jadid, Egypt Wadi Al 1996 Find 25°16.99 Great Sand Sea 025 al Jadid, Egypt Wadi Al 2005Libya Dar al Gani 1043 Dar al Gani Find 25°22.41 Great Sand Sea 023 al Jadid, Egypt Wadi Al 1996 Find 25°10 Acfer 389Acfer 390Ilafegh 017 du Plateau Al Tamanghasset, Tademait 06 Al Tamanghasset, Silet Algeria Adrar, Egypt Great Sand Sea 022 al Jadid, Egypt Wadi Al Jan-2004 1994 Algeria Tamanghasset, Find 21°35.44 Find 25°55 NameAlgeria Acfer 386Acfer 387Acfer 388 Location of recovery Al Tamanghasset, Al Tamanghasset, Tamanghasset, Istifane 004 region, Istifane Dar al Gani 1047 Dar al Gani Istifane 003 region, Istifane Dar al Gani 1044 Dar al Ga Dar al Gani 1048 Dar al Gani Mauritania TalhaAdam Mauritania Talha, Adam Bassikounou km SE of 11 Rhall Amane 001 Amane, Rhall Rhall Amane 002 Amane, Rhall Istifane 001Istifane 002 region, Istifane region, Istifane Sueilila Sueilila, Morocco Al Haggounia 00 Table 1. Table The Meteoritical Bulletin, No. 92 1671 O = O = 42.7 17 17 δ δ ; basaltic ; ; Wo entry 14.3 O = 0.752, O = 0.693, 2.1–4.5 17 17 3.9–5.6 17.7–39.7 Δ Δ ; Fs Wo Wo 14.5 2.0 Wo Wo Wo 3.0–57.8 O = 3.03, 3.33; O = 2.95, 3.11; 48.3 37–46.3.3 32.5–36 55.2 18 18 4.33, 4.95; Fs 4.29, 4.52; Fs 0.726 (all ‰) 0.732 (all ‰) δ See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry δ See separate entry See separate entry See separate entry See separate entry ) Info Comments χ Magnetic sus (log NAU-7 Fs5 Wo (mol%) ) Information Comments χ Magnetic sus (log Fs (mol%) Fa (mol%) Type Type specmen mass (g) SS WG 4 W3 23.6 20.6 MNB-2 Contains shock veins No. of pieces Class Total Total known mass (g) Type specimen mass (g) SS WG Fa mol% Fs mol% mol% Wo 4162 1 L6 40.4 S4 W1 23.8 20separate See ′ Longitude (E) Dio 21 ~11°02 ′ hundreds No. of pieces Class Latitude (N) Find/ Fall 000 1 H6 20.2 S4 W2 18.6–19.2 16.4–17.0 1.5 UWS-5 ,200 1 H5 41.4 S2 W3 19.5 17.1 1.5 UWS-5 Total known Total mass (g) A 12,000 1 L6 21 S2 W2 25.1–25.6 21 1.3 UWS-5 Date of recovery Apr-1984 Fall ~12°51 rate; Ext = extensive; IM= impact melt. extensive; Ext = rate; Mod = moderate; Ext extensive. e, Morocco 439 1 H7 20.3 18.4–18.7 16.4 3.1–4.2 UWS-4 e, Morocco 46.2 2 Dio 9.3 Morocco 134 1 Meso 20.1 Morocco 661 1 CV3 22.4 ite, Morocco 124 2 EL3 20 ion): Aub = aubrite; Ure = ureilite. Ure aubrite; ion): Aub = A list of meteorites recovered from specific locations within Africa. of list A Location of recovery or purchase Min = minimal, Kolomari, Gashua, district, Nigeria Dapchi Date of recovery or purchase Continued. NWA 2959NWA 2005 Efroud, Morocco 121 1 Euc 21.1 Min Min NAU-8 Fs NWA 4229NWA Dec-2005 Tagounit 4230NWA Dec-2005 Rissani, NWA 4232NWA Dec-2005 Tagoun NWA 4269NWA 4271 Sep-2004NWA 4272 Feb-2003NWA Hamada du Draa 4292 Dec-2003NWA Hamada du Draa 4293 Sep-2005NWA Northwest Africa 4294 Sep-2005NWA Colorado, US Denver, 4298 Feb-2006NWA Colorado, USA Denver, 54 4300 Sept-2005NWA 25, Arizona, USA Tucson, 6,768 4302 Mar-2006 Efroud, MoroccoNWA 6 Dec-2005 Erfoud, Morocco 84 1 Tagounit 1 1 45 Euc 18 Dio 1 Euc OC (type 3) 1 19.2 22 (type 3) OC 20 2.55 4 NWA 4255NWA Sep-2002 Hamada du Draa 6000 Many NWA 4304NWA 4312 2004NWA 4313 2004NWA 4319 2004NWA Baden, Austria 2004 Zagora, Morocco Zagora, Morocco Zagora, Morocco 22.97 48 118 18 68 1 1 Ure 1 H6 L6 L6 4.6 10.6 20.8 15.6 S4 S S3 W1 W3/4 17.1 22.7 14.5 19.3 MNB-2 MNB-2 Name 2956NWA 2005 3157NWA Efroud, Morocco 2004 Colorado USA Denver, 161 51.7 1 1 Euc OC (type 3) 10.6 22 Mod Min NAU-9 Fs NWA 3221NWA 3222 2002NWA 3223 2000NWA 3340 2002NWA Rissani, Morocco 4223 Apr-2006NWA Morocco 4226 Dec-2005NWA Algeria or Morocco Morocco Dec-2005 Algeria Algeria 38.5 12.7 1 2 79 51 Ure 329 CM2-an 617 1 1 2 Ure 1 2.7 Ure 7.7 Dio H7 15.8 9.8 24 20.1 18.5–19.2 16.3 3.5–3.9 UWS-4 NWA 801NWA 1461NWA 2001 1924 Mar-2002NWA 2044 Jan-2001NWA Erfoud, Morocco 2764 Aug-2003 Zagora,NWA Morocco Efroud, Morocco 2005 Efroud, 252 5,000 Efroud, Morocco 255 Many 1 CR2 1 134 Dio CV3 1 + 1.3 23 77.4 Euc 20.4 20.1 NameNigeria Gashua Location of recovery settlement Near desert For class (which refers to classificat Shock stage (SS): Min = minimal, Mod mode grade (WG): Weathering Table 2.Table A list of all approved meteorites from northwest Africa. Table 1. Table 1672 H. C. Connolly, Jr., et al. W ′ N, 16°30 ′ 5.1–16.6 See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry ringwoodite are observed See separate entry See separate entry See separate entry See separate entry See separate entry Fa ) Information Comments χ Magnetic sus (log .4–13.0 3.0–9.0 MNB-2 shock veins and no No 21.9 4.2–21.2 MNB-2 shock veins Contains 4 S4 W2 30.3 24.8 MNB-3 Contains shock veins 5.8 S2 W0/1 0.4–17.4 1.0–17.7 MNB-2 Type specimen mass (g) SS WG Fa mol% Fs mol% mol% Wo 4 Imb 20.7 S4-IM W2 17.8 15.1–18.6 MNB-3 type Imr 36.6 IM W0/1 21.9 18.3 MNB-2 L3H/L3 8.2 S2 30 W2 0.4–32.2 S4 8.4–26.9 W1 3.7–31.1 2–24.3CV3 MNB-2 20.6 S2 W2/3 MNB-3 0.1–75 0.9–1.5 MNB-3 No. of pieces Class 483 11 1 1 H4/5 1 L4/5 L4/5 H6 22.4 24.5 S2 25.4 S4 28.4 S3 W3 S2 S2 W4 17.3 23.1 W3/4 22.2 17.6 15.4 19.3 19.1 15.6 MNB-3 MNB-3 MNB-3 MNB-3 0 1 L5/6 21.9 S3 W2 23.3 19.8 MNB-1 158.0 1 H5 38.52 S2 W4 19.1 ± 0.35 16.91 ± 0.22 4.91 MNHNP-3 757.0 1 H5 37.56 S2 W4 ± 0.43 18.72 1.16± 17.58 4.73 MNHNP-3 756.0 1 LL5 23.63 S3 W4 ± 0.31 25.46 0.33± 21.65 4.19 MNHNP-3 ~21°36 Total known Total mass (g) o 9,990 1 L5 30 S2 W1 24.1 20.9 1.2 UWS-4 Algeria border Algeria border Location of recovery or purchase Western Sahara Western A list of all approved meteorites from northwest Africa. Date of recovery or purchase Continued. NWA 4470NWA Jul-2006 Morocco Rissani, 631 48 Euc 20.1 NWA 4427NWA 2006 Erfoud, Morocco/ NWA 4426NWA 2006 Erfoud, Morocco/ 4473NWA 4475 July-2006NWA 4478 Aug-2005NWA Morocco Laâyoune, 4479 Sep-2006 Morocc NWA Tagounite, Apr-2004 Algeria, Morocco Morocco Tagounite, 32 444 552 1 Dio 2 2 Lod H6 20.1 20.1 20.9 S2 W2 19.1–19.6 16.4 1.3 UWS-4 Name 4320NWA 2004 Zagora, Morocco 160 1 H3 22.2 S2 W4 1 4391NWA 2005 Midelt, Morocco 54.8 1 Euc 11.4 NWA 4392NWA 4396 2005NWA 4397 2006NWA 4398 2006NWA Krefeld, Germany 4399 2005NWA Morocco Tagounite, 4424 2005NWA Morocco Tagounite, 2006 Morocco Tagounite, 490 Morocco Tagounite, 680 Bir Ganduz area, 34 228 1 210 1 1 R4 1 many Euc Euc Acp Euc 21.7 20 20.3 6.8 20.3 S2 W3 38.4 9–17.5 MNB-4 NWA 4323NWA 4325 2004NWA 4328 2004NWA 4329 2004NWA Zagora, Morocco 4331 2004NWA Zagora, Morocco 4334 2004NWA Zagora, Morocco 4337 2004NWA Zagora, Morocco 4338 2002NWA Zagora, Morocco 4339 2002NWA 70 Zagora, Morocco 180 4343 2002NWA Zagora, Morocco 4351 2002NWA 28 Zagora, Morocco 2002 26 2 Zagora, Morocco 1 21 Zagora, Morocco 83 1 L4 Zagora, Morocco 4360NWA 42 H5 1 4362 2005NWA 53 1 L type Imr 4363 2005NWA 40 1 H3/4 4364 2005NWA 23 1 4500 H3/4 Erfoud, Morocco 4365 2005NWA 1 H/L3 Erfoud, Morocco 6.6 14.8 4366 2005NWA 1 21.4 L5 Erfoud, Morocco 4367 2005NWA 12 1 H5 Erfoud, Morocco IM S3 4371 2005NWA S2 6 Erfoud, Morocco 308.5 2005 L 4.8 H3 Erfoud, Morocco W3 4373 W1 17.4NWA 60.1 W2 many Erfoud, Morocco 244. 4374 2005NWA S2 S2 Munich, Germany 232. 23.4 4375 2005NWA S3 9.4 R3.6 16.8 1 11.8 474. 4377 2005NWA W3 Munich, Germany W1 274. 4378 2005NWA W1 S3 Munich, Germany S2 4379 2005 CK5/6NWA 51.5 19.7 339.7 12.5–17.9 Munich, Germany 13.3–16.1 15.2 4380 2005NWA W2 2.0–30.0 Germany Stuttgart, W2 23.2 3.6–18.1 4389 2006NWA 2.6–17.0 Germany Stuttgart, 1 56.8 1 2005 4.3–17.2 26.4 Erfoud, Morocco 33.1 14.4 17.4 Erfoud, Morocco 12.2 H4/5 H 1 49.2 Midelt, Morocco 1 42.1 22 15.7 1 H4/5 494.4 1 H5 211.2 1 30.5 Win 55 1 L/LL5 many LL5/6 S2 14.2 Dio MNB-2 MNB-2 MNB-2 MNB-2 1 W3 MNB-2 8.2 S2 11.1 3.9 Ure 17.8 9. S2 W4 S3 22.5 W3/4 17.7 W0 15.5 MNB-2 MNB-2 17.8 12.1 27.1 15.9 Low 16.1 22.1 Mod 22.8 19.8 MNB-3 MNB-3 MNB-3 MNB-3 MNB-4 Reduced rim: NWA 4353NWA 4354 2003NWA 4357 2004NWA 2005 Erfoud, Morocco Erfoud, Morocco Erfoud, Morocco 23 1891 264.7 4372NWA 1 2005 1 Imb L6 Munich, Germany 21.5 64.8 1 W2 CK4 23.9 20.2 13.5 MNB-1 Table 2. Table The Meteoritical Bulletin, No. 92 1673 See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry (FeO/MnO = 45–48) See separate entry See separate entry See separate entry See separate entry See separate entry FeO/MnO = 41 See separate entry <3 mm See separate entry See separate entry ) Information Comments χ Magnetic sus (log 8–24.6 20.0– 20.8 2.4–2.5 UWS-8 Olivine .8 21.6 2 NAU-2 thick melt veins Polymict; S4 W2S3-5 32.6 W1 23 25.8 19.8 1.8S3-5 W1 2.4 23.8 20.5 NAU-2 = 62 FeO/MnO 1.4 NAU-3 darkened Shock NAU-4 darkened Shock 64 S2 W2 18.5 16.4 1.7 NAU-1 of Pyx? Olv 25 S3-5 W2 23.7 21.4 1.8 NAU-1 = 53 FeO/MnO Type specimen mass (g) SS WG Fa mol% Fs mol% mol% Wo 4 20.1 S2 W1 25.4–25.7 20.8–21.1 1.1–1.2 UWS-4 4-6 23 S3 W1 24.2 20.5 AMSA-1 Brecciated L4 28 S2 W2 22.8 20 2.1 NAU-1 = 47 FeO/MnO No. of pieces Class 00 10 L5 1 4 L47 LL5 23 1 S2 25.7 20.5 H4 W2 S2 S3-5 25.2 W2 W2 22.1 31.8 24.5 21.1 S2 25 21.6 W1 2.9 17.7 1.8 2.1 15.6 NAU-3 2.4 NAU-3 NAU-3 NAU-5 76 60 H5 27.1 S2 W2/3 19.1–19.8 15.7 1.5 UWS-4 500 1 LL5 23 S2 W2 27.8 23.4 2 NAU-3 850 52 H4 33.8 S2 W2/3 19.1–19.7 16.2 1.2 UWS-4 Total known Total mass (g) AA 68.7 1,245 1 1 H4 H4 14 32.8 S1 S2 W1 W2 17.4–17.7 19.1 14.9 16.8 0.8 1.3 UWS-5 UWS-5 USA 1,490 1 H5 22.4 S2 W3 19.5 17 1.3 UWS-5 Morocco 5,812 30 Pal 20.1 , Morocco 10 2 Martian 2.1 i, Morocco 3.6 1 Dio 3.34 Location of recovery or purchase A list of all approved meteorites from northwest Africa. Date of recovery or purchase Continued. Name 4480NWA Sept-2006 Morocco Tagounite, 13 1 Martian NWA 4482NWA 4484 Aug-2006NWA 4486 Jun-2006NWA Tagounite, 4506 Sept-2004NWA Rissani, Morocco Oct-2006 4507 Colorado, USA Denver, NWA 4508 2006NWA Colorado, USA Denver, 4519 2001NWA 21.3 4523 2001NWA 140 23.2 Arizona, USA Tucson, 4524 2001NWA Rissani, Morocco 1 Sep-2006 Zagora, Morocco 1 Morocco Tagounite, 85 7 Al Nif, Morocco 4528NWA OC (type 3) 4531 Sep-2006NWA Pal 182 Euc 4532 Sept-2005NWA Morocco Tagounite, 185.5 1 114 4533 Sep-2005 Colorado, USA 4.6 Denver, NWA 174 239,9 4535 Sep-2005NWA Colorado, US Denver, 1 Ure 1 4546 Sep-2005NWA Colorado, US Denver, 39 1 2006 Colorado, Denver, 20 8.17 Ure 1 L Ure 1 Erfoud, Morocco Euc 17.22 OC (type 3) 20.2 7200 20 7.8 21 many H4 NWA 4526NWA 4527 Sep-2006NWA July-2006 Morocco Tagounite, M’Hamid 52, NWA 4590NWA 4615 June-2006NWA Morocco 4619 2006 Tagounite, NWA 4624 2006NWA 4636 2006NWA Morocco 4649 2005 213NWA Morocco 4653 2006NWA Ensisheim, France 2006 many Germany Erfoud, Morocco Ang Erfoud, Morocco 175 10.5 704 3200 2 843 2850 20.01 1 1 1 Euc R3.4 >2 1 R3-5 LL6 Meso L5 21.5 2.9 20.8 35 29 22 S3 S2 W2 W1 28.8 23 24 AMSA-1 NWA 4547NWA 4548 2006NWA 4552 2006NWA 4554 2006NWA Erfoud, Morocco 4555 2006NWA Erfoud, Morocco 4557 2006NWA Erfoud, Morocco 4558 2006NWA Erfoud, Morocco 4559 2006NWA 3600 Erfoud, Morocco 4562 2006NWA 9132 Erfoud, Morocco 4563 1998NWA Erfoud, Morocco 280 many 4564 1998NWA Erfoud, Morocco 50 many 4565 2006NWA 1313 L4 Aqalmim, Morocco 4567 2005NWA Aqalmim, Morocco 250 3 4570 2005NWA Erfoud, Morocco 90 4587 2005NWA 1 Erfoud, Morocco 90 440 4588 July-2006NWA LL6 Erfoud, Morocco 1 2005 Erfoud, Morocco 89 Erfoud, Morocco H4 1 L4 Agadir 87 1 30 22 530 L4 243 H4 20.6 1 1 18.7 1 S2 L4 1530 Ach-ung 20.7 W3 L4 17.8 S2 19.1 1 20 S2 18 W2 L5 W2 20.1 17 22.9 S3-5 19 W1 2 20.2 24.1 26.1 17.1 S5 1.8 20.6 1.6 W0 1.5 23. NAU-3 NAU-3 NAU-3 NAU-4 darkened Shock NWA 4656NWA 4677 2006NWA 4678 Jul-2006NWA Aug-2006 France Erfoud, Morocco Rissan 5000 1 156.4 H4 1 Euc 34 20.2 S2 2 18.6 16.1 2.2 NAU-6 NWA 4680NWA Nov-2006 Erfoud, Morocco 3830 1 L NWA 4681NWA 4682 2006NWA 4683 2006NWA 2006 Erfoud, Morocco Erfoud, Morocco Erfoud, Morocco 3994 2920 1552 1 1 1 L5 L5 H4 38 30 22 S3 S4 S3 W4 W3 W2 24.7 23.3 18.9 21 20 ± 1 16.5 AMSA-2 AMSA-2 AMSA-2 Table 2. Table 1674 H. C. Connolly, Jr., et al. fragments; dark-light breccia; melt-filled veins See separate entry from 1.7 g to 20 g See separate entry a; Imr = impact-melt rock; Mes = ) Information Comments χ Magnetic sus (log rdite; Imb = impact-melt brecci .5 ± 1 AMSA-3 Brecciated = eucrite; How howa 24 21.71 ± 0.75 4.44 MNHNP-4 Mostly individuals, some io = diogenite; Euc 3 W3 18.9 ± 1 16.5 AMSA-3 pieces range 481 ouped; Bra = brachinite; D Type specimen mass (g) SS WG Fa mol% Fs mol% mol% Wo No. of pieces Class ngrite; Aung = achondrite, ungr = extensive; IM= impact melt. Total known Total mass (g) l, Mod = moderate; Ext = extensive. rocco 851 4 H4 22 S2 W2-3 17.7 15 : Acp = acapulcoite; Ang a Morocco 866 1 R3–6 24.3 hased unless otherwise stated. ud, Morocco 703 1 H6 22 S3 W3 19.7 17 ± 1 AMSA-3 Location of recovery or purchase A list of all approved meteorites from northwest Africa. = minimal, Mod moderate; Ext Date of recovery or purchase Continued. mesosiderite. Name 4684NWA 4686 2006NWA May-2006 Erfoud, Mo Erfoud, Morocco 3650 1 H5 24 S4 W4 18.9 ± 1 16.5 AMSA-1 NWA 4747NWA 2001For class (which refers to classification) Erfoud, Morocco 1200 1 Meso 20.9 Shock stage (SS): Min grade (WG): Min = minima Weathering All meteorites are finds and purc NWA 4693NWA 4695 Nov-2006NWA 4727 2006NWA Erfoud, Mar-2006 Morocco Agadir, Morocco 605 20.20 1 L6 H6 57 4.6 S5 S3 W2 W2 24.98 ± 0. 18 16.6 MNB-1 NWA 4687NWA 4688 May-2006NWA May-2006 Erfo Erfoud, Morocco 2184 481 H5 22 S Table 2. Table The Meteoritical Bulletin, No. 92 1675 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameGRO 03110GRO 03115GRO 03116 L5 Class GRO 03117 LL5 GRO 03118 CR2 GRO 03119 L5 LaPaz Icefield (LAP) L5 LAP 03551 L5 LAP 03552 111.5 86.1LAP 03554 B/C L6 108.3LAP 03555 A L6 B/C ALAP 03556 H4 87.5LAP 03557 A/B L5 A 64.1 B/CLAP 03558 L5 75.4 B/CLAP 03559 A/B L5 B/C 2703.4LAP 03560 A/B 1–37 L4 3521.5LAP 03561 A/B A/B L6 4201.2LAP 03562 A/B L6 1–8 A BLAP 03563 458.8 L5 A/B 1823LAP 03564 t H5 A/B 1505.1LAP 03565 A/B L6 A/B 1521.1 ALAP 03566 A/B t H4 1839.1LAP 03567 B A L5 A 1780 t LAP 03568 A/B L6 1853.2 t LAP 03570 L6 A A A/B t LAP 03571 B 833.5 LL6 t LAP 03574 A/B 868.5 LL4 B/CLAP 03575 853.8 L5 A/B A/B 1198.7 B LAP 03576 LL6 B 1454.4 A LAP 03577 B LL5 1009.5LAP 03578 A/B LL4 A 514.9LAP 03579 A/B LL6 A t A/B 801.6 A/BLAP 03580 L5 A/B BLAP 03581 796.9 LL4 A/B 580.7LAP 03582 LL6 B/C 643 A/BLAP 03584 A LL4 561 A LAP 03585 LL5 A B 556.2LAP 03586 LL5 B A/BLAP 03588 471.6 L5 411.8 A LAP 03589 L5 A/B A/B 582.9 A B/CLAP 03590 L5 541 A/B A/BLAP 03591 H4 A/B 408.6 t LAP 03592 LL5 A/B B 311.4 BLAP 03594 L6 BLAP 03595 289 LL5 A/B B 343.9 L5 t A/B B 209.6 LL5 A/B 232.7 A/B A/B 342.6 A B A/B A/B 235.6 192 A/B B A t t 297 C 175.4 t B B B B/C t C B t t t t t t t Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a Allan Hills (ALH) ALH 03541ALH 03542Cranfield Peak (CRA) H5 CRA 03540 L6 Mountains (GRO) Grosvenor GRO 03003 L3 GRO 03004GRO 03005 L5 1053.5GRO 03006 L5 BGRO 03008 L5 20.4GRO 03009 L5 B/CGRO 03010 A L5 151.9GRO 03011 10,640 L5 A/B BEGRO 03012 L5 2470 CEGRO 03018 A/B L5 2576GRO 03026 L5 B/CE C 1161.6GRO 03030 L5 B/CE B/C 1693 B/CEGRO 03034 0–26 L5 B/C 1112.9 B/CGRO 03040 L5 B/CE 1397.5 B/CEGRO 03041 LL5 B/C 1257.6 B/C B/CGRO 03042 H5 1184 B/CEGRO 03043 L5 B t 1554 B/C t GRO 03044 L5 t A/BEGRO 03045 561.2 L5 B/C BEGRO 03046 895.3 L5 B/C 274.6GRO 03047 L5 B B/CE A/B B 150.4GRO 03048 L5 t A/BGRO 03049 183.8 L5 B/C A t t GRO 03055 288.3 L5 A/B AGRO 03056 274.5 L5 t A/B t A/BGRO 03057 275.5 L4 A/B A/BGRO 03058 256.1 H5 B/C t A/B t GRO 03059 196.1 L5 B/C A/BGRO 03064 282 L5 t B A/BGRO 03065 394.4 L5 B/CEGRO 03066 311.3 LL5 B/C A t AGRO 03067 384.4 L5 B/C t A/B 422.5GRO 03068 L5 B/C t A/BGRO 03069 662.9 L5 B AGRO 03075 420.7 L5 t B/C t GRO 03076 625.3 L5 B/C t A/B 392.5 A/BGRO 03077 LL5 A/BE t B A/BGRO 03078 303.9 H5 A/B t 23GRO 03079 265.1 L5 B/C t A/B 140.1 LL5 A/B B 288.2 20 LL5 B A t 219.3 B/CE t t 294.2 B/CE A/B t A t A/B 257.7 A/B 201.1 B/C A 239.8 t B/CE t 165.4 A A/B A/B t A/B t A A t t t t t Name Class Table 3.Table A list of all meteorites approved from the 2003 to 2005 ANSMET seasons. 1676 H. C. Connolly, Jr., et al. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameLAP 03648LAP 03649LAP 03650 LL5 Class LAP 03651 L5 LAP 03652 LL4 LAP 03653 L5 LAP 03654 L5 LAP 03655 L5 214.7LAP 03656 LL5 A/BLAP 03657 149.4 L5 150.7LAP 03658 LL6 A A/B BLAP 03659 162 L5 A/BLAP 03660 LL6 98.6LAP 03661 A/B A/B L6 75.6 A/BLAP 03662 89.3 L5 A A/BLAP 03663 L5 A B 49.6LAP 03664 74.6 LL5 A/B B/CLAP 03665 L5 A/B A 87LAP 03666 79.7 LL6 A A LAP 03667 L5 A/B B/C 95.3LAP 03668 L5 96 A A/B t A LAP 03669 103.1 L5 t LAP 03670 68.1 LL5 A/B A/B A/B t LAP 03671 L4 A/B 64.1 A A/BLAP 03672 61.4 H6 A/B A/BLAP 03673 L5 A 40.8LAP 03674 H4 A 86.9 ALAP 03675 L4 A/B 42.4 A/BLAP 03676 42 L5 A/BLAP 03678 B/C L5 A/B 96.1 A/BLAP 03679 LL5 A 85.7 A/BLAP 03680 L5 A 73 CELAP 03681 L5 A 45.8LAP 03682 L6 B A/B t 76.4 B/CLAP 03683 L4 t 38.1 B/CLAP 03684 A L5 35.7 B B/CELAP 03685 52 L5 A t B ALAP 03686 t L4 58 BLAP 03687 H5 75.3 t LAP 03688 t B L5 B/C 55.8 B/CLAP 03689 B 126.2 L5 t A/B A/BLAP 03690 123.7 H5 B B t LAP 03691 L5 A A/B 57.7 t LAP 03692 t LL5 61.5 A A/B A LAP 03693 L5 54.8 B H5 A 42 t B/C t LL5 54.5 t A A t A/B 86.8 A/B 95.4 B/C A 69.1 A t B A/B A/B 88.3 t t 78.4 A A/B t A 71 B/CE t A A A/B A t t t Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameLAP 03596LAP 03597LAP 03598 LL5 Class LAP 03599 LL4 LAP 03600 L5 LAP 03601 LL6 LAP 03602 LL5 LAP 03603 H4 397.1LAP 03604 L6 245.2 BLAP 03606 L5 BLAP 03607 327.2 L5 413.2LAP 03608 A/B LL6 B 353 A/BLAP 03609 B L5 LAP 03610 331.7 H4 A/B A B LAP 03611 420.8 L5 A/BLAP 03612 305.4 L5 A/B A/B ALAP 03613 392.3 LL6 B/C 486.1 ALAP 03614 H6 A/B A/B ALAP 03615 359.2 L5 29 ALAP 03616 330.7 LL6 A A/BLAP 03617 451 H4 B ALAP 03618 447.2 H5 23 376.1LAP 03619 B L5 A/B A A/BLAP 03620 206.2 L5 ALAP 03621 229.8 L4 A B/C A/BLAP 03622 98.4 L6 A/B A/BLAP 03623 120.9 t L5 A/B ALAP 03625 L5 B/C t 99.5 ALAP 03626 173.8 L5 t B/C ALAP 03627 165 L6 t A/B t LAP 03628 164.3 A/B L4 BLAP 03629 B/C 121.8 L6 t A/BLAP 03633 173.5 L5 B A ALAP 03634 t 127.1 L6 A/BLAP 03635 t 147.8 L5 t A B t A LAP 03636 144.7 L5 A/B t LAP 03638 145.2 LL5 B/C A 23 A/B LAP 03639 155.5 L5 t B/C B LAP 03640 103.3 t L5 B/C A/B LAP 03641 14–19 R t B 56 A t LAP 03642 261.5 H4 t LAP 03643 103.3 H6 t A/B B/C A/B 124.3LAP 03644 H6 A A/B A/B A LAP 03646 t 190 L5 LAP 03647 134.8 LL5 A A A/B t L5 A/B 139.9 168.7 LL5 A A/B A 212.1 B 175.8 A B/C 230.2 B/CE A 126.4 A A B/C A/B 207.8 219.5 A 19–38 A A/B A/B 13–29 A A t t t t t t t t t t t t ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1677 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameLAP 03741LAP 03742LAP 03743 L5 Class LAP 03744 L5 LAP 03745 L5 LAP 03746 L6 LAP 03747 H5 LAP 03748 L6 LAP 03749 H6 70.1LAP 03750 H5 38.1 A/BLAP 03751 L5 46.3 BLAP 03752 LL6 A 79.4 BLAP 03753 L5 40.7 BLAP 03754 A H6 49 B/CELAP 03755 A H6 55.4 ALAP 03756 A LL6 A/B 65.9 B/CELAP 03757 LL5 22.5 B/C A/B ALAP 03758 29.6 L5 A/BLAP 03759 A/B LL6 A/B 49.5LAP 03760 L4 A 49.3 A/B A/BLAP 03761 H4 27.9 CLAP 03762 36.7 H6 A/B C t LAP 03763 28.4 L5 A/BLAP 03764 B L5 A/B t 56.1 A/BLAP 03765 C 25 H6 t A/B BLAP 03766 t L5 t 28.1 BLAP 03767 H4 t 48.8 ALAP 03768 A/B L5 t C 8.6 t LAP 03769 B L5 26.1LAP 03770 A/B C L5 t 34.5 t B/CLAP 03771 A H4 50.7 BLAP 03772 t L5 B B 33.6 CELAP 03773 H5 73.7 BLAP 03774 B L5 B t t 23 BLAP 03775 L5 t t 38.8LAP 03776 B L5 B 84.3 B/CLAP 03777 A/B L6 61.1 t BLAP 03778 L6 B 35.4 B B/CLAP 03779 H5 55.3 t t BLAP 03781 B 102.6 B L5 CLAP 03783 L5 B t 55.7LAP 03786 B Dio 58.2 A/B t t LAP 03789 B L6 23 B BLAP 03790 CM2 B t 14.6LAP 03791 t L6 A/B 71.9 B/C A L5 t 91.2 t C A/B L5 B 41.5 B 35 B t A/B t 17.3 22.4 A/B B t t C A/B B 20.8 A A/B t 37.8 B/C B/C 16.6 A/B A B A/B 22 1–40 A/B 6 2 t Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameLAP 03694LAP 03695LAP 03696 L5 Class LAP 03697 H6 LAP 03698 LL6 LAP 03699 LL5 LAP 03700 LL5 LAP 03701 H5 LAP 03702 H4 83.1LAP 03703 L5 44 A/BLAP 03704 39 H4 LAP 03705 58.7 L5 A B/CE A/BLAP 03706 84.5 H6 A/B ALAP 03707 L5 A/B A 89.5 ALAP 03708 L6 85.8 A/B ALAP 03709 H5 57.7 BLAP 03710 A L6 58.3 ALAP 03711 LL6 97.2 B/CLAP 03712 A/B H6 61.4 A/BLAP 03713 A/B B H6 59.4 CLAP 03714 L5 A/B 30.5 ALAP 03715 H5 84.6 t B/CLAP 03716 A L4 39.3 A t LAP 03717 A 41.3 LL5 B A t LAP 03720 t LL6 B/C 40.2 A LAP 03721 t LL5 63.5 C B LAP 03722 A LL5 84.9 t CLAP 03723 Ure 69.1 t BLAP 03724 B Ure 80.7 CLAP 03725 B 53 L6 A/BLAP 03726 B 25.7 H5 A/BLAP 03727 B 58.6 LL6 A/B BLAP 03728 51.4 L6 B A/BLAP 03729 LL5 B/C 87.5 BLAP 03730 L6 23 29.6 B B BLAP 03731 LL5 97.5 BLAP 03732 L5 60.5 B 13–18 B/CLAP 03733 45.7 R CLAP 03734 B/C t L5 B 57.9LAP 03735 B 30 L5 t B/CLAP 03736 A/B 9–25 H6 B t 62.1 BLAP 03737 4–25 58 L5 A/B t A/BLAP 03738 t LL6 47 B/CLAP 03739 B L5 A/B LAP 03740 56 t L5 B B 89.3 t L5 t 31.2 B B LL5 19.2 B C 130.1 B A B 68 B A/B 23.2 B B/C 30.2 B B 63.3 36 A/B 35.5 B B B B A/BE A/B 29 A t t t t t t t t t t ANSMET seasons. Table 3. 1678 H. C. Connolly, Jr., et al. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameLAP 031146LAP 031147 H5 LAP 031148 Class LL6 LAP 031149 H6 LAP 031160 H6 LAP 031161 L5 LAP 031162 L5 LAP 031163 L4 LAP 031164 4.9 L4 LAP 031165 5.5 B/C L5 LAP 031166 B 3.6 CM2 LAP 031167 A/B 2.3 C CM1-2 LAP 031168 38.9 A C L5 LAP 031169 18.6 C L5 LAP 031190 A 25.1 C L4 LAP 031191 A 37.3 B A/B Euc-brecciatedLAP 031192 32.2 A/B 27 B 15.1 L5 LAP 031193 B B L5 A/BLAP 031194 B B L4 4.7LAP 031195 10.7 B H6 LAP 031196 A 11.7 B C B CM2 LAP 031197 B/C 7.5 L5 LAP 031198 A B C H6 BLAP 031199 5.3 L5 LAP 031200 0–1 1–51 1.6 B/CE H6 LAP 031201 B 3.1 B/C B H6 LAP 031202 2.4 B/C H4 0.6LAP 031203 t B t C H6 LAP 031204 B t B 5.2 L5 LAP 031205 t 25–57 0.5 t C H6 LAP 031206 B t B 5.6 B t L5 LAP 031207 1.4 B/C H6 LAP 031208 B 15.4 B L5 LAP 031209 B 24.3 t C B t L4 LAP 031220 1–33 18.1 B L5 LAP 031221 B 25.2 C A/B t EH4 LAP 031222 23.2 2–22 t B A/B LL6 LAP 031223 14.4 C A/B t t H6 LAP 031224 26.8 B A t L3 LAP 031225 19.7 B/C A/B LL6 LAP 031226 26 B t A/B A/B LL6 LAP 031227 29.5 LL6 LAP 031228 B 3.1 B t A/B L5 LAP 031229 7.2 C t t L5 LAP 031230 A/B A 5.4 A/B LL5 t B t 4.8 C H5 7 t A/B B/C 3.3 t A/B A 2.7 B B t t B A/B 4.5 t t A/B 2.4 C 5.2 A/B B/C 1–27 12.9 B t 0–2 A C A/B t 3–19 t A/B t B Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameLAP 03792LAP 03793LAP 03794 H6 Class LAP 03795 R LAP 03796 H4 LAP 03797 H6 LAP 03798 DioLAP 03799 H6 LAP 03822 H6 7.4LAP 03824 L5 LAP 03900 15 C L-metal 8.5LAP 03901 L-metal BE 3.2LAP 03902 C L5 A/B 16.5LAP 03903 C L5 A/B B 4.6LAP 03904 R A/B 4.5LAP 03905 C L5 C 1.7LAP 03906 A/B 6.9 C H6 35 1.5 CLAP 03907 B L5 B CLAP 03908 L4 ALAP 03909 8.9 A 28 L5 BLAP 03950 8.6 A B/C L5 LAP 03991 B/C H6 6.2 12.7 t BLAP 031000 t H5 23 13.8 A/B B 24 CLAP 031037 H5 15.4 C 24 DioLAP 031043 A t 11.9 B FC t LAP 031046 B 20 B CM2 t LAP 031047 A/B 5.8 20 H5 LAP 031062 6.4 B C 37 L-IM t t 6.6LAP 031079 A/B C t Euc-brecciated 7.8LAP 031109 C A/B 10.5 CM1 LAP 031113 t 27.9 B/C 11–21 A/B C UreLAP 031117 B B 12.3 A t 0.1 Euc-brecciated 8.1LAP 031120 A/B CO3 A/BLAP 031121 C A/B 14.6 t A/B 16.5 L5 LAP 031122 A/B C A/B A/B A L5 2.2LAP 031123 t t L5 1.8LAP 031124 A 22 C 17 L5 LAP 031125 A C 14.5 1–48 t t L5 LAP 031126 B/C A H-IMLAP 031127 4.2 2 t C 15 A LL6 LAP 031128 B t 19 17–41 6.2 23 LL6 LAP 031129 11.9 B LL6 t LAP 031140 t B A/B 6.1 H6 17LAP 031142 19.6 17 9–25 B LL6 LAP 031144 B 10.4 B B L5 7 B 21–64 1–36 R B 8.5 B B 33.8 1 A B 32.5 A/B A A 13.5 A A 5.5 CE A B/C 9.9 A/B 17 B B 2.5 C A/B t 16 A/B t t t t 16–42 t t 7–19 t t t ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1679 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameLAP 031301LAP 031302 L5 LAP 031303 Class LL5 LAP 031304 LL5 LAP 031305 L5 LAP 031306 LL5 LAP 031307 LL5 LAP 031308 L4 LAP 031309 6.6 H-IM 23LAP 031310 C DioLAP 031311 4 B/C H4 LAP 031312 1.3 L5 B/CLAP 031313 B/C B 6.5 18.8 B LL6 LAP 031314 B/C B H5 BLAP 031315 45.8 8.7 B L5 LAP 031316 B B L5 CLAP 031317 14.1 B Euc-brecciatedLAP 031318 11.4 B A/B L5 LAP 031319 C 14.7 C 11.4 L5 LAP 031321 B/C 25.8 A H6 A/BLAP 031330 18.4 B B L-metal A/BLAP 031331 20.4 C A/B t LL5 19LAP 031332 34 B/C t LL5 LAP 031333 A/B B LL5 A/B t LAP 031334 B 16.1 18 16 H6 LAP 031335 17.3 t B t L5 LAP 031336 17.5 1.3 A/B B/C 23 t LL5 11–22LAP 031337 t B C t A/B 10.7 L5 BLAP 031338 t 17.7 LL6 BLAP 031339 t 27–84 A/B B 12.8 LL6 BLAP 031340 t t L4 CLAP 031341 t A/B 8.5 H6 LAP 031342 A/B 5.5 C H6 LAP 031343 8.7 B/C 24 t C UreLAP 031344 t 19.3 A/B L5 LAP 031345 C 9.4 C 22.9 A/B LL5 LAP 031346 t 20 B B H5 BLAP 031347 75.5 t B L3 LAP 031348 B/C t 2.7 t A/B L3 LAP 031349 B/C t 1.5 C LL5 BLAP 031350 3.2 C H5 t LAP 031351 3.6 C LL6 t LAP 031352 B 6.2 C L6 t LAP 031353 B B 7.3 L5 A/BLAP 031354 5.4 C H5 A/B t t B 9 B/C L5 5.7 t 2–21 A/B B/C B C 6.1 2.4 t t C B t A/B 2.6 B t 1.5 A B B 5–40 4.7 B/C t t 8.2 C A 4–16 B 0–33 t B/C t t A/B B 2–5 t t t t t t t t t t Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameLAP 031231LAP 031232 LL6 LAP 031233 Class L5 LAP 031234 L5 LAP 031235 L5 LAP 031236 H6 LAP 031237 L5 LAP 031238 12.8 H6 LAP 031239 L5 BLAP 031250 14 L5 LAP 031252 35.2 L6 LAP 031253 C A/B 11.9 B/C CM1 LAP 031254 33.6 B/C L5 BLAP 031257 13 B C H6 BLAP 031258 9.6 L5 LAP 031259 C A 9.4 C H5 LAP 031260 8.7 B L5 LAP 031261 B 1.1 B H5 0.8LAP 031262 B/C B L5 LAP 031263 BE B 1 L5 LAP 031264 B 1.3 B L5 t LAP 031265 A/B B 1.4 B L5 LAP 031266 2.1 B L6 LAP 031267 t 1.6 B C t H5 LAP 031268 A/B 11.8 t C L5 LAP 031270 B C 6.8 CM2 LAP 031271 B t 11.1 B H6 LAP 031272 B 15.6 B/C C t t LL5 LAP 031273 B 8.1 LL6 BLAP 031274 A/B t 8 B H6 LAP 031275 4.4 t A/B t L6 LAP 031276 16.6 A/B 15.4 C R LAP 031277 A/B B B L5 A/BLAP 031278 3.2 LL6 LAP 031290 B 8 B C L5 BLAP 031291 3 LL5 CLAP 031292 3.6 LL5 CLAP 031293 A/B 5.5 B LL6 LAP 031294 B 1–38 t C H5 LAP 031295 6.1 B t 6.2 H5 LAP 031296 A 2.2 B/C t C LL5 1–5LAP 031297 A C 2.5 A t LL5 LAP 031298 5.3 t t 13.7 C LL5 LAP 031299 A B/C B L6 BLAP 031300 2.1 t B CM2 B t B 17–42 1.1 LL5 B 4.4 t 24 1.7 B C 1.9 B 2.1 B A/B A/B B B 5.5 6.9 B C B 9.4 B B/C B B B t t 1–43 t t 1–38 t t t t t t ANSMET seasons. Table 3. 1680 H. C. Connolly, Jr., et al. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameLAP 04759LAP 04770LAP 04771 H4 Class LAP 04772 H5 LAP 04773 CM2 LAP 04774 L5 LAP 04775 AcpLAP 04776 L5 LAP 04777 L6 6.3LAP 04778 L5 1.1LAP 04779 C L5 0.6LAP 04830 B L5 BLAP 04831 1.6 Ure B 8.3LAP 04832 B/C LL5 B B CLAP 04833 5.4 L6 A LAP 04834 4.1 C H6 LAP 04835 3.8 19 B A/B L6 LAP 04836 3.4 19 B H5 A 1–50LAP 04837 7.9 B L6 B 16 1.8LAP 04838 C 13 Dio 2 B 4.3 16 LAP 04839 C Dio B BLAP 04841 0.3 How A/B 13–16 0.9LAP 04845 B Dio 24 B/CLAP 04846 A/B 0.5 C Lunar-basalt 0.9Larkman Nunatak (LAR) C R A 21 LAR 04328 0.8 B 263.1 Eur (brecciated) B 4–22 LAR 04360 4–22 542 B B C 56 323.5LAR 04361 H5 B B B 0.5LAR 04363 569.4 H6 A/B B ALAR 04365 B H6 B A/BLAR 04366 A H6 A/BLAR 04367 H6 1.1 A/B ALAR 04368 15,850 H6 BLAR 04370 H6 B/CLAR 04371 LL6 15.2 A/BLAR 04372 H6 A/B C 23 7.2LAR 04373 H6 27–75 31.4 23–54 LAR 04374 C L5 23 14.6 C 12–41 13–38 AB LAR 04375 H6 C 23 5.9LAR 04376 L4 A/B 12.3 8–16 B LAR 04377 C L6 4.3 C B LAR 04378 H5 15.5 ALAR 04379 LL6 A/B 17.1 C B LAR 04381 L6 C A 9.2LAR 04383 H6 16.3 B C H6 20.2 C B L5 17.3 C B 12.5 B/C B 24 B/C A/B A/B 36.2 B A/B C 9.2 14.7 C A/B C 2.4 B C B A B Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameLAP 031355LAP 031356 L6 LAP 031357 Class L5 LAP 031358 H6 LAP 031359 H5 LAP 031360 L6 LAP 031361 H5 LAP 031362 H6 LAP 031363 9.2 H5 LAP 031364 3.2 B/C L4 LAP 031365 2.9 C L5 LAP 031366 A 4.3 C H5 LAP 031367 2.5 C H5 LAP 031368 C 10.8 B/C LL6 LAP 031369 A/B 12.3 C H5 LAP 031371 A/B C B 4.7 L6 LAP 031373 A/B 9.1 C CM2 LAP 031374 B 5.4 B LL5 LAP 031375 11.8 C LL5 LAP 031376 B 12.8 C L5 LAP 031377 B 3.7 C H5 LAP 031378 B 10.1 A/B B t L5 LAP 031379 C B 3.2 A/B L5 8.8LAP 031380 t t 15.1 B/C Euc-brecciatedLAP 031382 B B t L5 CLAP 031383 6.5 B t H6 LAP 031384 t C B 4.5 LL6 4.3LAP 031385 B/C 2 B LL5 LAP 031386 A/B t B 2.2 H6 LAP 031387 C t A/B 1.5 C H6 LAP 031388 B 1–36 t C R LAP 031389 B/C t 1.1 H6 LAP 031391 B/C t 1–30 t 0.4 B H5 LAP 031392 B/C t 1.4 t B/C LL6 LAP 031393 0.2 A/B H5 LAP 031394 A/B t A/B B 0.6 A/B t H6 25–57LAP 031395 0.3 B/C H5 LAP 04750 t A/B B/C H6 LAP 04751 1.1 A/B 0.8LAP 04752 B A/B L5 1 B/CLAP 04753 1.7 H-IM t LAP 04755 A/B L5 A/B B t A/B 3.3 t LAP 04756 L5 1.1 B/C A t LAP 04757 L6 1.7 A/B BLAP 04758 A LL5 1–38 3 B/C t t Acp t A 5.9 A L6 2.8 B/C 1–30 B/C t B/C A t t 1.4 A/B t A/B 5.2 B 4.3 C 6.7 t B 12.8 B C 19 A C 7.5 t t A/B A/B C 16 B B/C 13 12–17 ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1681 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameMAC 041138MAC 041139 H5 MAC 041140 Class L5 MAC 041141 L5 MAC 041142 L5 MAC 041143 L5 MAC 041144 L5 MAC 041145 H4 MAC 041146 0.9 L5 MAC 041147 0.6 B L5 MAC 041148 0.3 B L5 MAC 041149 0.5 B L5 B MAC 041150 0.6 B L5 B MAC 041151 0.7 B L4 B MAC 041152 0.9 B L5 B MAC 041153 0.9 B H5 B MAC 041154 0.7 B L5 B MAC 041155 0.7 B L5 B MAC 041156 0.8 B L5 B MAC 041157 0.4 B H5 B MAC 041158 1.3 B H5 B MAC 041159 0.5 B L5 B MAC 041180 0.3 B L5 B MAC 041181 0.5 B L5 B MAC 041182 0.2 B L5 B MAC 041183 0.3 B L5 B MAC 041184 0.4 B L5 B MAC 041185 0.9 B L4 B MAC 041186 0.5 B L5 B MAC 041187 0.3 B H5 B MAC 041188 0.6 B L6 B MAC 041189 1.1 B L5 B MAC 041190 0.9 B L5 B MAC 041191 1.1 B L4 B MAC 041192 1.6 B L5 B MAC 041193 0.8 B L5 B MAC 041194 0.2 B B Acp/LodMAC 041195 0.5 B H5 B MAC 041196 0.9 B LL5 B MAC 041197 0.7 B L5 B MAC 041198 1.2 B L6 B MAC 041199 0.4 B L5 B MAC 041200 1.3 0.4 B L5 B MAC 041201 B B L5 B MAC 041202 0.5 L4 B 0.9 B L5 A/B B B 0.5 1.4 B B B 0.8 B 11 1 B B 0.5 B B 0.8 11 B B 0.5 B B B B B B Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameLAR 04384LAR 04385LAR 04386 L4 Class LAR 04387 H6 LAR 04388 H6 LAR 04389 H6 MacAlpine Hills (MAC) H6 MAC 04990 LL6 MAC 04991 10.1 L5 MAC 04992 43.9 B/C L5 MAC 04994 24.1 C L5 MAC 04995 B C 6.2 L5 MAC 041010 25.6 B/C L5 MAC 041011 C 9.6 L5 C B MAC 041012 L5 BMAC 041013 A/B L5 0.2 A MAC 041014 L5 0.6 B B MAC 041015 L5 0.6 BMAC 041016 L5 0.5 BMAC 041017 B L5 0.4 BMAC 041018 B 0.9 L5 BMAC 041019 B 0.4 B L5 MAC 041070 B 0.8 B L5 MAC 041071 B 0.4 B L5 B MAC 041072 0.6 B L5 B MAC 041073 0.4 B L5 B MAC 041074 0.7 B L5 B MAC 041120 1.1 B L5 B MAC 041121 1.2 B L5 B MAC 041122 0.8 B L5 B MAC 041123 0.7 B L5 B MAC 041124 1 B L5 B MAC 041125 1.2 H5 B MAC 041126 B 0.6 B L5 B MAC 041127 0.3 B L5 MAC 041128 0.9 B B H4 B MAC 041129 0.9 B H5 B MAC 041130 0.5 B L5 B MAC 041131 0.8 B LL5 B MAC 041132 0.5 B L5 B MAC 041133 0.5 B L5 B MAC 041134 0.6 B L5 B MAC 041135 0.5 B L5 B MAC 041136 0.5 B L5 B MAC 041137 0.7 B L5 B 0.3 B H5 B B 0.6 B 0.2 B B B 0.4 B 0.7 19 B B 0.4 B B 1.2 B B 0.6 5–21 B B B B B B ANSMET seasons. Table 3. 1682 H. C. Connolly, Jr., et al. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameMCY 05207MCY 05208 L6 MCY 05209 Class L6 MCY 05210 LL6 MCY 05211 LL5 MCY 05212 LL5 MCY 05213 L5 MCY 05214 210.9 LL5 MCY 05215 167.2 L4 MCY 05216 B/C 104.7 LL5 MCY 05217 B/C 426.4 A/B A/B L5 MCY 05218 344.8 A/B B/C L5 MCY 05219 A/B A/B 319.7 H3 MCY 05220 A 352.3 CV3 MCY 05221 A B/C A/B 306.1 L5 MCY 05222 254.3 A L5 MCY 05223 A B/C B 145.5 LL5 MCY 05224 A/B 198.7 H5 MCY 05225 A/B 214.5 A LL5 MCY 05226 B/C 145 A/B LL6 MCY 05227 B/C A L5 MCY 05228 B 96.6 A/B LL6 MCY 05229 81 B 81.3 L6 MCY 05230 A/B CM2 MCY 05231 A/B C 69 1–21 A/B 40.5 CM2 MCY 05232 A 67.6 CM1-2 MCY 05233 C B 0–4 B 2–9 CK4 MCY 05234 A 65.5 L5 MCY 05235 6.3 A A C CM1-2 MCY 05236 A 29.9 A/B L6 9.7MCY 05237 C 60.1 A/B B L6 MCY 05238 B 6.2 B L5 MCY 05239 B B/C L5 MCY 05240 2.1 B MesMCY 05241 A B 0.8 8.7 A/B LL5 MCY 05242 B C L5 MCY 05243 B 1.3 CM2 MCY 05244 1–28 2.1 A/B 0–33 1–32 B/C L6 MCY 05245 A/B 9.7 C LL5 MCY 05246 B 1.4 B 1–40 CM2 MCY 05247 19.3 33 0–2 C L6 MCY 05248 A/B C 1.2 LL5 MCY 05249 A/B B/C 2.5 L5 2MCY 05250 A/B B B/C A/B LL5 MCY 05251 11.1 B L6 3.1 A/B B/C CM2 1.3 B B B B 34–39 1.2 9.2 27–36 A/B B/C B B 0.8 4.7 B 1–25 B/C 34.9 B 25.3 A/B B B/C 6 B 0–40 B B 3 B 1–38 1 Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameMAC 041203MAC 041204 L5 MAC 041205 Class H5 MAC 041206 L5 MAC 041207 L5 MAC 041208 L5 MAC 041209 L5 MAC 041210 L5 MAC 041211 0.2 L5 MAC 041212 1 B L5 MAC 041213 1.3 L5 MAC 041214 B 0.9 B L5 B MAC 041215 0.8 B L5 MAC 041216 B 0.5 B H5 B MAC 041217 0.4 B LL6 B MAC 041218 0.5 B L5 B MAC 041219 0.4 B L5 B MAC 041220 1 B CM2 B MAC 041221 0.4 L5 B MAC 041222 B 0.2 B L5 B MAC 041223 1 B L5 0.7MAC 041224 B L5 B MAC 041225 B B 1.8 L5 B MAC 041226 0.9 B L5 0.5MAC 041227 B B B L5 BMAC 041228 0.8 L5 B MAC 041229 0.5 B L5 B MAC 041230 B 0.9 B L5 MAC 041231 0.9 B L5 B MAC 041232 0.8 B L5 B MAC 041233 0.4 B L5 B 1–38 MAC 041234 1.1 B L5 B MAC 041235 0.5 B L5 B MAC 041236 1.5 B L5 B MAC 041237 1.3 B L3 B MAC 041238 1.2 B L5 B MAC 041239 1.5 B L5 B MacKay Glacier (MCY) 1 B L5 B MCY 05200 1.1 B MCY 05201 B 1.1 B B LL5 MCY 05202 1.8 B L5 MCY 05203 1.5 B B B L5 MCY 05204 1.5 B B LL6 MCY 05205 1.6 B B LL6 MCY 05206 1.5 B B L6 3532.3 B B LL6 A/B 1917.7 B 1178.1 A A/BE B 1078.4 A/B A/BE A/BE 894.3 A A/B A 350.9 247.2 B B B A/B A/B ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1683 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameMIL 03371MIL 03372MIL 03373 L4 Class MIL 03374 LL5 MIL 03375 L5 MIL 03376 L5 MIL 03377 L5 MIL 03378 H6 MIL 03379 CO3 82.7MIL 03380 97.8 L5 BMIL 03381 103.9 H5 B/CMIL 03382 L5 B 71.3 A/BMIL 03383 A 125.9 H5 B/CEMIL 03384 212.5 LL5 C 129.8 A AMIL 03385 L5 C BMIL 03386 145.1 LL5 A/B 24MIL 03387 207.5 LL6 C BMIL 03388 A/B L5 C 85.7MIL 03389 L5 19 46 B BMIL 03390 58.4 L5 A/BMIL 03391 1–42 191 LL5 B/C B/C 122.5MIL 03392 t A/B H5 t A A BMIL 03393 A/B 99.3 L5 MIL 03394 127 LL5 A/B AMIL 03395 t A/B H5 t 68.3 AMIL 03396 B/C t 154.3 H6 t 146 BMIL 03397 H5 B A/BMIL 03398 t H5 B 83.9MIL 03399 A H5 68.9 A B/CMIL 03420 94.5 t H5 t A BMIL 03421 A LL5 B 64.7 t MIL 03422 LL5 22.3 B/CMIL 03423 A H5 t t 20 A B/CMIL 03424 A L5 29.1 t MIL 03425 t B LL5 B/CE B/CMIL 03426 3.9 t LL5 A/B 16.6MIL 03427 B/C 18.6 A t H5 B/CMIL 03428 45.1 L5 A/B AMIL 03429 A/B H5 A/B t AMIL 03430 2.4 t L5 29.4 AMIL 03431 B/C 45.4 t H5 t BMIL 03433 H5 A/B 4.4 AMIL 03434 H6 18.2 t A/B AMIL 03435 t A H6 35.2 t B/CMIL 03436 A L5 54.7 t B/C t A/B H5 23.5 B/C H6 A/B 27.3 t B/C A/B B/CE 4.4 t t A/B A 5.8 C t 16.5 CE t C 6.5 A/B A/B 4.6 t B/C 14.2 A C t t B C t t A/B A/B t t t t t t t t t Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameMCY 05252MCY 05253 LL6 MCY 05254 Class H6 MCY 05255 LL6 MCY 05256 L5 MCY 05257 H6 MCY 05258 L6 MCY 05259 41.5 L6 MCY 05260 L6 MCY 05261 A/B 18.2 L5 MCY 05262 8.8 B/C A/B LL5 MCY 05263 A/B 1 B LL6 MCY 05264 1.3 A/B LL6 Miller Range (MIL) B/C 0.5 B/C L6 MIL 03331 0.6 B/CMIL 03332 B B 0.8 B/CMIL 03333 H6 B 4.2 B/CMIL 03334 0.2 L5 B B/CMIL 03335 0.8 L5 B B MIL 03336 0.9 H6 B B MIL 03337 L5 B A/B 0.8MIL 03338 L5 A/B 1550 B/CMIL 03339 LL5 A/B 2395MIL 03340 L5 B C 1922MIL 03341 LL5 A/B 4025.9MIL 03342 LL5 A/B C 2283.3 B/CEMIL 03343 A LL5 MIL 03344 A B/CE B/C 969.8 H5 1564.7MIL 03345 A/B H5 BE A/BE 1597.3MIL 03347 H5 A 903.7MIL 03348 A/BE A/B L6 911.5 A/BMIL 03349 A/B LL6 717.2 A/BMIL 03350 LL6 A/B A/BMIL 03351 658 H5 B/CMIL 03352 765 LL5 A/B BMIL 03353 536.5 LL6 B/CMIL 03354 603.1 H5 B/C 548.2MIL 03355 A/B L5 B/C B/C 395 B/C A/BMIL 03357 L5 MIL 03358 B/CE 274.6 L6 B/C B 309.3 t MIL 03359 t H5 B/C t 368.6 A/BMIL 03365 H5 A/B A B/CMIL 03366 t 258.7 L5 A/BMIL 03367 t 262.9 L5 C BMIL 03370 t 159.8 L5 B/C 202.6 H6 B/C B/C A 501.2 H5 B t A 323.2 t C t t 502.7 C A 1114.8 t B B A/B 815.9 B 372.9 B/C A/B t BE t 169.8 t B/C A/B C B/C t t B t t t t t t t t t t ANSMET seasons. Table 3. 1684 H. C. Connolly, Jr., et al. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameMIL 05041MIL 05042MIL 05043 Eur (brecciated) Class MIL 05044 LL5 MIL 05045 239.8 L6 MIL 05046 L5 BMIL 05047 L5 MIL 05048 L5 B/CMIL 05049 LL5 262.6MIL 05050 L5 A/BMIL 05051 308 L5 60 MIL 05052 180.2 L3 A/B MIL 05053 C 283.4 L5 CMIL 05054 388.3 L5 B/CE 289.7MIL 05055 LL6 C B A/B C A/BEMIL 05056 197.2 H5 A MIL 05057 152 LL5 B/C A/B MIL 05058 253.3 LL5 B MIL 05059 B/C 368 LL6 BMIL 05060 257.6 L6 B 399MIL 05061 C L5 C A/BMIL 05062 233.6 LL6 B 109.2MIL 05063 L5 A/B B/C B 113.6 A/BMIL 05064 How 6–25 472.2 B/C A BMIL 05065 L5 A A/BMIL 05066 128.1 L5 3–17 MIL 05067 A 118.5 H5 A/B A/BMIL 05068 34.7 H5 B/C B/C MIL 05070 LL5 A/B 58.8 A MIL 05071 23.8 H5 A B/CMIL 05072 L6 B 23.3MIL 05073 L6 A/B 82.5 B/CMIL 05074 L5 23.3 A A/BMIL 05075 LL5 A/B 21.1 B/CMIL 05076 42 H5 A/B A/BMIL 05077 A L5 36.1 A/BMIL 05078 A L3 29–54 61.9 A/BMIL 05079 L5 A/B 28.4 CMIL 05080 A/B LL6 28.1 106.7 CMIL 05081 L5 C BMIL 05082 B LL6 88.4MIL 05083 B H6 86.8 CMIL 05084 A/B A/B CB 59.5 CMIL 05085 L6 32.5 BMIL 05086 A/B 41.2 L6 C B How A/B 82.7 A/B 30.2 CM2 A/B A/B B A/B 41.2 B 12 C A/B 35.7 B 30.9 B/C C 18.6 B/C 1.7 B B B B BE B A/B 1–3 0–25 1–3 0–4 27–60 Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameMIL 03437MIL 03438MIL 03439 H6 Class MIL 03440 H5 MIL 03441 H3 MIL 03442 H6 MIL 03443 L5 MIL 05001 CO3 MIL 05002 MesMIL 05003 6.8 L5 37MIL 05004 C H5 MIL 05005 1.4 LL5 C 31.7MIL 05006 B L6 A/B 34.3 CMIL 05007 63.8 L5 B B/CMIL 05008 C L5 46.3 A 3055.5MIL 05009 A/B 21,490 L5 B BMIL 05010 BE H5 2181.8 A/B CEMIL 05011 L6 A/B B BMIL 05012 2–20 831.1 H4 C 1127.8MIL 05013 A/B L5 B/C 0–38 1234.8MIL 05014 BE L5 0–15 B/CMIL 05015 BE 2 304.4 CO3 26 AMIL 05016 330.9 L5 B/C A MIL 05017 396.8 L5 B/CE B MIL 05019 582.4 L5 A/B A/B 1608.3MIL 05020 H5 B/C 2409.6 A MIL 05021 A/B 1494.6 L5 A/BMIL 05022 A/B L5 B/CE A/B MIL 05023 881.6 LL5 A/B A t 1025.8MIL 05024 t L5 A/B 1336.2 19MIL 05025 B LL4 t A MIL 05026 C 987.2 CO3 1–47MIL 05027 394.4 L5 t B B/C 16 MIL 05028 368.7 L5 A/B B/C 1–6 300.5 B/CE MIL 05029 LL6 B/C A/B A/B MIL 05030 235.7 LL5 133.1 B/C MIL 05032 L -IM A B/CE 196.6 A/BMIL 05033 LL5 A/B A/BMIL 05034 104.3 H6 A/B MIL 05035 A H5 A/B 72.5MIL 05036 67.5 L6 B/C A MIL 05037 77.9 Lunar-basalt A/BE 132.7MIL 05038 L6 A A/B B A/BE 112.9MIL 05039 0–55 H5 A/B A/B BMIL 05040 127.8 L6 179.2 L5 B/C A/B 192.4 L5 C 25 A/B C 314.1 A/B 21 239 C B 187.4 C 227.6 C B 305.4 A/B A/B B C A/B B ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1685 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameMIL 05134MIL 05135MIL 05136 L6 Class MIL 05137 L6 MIL 05138 L-IMMIL 05139 CM1 MIL 05140 LL6 MIL 05141 EH3 MIL 05142 H6 MIL 05143 3.6 L5 MIL 05145 4.9 C L5 8.3MIL 05146 C L6 2.4 B/CMIL 05148 LL6 BE A/B 7.5MIL 05149 10.6 B L5 B AMIL 05150 C B L6 13.4MIL 05151 L5 CMIL 05152 A/B 1.6 L5 C 11.4 25MIL 05153 C LL6 CMIL 05154 C 4.2 CM2 2.1MIL 05155 C L5 21 C AMIL 05156 2.3 B L5 2MIL 05157 0.9 C L-IM B MIL 05158 A/B 2.6 C LL6 42.3 101.5MIL 05159 B L6 B 0–3 C 46.6 AMIL 05160 L6 B MIL 05161 B LL5 B 51.2MIL 05162 B A/B L5 72 B/CMIL 05163 53.5 H6 A/BMIL 05164 94.4 B L5 B B/CMIL 05165 H6 B 95.2 A/B MIL 05166 L6 1–37 B 73.7 A/BMIL 05167 89 How B CMIL 05168 H6 B 1–26 38.4 BMIL 05169 L6 24.6 CMIL 05171 B 25 L6 33.7 CMount Pratt (PRA) B L5 42.9 CPRA 04401 A H6 38.8 C 21 PRA 04402 B 25.6 B/CPRA 04403 B How B 39.7PRA 04404 B How B 29 CPRA 04405 LL6 B 75.7PRA 04406 LL6 C 48.1 BPRA 04407 A LL6 B/CPRA 04408 4.3 H6 A PRA 04409 55 B C L5 B 37.8 LL6 655.7 CE LL6 B B/C 358.9 B 1373.5 B 30–60 B A B 1188.6 A C A 508 384.7 A 326.8 A/B B A/B A/B A A/B B 1–60 16–60 Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameMIL 05087MIL 05088MIL 05089 LL6 Class MIL 05090 L5 MIL 05091 L6 MIL 05092 L6 MIL 05093 L5 MIL 05094 L5 MIL 05095 13.1 LL6 MIL 05096 LL5 B 16.8MIL 05097 LL5 17.3 BMIL 05098 LL5 B 23.5 A/BMIL 05099 LL6 14.8 A/BMIL 05100 B H4 B 31.5 CMIL 05101 L5 B 6.9 CMIL 05102 L6 9.4 AMIL 05103 A/B 28.3 L5 B/CMIL 05104 A/B 13.9 L5 BMIL 05105 A 24.6 B L5 A/BMIL 05106 CO3 B B B MIL 05107 9.9 L5 49.9MIL 05108 C LL5 B 17.3 BMIL 05109 LL6 22.2 CMIL 05111 L6 B 12.8 CMIL 05112 A/B LL5 B/CMIL 05113 41 5.6 C L5 MIL 05114 C C CM2 B 33.3 BMIL 05115 12 LL5 A/BMIL 05116 18.7 H6 B A/BMIL 05117 A L5 A A/BE 19.5MIL 05118 L5 A A 5 CMIL 05119 L5 MIL 05120 0.9 H4 2.8 B/C 1–28MIL 05121 A/B B/C CM2 0.3 B MIL 05122 L6 1 B/C B MIL 05123 7.8 LL6 MIL 05124 5.9 C B L6 MIL 05125 2.2 B/C L6 MIL 05127 1.3 C CM2 A/B B MIL 05128 1.4 B/C L5 0.9MIL 05129 CE LL6 B A/B 1–20 B MIL 05130 2.7 L6 2 BMIL 05131 C LL6 BMIL 05132 0.8 L6 B/CMIL 05133 5.2 C L6 2.6 A/B B C L6 B 20 0.8 LL5 A/B 0–32 3.5 C A/B B/C B 1.9 17 2.8 C B A/B 12.5 A/B A/B 4.7 A B 1–20 17.4 B/C A 4.6 C 32 A B B A/B 28 24 ANSMET seasons. Table 3. 1686 H. C. Connolly, Jr., et al. Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameRBT 04124RBT 04125RBT 04126 H6 Class RBT 04128 LL5 RBT 04129 L5 RBT 04134 L5 RBT 04135 LL5 RBT 04136 L5 RBT 04137 297.4 L6 375.4RBT 04138 LL5 C 1348.2 A/BRBT 04139 H4 1104.8 CRBT 04140 L5 1140 B B B/CRBT 04141 L5 RBT 04142 B 277.3 L6 B A/BE RBT 04144 245.5 H5 C 217.4RBT 04145 H6 B C BRBT 04146 235.2 H6 B RBT 04147 219.7 H6 C B RBT 04148 A/B 141.4 H6 CRBT 04149 L6 C B 35.3RBT 04150 126 H6 B CRBT 04151 101.4 H6 B CRBT 04152 192.7 H5 CRBT 04153 B/C H6 C 47.3RBT 04154 130.7 B H6 B/C CRBT 04155 126.6 L5 C A/B RBT 04156 124.1 H5 C B RBT 04157 H6 C 94.7 B RBT 04158 H6 27.5 A/B CERBT 04159 120 H5 A/B CRBT 04160 151.9 LL6 C CRBT 04161 H6 C 86.1 B RBT 04162 103.8 H6 B/CRBT 04163 103.6 B H5 C B RBT 04164 100.2 Iron-ung C B RBT 04165 H5 C 62.6 B RBT 04166 86.4 H6 B CRBT 04167 H6 B/C 61.9 B RBT 04168 LL6 60 C B 52.3 B RBT 04169 H5 57.1RBT 04170 H6 C C B RBT 04171 H6 35.6RBT 04172 LL5 11.9 A/B C A/B RBT 04173 H5 14.4 CRBT 04174 11.1 H5 C B L5 C 23.5 C L5 11.3 C B A/B C 9.1 71.3 B C 170.3 B A/B 141.6 C B/C A/B A/B 99.6 110.5 A/B B/C A/B C A/B A/B Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NamePRA 04410PRA 04411PRA 04412 LL5 Class PRA 04413 LL5 PRA 04415 L6 PRA 04416 L5 PRA 04417 LL6 PRA 04418 LL5 278.6PRA 04419 LL5 170.6 BPRA 04420 L5 B/CPRA 04421 LL6 82.8PRA 04422 A L6 A/B 84.6 106.8 CRoberts Massif (RBT) L5 B BRBT 03520 69.8 LL6 RBT 03521 B 87.5 B/CRBT 03524 A A/B LL6 B 36.7 B RBT 03525 62.9 LL5 B/CRBT 03526 H6 B B 21.6RBT 03527 L5 B 5060 25.7 CRBT 03528 H5 A CRBT 03529 A L5 1327.7RBT 04100 B LL6 1378 A/BRBT 04101 B H5 A A/B RBT 04102 A 182.6 L6 RBT 04103 299.7 L5 CRBT 04104 269 L5 A A/BRBT 04105 142.3 H5 A A/B CRBT 04106 78.3 LL5 BRBT 04107 128.5 L5 B 2609RBT 04108 A L4 C B 1918.6RBT 04109 LL5 A/B C 1328.4 CRBT 04110 L6 B B/CRBT 04111 184.9 LL6 204.8 B RBT 04112 LL6 B/C C A/B A/BRBT 04113 298.2 H6 RBT 04114 292.4 LL5 A/B C A/B 522.9RBT 04115 L6 C BRBT 04116 386.1 L3 B 198.9RBT 04117 LL5 29 B/C C 172.1 BRBT 04118 A/B LL6 B/C B RBT 04119 273.6 t H5 t 204.3 24 RBT 04120 B LL5 C C BRBT 04121 383.2 H5 RBT 04122 281.6 L5 1456.3 C A/B RBT 04123 A/B L5 1142.9 B/C B H5 A/B C A/B 965.3 H6 985.5 A/B A/B C A/B 945.5 1–29 766.4 C B A/B 495.4 C 3–18 302.1 B C 367.7 B/C A C A C A/B ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1687 Fs (mol%) Info Fa (mol%) Fracturing b Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 Continued. NameRBT 04220RBT 04221RBT 04222 H5 Class RBT 04223 H5 RBT 04224 L5 RBT 04225 L5 RBT 04226 LL5 RBT 04227 H6 RBT 04228 H5 66.8RBT 04229 L6 57.3 CRBT 04230 Acp 64 CRBT 04231 H5 28.4 B RBT 04232 44.8 L5 B B B RBT 04233 LL6 C 34.1RBT 04234 H5 29 A/B CRBT 04235 B L5 B 57.3RBT 04236 H6 C 19.8 B A/B RBT 04237 H6 75.1 CRBT 04238 LL5 B 68.9 CRBT 04239 A/B 11.1 L5 C CRBT 04241 L5 B 9.3 B RBT 04242 Achon-ung 20.3RBT 04243 A/B C L6 16.3 A/B CRBT 04244 L5 8 C 8.5RBT 04245 13.8 H5 A/B RBT 04246 B C 12 LL6 A 40.9 B RBT 04247 L5 10 10.1 C CRBT 04248 LL5 C A CRBT 04249 H5 86.7RBT 04250 B A/B L5 54.6 B/CRBT 04252 C L5 41.4 B/CRBT 04253 73.5 L5 A B/CRBT 04254 24 L5 A/B B/C 34RBT 04256 28.1 A/B L5 A RBT 04257 L5 A/B B/C 44.2 20 RBT 04258 L5 35.6 A B/C RBT 04259 L5 25.2 B/CRBT 04260 L5 B/CRBT 04261 7.9 LL6 A/B 32.7RBT 04262 C CM2 B/C 47 BRBT 04270 Martian 54.9RBT 04271 Martian C B 34.7 CRBT 04272 A/B L6 34.1 CRBT 04273 L5 B CRBT 04274 7.6 B L5 4.5 86.3 B 78.8 C H5 B/C 204.6 CE B L5 B B B B C 370.6 B 341.8 B C 400.5 B/C 257.1 B/C 0–1 A/B B/C 431.1 C 39 B 38–40 C 1 16–32 B 20–27 B Table 3. Table ANSMET seasons. Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameRBT 04175RBT 04176RBT 04177 L5 Class RBT 04178 L5 RBT 04179 L6 RBT 04180 H6 RBT 04181 L5 RBT 04182 H6 RBT 04183 LL5 61.2RBT 04184 H6 22.1 B/CRBT 04185 H6 42.6 B/CRBT 04186 H5 A/B 27.4 BRBT 04187 LL5 A/B 19.8 CRBT 04188 Iron-IIE (?) 19.7 CRBT 04189 B L5 3.1 C A/B RBT 04190 LL6 20 BRBT 04191 A/B H5 12 B RBT 04192 L6 C 4.6 11.5 B RBT 04193 L5 C 7.7 CRBT 04194 L5 B BRBT 04195 L5 B B RBT 04196 5.1 10.3 L5 A/B RBT 04197 C L5 B 11.6RBT 04198 191.5 L5 CRBT 04199 L5 B A/B B 69RBT 04200 L5 28.5 18–20 B RBT 04201 L5 C 85 B CRBT 04202 16–19 123.9 H6 RBT 04203 162 L5 C B A/B RBT 04204 B/C H5 93.3 CRBT 04205 LL6 39.9 A/B A/B A/BRBT 04206 H6 77.9 CRBT 04207 H5 A/B A 38.3 BRBT 04208 L5 31.3 CRBT 04209 B H5 12.2 CRBT 04210 A/B H6 14.8 CRBT 04211 B 17.8 LL6 C A/B RBT 04212 H4 B 13.3RBT 04213 B H5 12.4 C C RBT 04214 H6 C 12.8 CRBT 04215 L5 38.2 C B RBT 04216 H5 C 1.1 B RBT 04217 H5 2.2RBT 04218 A/B C 133.5 L5 C A/B RBT 04219 182.7 L5 A/B 136.1 L5 C B/C A/B A/B 127.9 L5 C B 73.9 A/B 111.8 C C 18 C 86.5 A 187.3 C C 118.9 16 C C C 69.2 B/C B/C C A/B B ANSMET seasons. Table 3. 1688 H. C. Connolly, Jr., et al. Fs (mol%) Info crust chondrite; How = her abbreviations can be Fa (mol%) Fracturing ; Ang = angrite; Achon-ung achondrite, b impact melt; Imr = impact-melt rock; Mes Euc = eucrite; FC fusion hondrite; Ure = ureilite. Ot Mass (g) WG a A list of all meteorites approved from the 2003 to 2005 to classification): Acp = acapulcoite Continued. ungrouped; Bra = brachinite; Dio diogenite; howardite; Iron-ung = iron ungrouped; IM-Im mesosiderite; Pal = pallasite; PrA primitive ac found on the JSC Curation Web page. found on the JSC Curation Web t = thawed. WG = weathering grade. NameSAN 03472SAN 03473SAN 03474 How Class SAN 03475 DioSAN 03476 L5 SAN 03477 L5 SAN 03478 L5 SAN 03479 L5 195.2 Glacier (TYR) Taylor LL5 BTYR 05180 125.4 LL5 224.5 B/C A/B 179.8 L5 BE A 145.6 B/C A/B 108 BE 107.2 A BE B/C 58.7 A/B 22 B/C A/B A/B 244.2 20–52 A/B 2 B/C A/B For class (which refers Table 3. Table ANSMET seasons. a b Fs (mol%) Info Fa (mol%) Fracturing pproved from the 2003 to 2005 b Mass (g) WG a A list of all meteorites a Continued. NameRBT 04275RBT 04276RBT 04277 L5 Class RBT 04279 H6 RBT 04280 H5 RBT 04281 H5 RBT 04282 L5 RBT 04283 H5 RBT 04284 712.2 L5 RBT 04285 189.7 LL5 B/CRBT 04286 326.9 LL5 C B RBT 04287 195 L6 B/CRBT 04288 225.7 H6 B B B/CRBT 04289 138.4 H5 CRBT 04290 144.9 H5 C B 119.6RBT 04291 H5 C B 102.8 BRBT 04292 H5 B B/CRBT 04293 L5 83.2 B RBT 04294 B/C L5 B 67.8 CRBT 04295 L5 37.8 CRBT 04296 L5 45 CRBT 04297 B L5 43.1 B RBT 04298 L5 C 25.6 C B RBT 04299 L5 54.2 BRBT 04300 LL5 B 32.3 C B RBT 04301 Iron-ung 72.2 C B RBT 04302 L5 59.3 CRBT 04303 B L5 70.3 CRBT 04304 B CV3 52.9 CRBT 04305 A/B L5 77.5 B/C 55.2 RBT 04306 B 44 L5 CRBT 04307 A/B L5 A/B BERBT 04308 L6 RBT 04309 3.1 B L5 B 11.6Sanford Cliffs (SAN) 9.1 C L5 SAN 03450 B C CM2 16.6SAN 03454 B CSAN 03457 8.5 L5 B B 14.7SAN 03464 C L5 11.8 CSAN 03465 B L5 CSAN 03466 8.1 L5 B SAN 03467 7.1 B/C A/B L5 1–9 1.3SAN 03470 B B/C L5 BE A 5168SAN 03471 L5 1 B 1346.8 L5 B B B 786.9 L5 919.1 B A/B 596.5 A BE 1–50 553.4 B B A/B 462.9 BE 224.1 B A/B A/B 237.4 B/CE BE A/B A/B A/B ANSMET seasons. Table 3. The Meteoritical Bulletin, No. 92 1689 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 with ALH 06001 Type Type specimen mass (g) Comments Type Type specimen mass (g) Info Comments 226.3 MNA-SI Likely paired ) χ xpedition. ) χ Magnetic sus (log 4.6 PRIC See separate entry Magnetic Magnetic sus (log Fs (mol%) 17.5 5.09 128.1 MNA-SI 20.6 ± 0.5 Fs (mol%) Fs Fa (mol%) 24.0 ± 0.4 Fa (mol%) No. of pieces Class SS WG 6 1 H~5 5.05 6 MNA-SI Likely paired 1.08 1 H~5 5.07 1.08 MNA-SI Likely paired 91 2 H5 S3 W1-2 18.7 17.8 5.07 91 MNA-SI Likely paired 61.7 1 H~5 5.07 61.7 MNA-SI Likely paired 28.6 1 H~5 5.08 28.6 MNA-SI Likely paired Total known mass (g) 128.1 1 H5 S3 W1-2 18.3 119.2 1 H~5 5.04 119.2 MNA-SI Likely paired 280.9 4226.3 1 H~5 H5 S3 W1-2 18.7 16.9 5.20 5.08 280.9 MNA-SI Likely paired No. of pieces Class SS WG 24.3 1 H~5 5.10 24.3paired MNA-SI Likely 25 1 H~5 5.07 25paired MNA-SI Likely 120 2 H~5 5.06 120 MNA-SIpaired Likely ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ Ricerche in Antartide (PNRA), the Italian government-sponsored e 96.7 1 L5 S6 W1 Fa Total known mass (g) 396.4 1 Mes PRIC See separate entry Longitude (E) 158°46.117 158°46.491 ′′ ′′ 158°46.439 158°50.583 158°47.570 158°46.703 158°46.703 158°46.552 158°46.550 158°46.516 158°46.717 158°46.716 ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ 8 6 ′ ′ 75°20 Longitude (E) 75°13 Latitude (S) ′′ ′′ red by the Chinese Antarctic Expedition. 23 36 ′ ′ Latitude (N) Date of recovery sification): Mes = mesosiderite. ice 15-Oct-2006 76°43.040 ice 15-Oct-2006 76°43.017 ice 15-Oct-2006 76°44.552 ice 15-Oct-2006 76°42.677 ice 15-Oct-2006ice 76°42.313 15-Oct-2006ice 76°42.313 15-Oct-2006ice 76°42.335 15-Oct-2006 76°42.331 ice 15-Oct-2006ice 76°42.331 15-Oct-2006 76°42.729 ice 15-Oct-2006ice 76°42.758 15-Oct-2006 76°42.753 Type of Type find site Date of recovery Grove Mountain Grove 052049GRV 16-Jan-2006 72°46 Name For class (which refers to clas GRV 055364GRV 9-Jan-2006 72°59 Name Allan Hills 06012 Blue Allan Hills 06001 Blue Allan Hills 06002 Blue Allan Hills 06003 Blue Allan Hills 06004 Blue Allan Hills 06005 Blue Allan Hills 06006 Blue Allan Hills 06007 Blue Allan Hills 06008 Blue Allan Hills 06009 Blue Allan Hills 06010 Blue Allan Hills 06011 Blue Table 4. A list of meteorites recovered by Programma Nazionale Table Table 5. A list of meteorites recove Table 1690 H. C. Connolly, Jr., et al. ) Comments χ 130 × 12 mm). Thin, light Magnetic sus (log ion halo extends ~1 cm out from inent worm burrows in plate. One Wo mol% agonal limestone plate (about 100 × 80 10 Fs mol% limestone plate (165 × Fa mol% 50 mm). Light gray reduction halo (total cross section including meteorite: 135 × mm) around dark gray depression from which most of the meteorite has weathered out. This stone a synonym Österplana 001. gray reduction halo (75 × 75 mm). worm track follows closely outer rim of reduction halo. In the plate there is also a perfectly round white circle of calcite from vertically positioned nautiloid shell. × 110 × 18 (height) 17 mm). Plate cut diagonally through center of × 110 meteorite. Central part of meteorite bluish-greenish, surrounded by rusty red cm-thick zone. Light reduct meteorite. prom duction halo (52 × 54 mm). Two Type specimen mass (g) SS WG No. of pieces Class 12.92 1 Ure 2.6 separate entry See 665 1 H5 359 6 3 19.4 ± 0.4 17.1 ± 0.2 4.45 See separate entry 17,960 64 CH3 20.1 separate entry See Total Total known mass (g) ′ ′ 45 × 30 LundU-1 meteorite contained in red limestone plate (98 × 80 Weathered 45 × >25 >15 LundU-1pent red in meteorite Dark 50 × 52 LundU-1 meteorite in red limestone plate (127 × 175 31 mm). Light re- Dark Approximate sizes (cross sections in mm) Info Comments ′ 55 × > 13 LundU-1red in meteorite Dark ′ ′ ′ ′ 54°49.126 54°49.126 99°49 Longitude (E) Latitude (E) 13°26 13°26 13°26 13°26 ′′ ′ 31.6 ′ ′ ′ ′ ′ ′ Latitude (N) Longitude (N) Find 19°6.771 Find/ fall 2004 Find 21°04 17 January 2001 20062006 Find2006 Find2006 Find2005 Find2005 Find Find2006 145 Find 1 40°16 54 56 1 Dio 31 1 21 Euc 146 1 Dio 10.8 1 67 Dio 11.2 1 Euc 7 21 Euc 13.5 See separate entry See separate entry See separate entry See separate entry See separate entry See separate entry Date of recovery or purchase Date of recovery relict meteorites from Sweden. cation): Dio = diogenite; Euc eucrite. Uhaymir region region Emirates Emirates Emirates Emirates Emirates Emirates Gansu Province Location of recovery Sayh al Uhaymir 290 Sayh al Oman Dhofar 1427 Dhofar Arabian Peninsula 002 United Arab Arabian Peninsula 003 United Arab Arabian Peninsula 004 United Arab Arabian Peninsula 005 United Arab Arabian Peninsula 006 United Arab China Weikengquan City, Jiuquan United Arab Emirates Arab United Arabian Peninsula 001 United Arab Name For class (which refers to classifi SS = shock stage. WG = weathering grade. NameÖsterplana Öst 001 Abbreviation Österplana 002 1987 002 Öst 10-Oct-1993 58°35 58°35 Österplana 003 003 Öst 8-Nov-1993 58°35 Österplana 004 004 Öst 6-Jan-1994 58°35 Table 6. A list of all approved meteorites from Asia. Table Table 7.Table A list of approved The Meteoritical Bulletin, No. 92 1691 of the plate. Chambers shell in front of a garage entrance and e 0.5 to 0.6 mm in diameter. Size e 0.5 to 0.6 mm in diameter. duction halos (85 × 85 mm). Worm duction halos (85 × 85 mm). Worm 12 and 190 × 160 mm). Nautiloid teorite in red limestone plate (215 × 237 tone plate (97 × 116 × 54 mm). Meteorite at tone plate (97 × 116 teorite in two large plates (each 480 × teorite in two large ped meteorite in red limestone plate (135 × haped meteorite with intense reduction halo. tical shape in two red limestone plates sawed ction halo (60 × 50 mm). × 22 mm) with worm burrows. Proportionally large (110 × 110 (110 × 22 mm) with worm burrows. Proportionally large mm), gray reduction halo. but diffuse 30 intense and distinct light orange-gray reduction halo (80 mm). Very × 80 mm). has been driven over by cars thousands of times. 30 mm). Surrounded by inner light orange reduction halo (210 × 200 mm) and an another outer darker red halo. Meteorite with halos looks like an eye, where the meteorite is pupil. meteorite mass is lost and mainly the depression of remains (~Öpl 001). The meteorite is Plate sizes are 160 × 100 27 mm and perpendicularly to the sea floor. 160 × 100 20 mm. edge of plate and sawed through both perpendicularly horizontally relative to the sea floor. 6 Meteorite has extraordinarily well preserved chondrule mm). structures. Chondrules are on averag of reduction halo 50 × 70 mm. (each 400 × 25 mm). Light re tracks along the rim of reduction halo. A particularly sharp-edged meteorite. meteorite in red limestone plate (215 × 165 30 mm). excellently displayed. Very intense light gray reduction halo (60 × excellently displayed. Very 60 of and in tracks along margin mm) around meteorite. Worm reduction halo. red limestone plates (190 × 150 shell extending along the whole long side of limestone plate. Plate cuts through shell. Redu 125 × 12 mm). Diffuse, but large gray reduction halo (70 × 60 mm). but large 125 × 12 mm). Diffuse, Dark meteorite in red limestone plate (95 × 145 12 mm). Thin, very intense orange-gray reduction halo (28 × 24 nautiloid shell mm). Large in plate (vertical cross section of two chambers). nautiloid shell limestone plate (400 × 250 34 mm) with large spanning almost diagonally across most 40 × 30 LundU-1 meteorite in red limestone plate (245 × 170 pear-shaped Dark 95 × 80; 80 LundU-140 × 18; 28 15me round very dark, Large LundU-1ellip with meteorite Dark 50 × 50 LundU-2 weathered, square-shaped meteorite with sharp edges. Most of Strongly 40 × 25 8 LundU-1limes red in meteorite Dark 35 × 2037 × 44; 32 57 LundU-1 LundU-1 meteorite in very small and thin red limestone plate (67 × 80 Dark red limestone plates dark, almost black meteorite in two large Very 58 × 2123 × 34 LundU-1 greenish and reddish elongate, “coprolite-shaped” gray, Distinctly LundU-1 teardrop shaped dark me Small about 10 × LundU-2 somewhat square-s Small Approximate sizes (cross sections in mm) Info Comments 25 × 32; 40 × 33 LundU-1 in two dark, almost black meteorite, somewhat triangular-shaped, Very 23 ×15 × >1122 × 15 LundU-120 × 27 Gray distinctly square-sha LundU-1 LundU-1 red dark, almost black squared to subrounded meteorite in large Very ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 Latitude (E) 13°26 13°26 13°26 13°26 13°26 ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ 58°35 Longitude (N) 5-May-1992; recovered in the 1960s Date of recovery A list of approved relict meteorites from Sweden. Continued. Österplana 014 014 Öst Österplana 015 015 Öst 11-Apr-1996 58°35 1-Jun-1996 58°35 Österplana 007 007 Öst Österplana 008 28-Dec-1993 008 Öst 58°35 5-May-1995 58°35 Österplana 006 006 Öst Identified Österplana 009 009 Öst 15-Jan-1996 58°35 Österplana 010 010 Öst Österplana 011 1995 011 Öst 31-Jan-1007 58°35 58°35 Österplana 012 012 Öst Österplana 013 013 Öst 10-Sep-1996 58°35 11-Mar-1996 58°35 NameÖsterplana 005 005 Öst Abbreviation 8-Feb-1990 58°35 Österplana 018 018 Öst 15-Jan-1996 58°35 Österplana 016 016 Öst Österplana 017 017 Öst 4-Aug-1996 58°35 15-May-1997 58°35 Table 7. Table 1692 H. C. Connolly, Jr., et al. gray to black imprints of the ate cut diagonally giving the plate plate. Thin, intense reduction halo plate. Intense reduction halos (70 ed chambers and siphuncle crosses greenish gray. In the two blocks greenish gray. th the enclosing red limestone. In and 660 × 400 30 mm). Plates with at triangular, but rounded corners, in red at triangular, shaped meteorite in red limestone steps of d” margins in red limestone plate (220 × d” margins ewhat bean- or kidney-shaped) meteorite in ry large red limestone plates (each 1200 × 700 ry large two gray limestone plates (each 315 × 30 mm). blocks there are imprints made by the meteorite. Some meteoritic material is left in these depressions. The loose meteorite has a compressed appearance; it is dark (each 230 × 260 30 mm) with dark meteorites there are also large gray reduction halos. meteorites there are also large limestone plate (385 × 200 × 22 mm). Comparatively large, but diffuse but diffuse limestone plate (385 × 200 22 mm). Comparatively large, reduction halo (90 × 90 mm). Halo changes color from gray to reddish burrows in reduction halo. Worm gray. Dark meteorite with shape similar to Indian subcontinent in two red limestone plates (415 × 355 30 very intense red and orange colors, prominent reduction halo (about 110 × 110 mm). Intense reduction halo (50 × 60 mm). Two very large nautiloid shells very large Intense reduction halo (50 × 60 mm). Two (560 and 350 mm) in plate. One only about 100 mm from meteorite. plate (570 × 740 30 nautiloid shells in plate. Thin, large mm). Two mm). intense reduction halo (15 × 11 polished) (130 × 90 mm). Prominent light gray reduction halo (60 50 mm). (~110 × 110 × 23 mm). One side of pl × 110 (~110 a somewhat triangular appearance (but still four corners). Intense, like, reduction halo (50 × 50 mm). solar-corona × 24 mm). Many nautiloid shells on × 60 mm). (35 × 30 mm). 170 × 12 mm). Meteorite in corner of the garden of Gunnebo castle. Meteorite is presently weathering at a fast rate. 12 mm and 520 × 300 13 mm). In one plate excellently preserved long nautiloid shell with perfectly expos imprint of the In second plate more diffuse plate almost diagonally. imprints also of other shells in the two plates. Mete- same shell. Weak plates. orite occurs in one of the corners large LundU-1 Loose meteorite and two blocks wi 80 × 124; 124 LundU-1(som rounded black Large 80 × 50 20; 50; 80 × 50 30 × 20 LundU-1somewh shape meteorite, Gray 60 × 55; 50 70 LundU-1 50 × 30 LundU-1 × 735 18). red limestone plate (1115 Dark meteorite in very large 11 × 711 LundU-1 red limestone small dark meteorite in proportionally very large Very 40 × 35; 50 30 LundU-1ve two in meteorite Dark 25 × 15 LundU-1 Dark elongate meteorite in rough red limestone block (not sawed or about 12 × 25 LundU-1square to subrounded Gray, 18 × LundU-1 Dark meteorite with five subrounded corners in red limestone plate 25 × 17 LundU-1 Dark meteorite with “rugge 35 × 20; 40 65 LundU-1 red limestone plates (500 × 300 dark meteorite in two large Large Approximate sizes (cross sections in mm) Info Comments ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 Latitude (E) ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ Longitude (N) Date of recovery A list of approved relict meteorites from Sweden. Continued. Österplana 030 Öst 030 8-Apr-1994 58°35 Österplana 029 Öst 029 2-Oct-1998 58°35 Österplana 028 Öst 028 11-Sep-2000 58°35 Österplana 027 Öst 027 29-Mar-2000 58°35 Österplana 026 Öst 026 17-Mar-2000 58°35 Österplana 025 Öst 025 29-Mar-2000 58°35 Österplana 023 Öst 023 2-Dec-1999 58°35 Österplana 024 Öst 024 2-Dec-1999 58°35 Österplana 021 Öst 021 15-Jun-1997 58°35 Österplana 022 Öst 022 27-Nov-1999 58°35 Österplana 020 Öst 020 10-Jun-1997 58°35 NameÖsterplana 019 Öst 019 Abbreviation 15-Apr-1997 58°35 Table 7. Table The Meteoritical Bulletin, No. 92 1693 part of the Sextummen bed, oor. Meteorite has fish-like shape. oor. ccurs in two gray limestone blocks not sawed) rock surface, other sides t worm tracks around meteorite. original meteorite also preserved. and 320 × 110 × 31 mm). Only a part and 320 × 110 rfect fossil meteorite found by 2006. perfectly preserved chondrule of red limestone (195 × 290 31; 195 tone block (115 × 135 65tone block (115 mm). Meteorite- e in red limestone plate (150 × 130 25 mm). most like opal) in two gray limestone plates ite in red limestone plate (205 × 230 meteorite in two gray limestone plates (300 × meteorite at crack surface in two red limestone exposing side of block is a raw (i.e., sawed. Prominent gray reduction halo (80 × 80 mm). 100 mm). 280 mm). Gray reduction halo (120 × 120 mm). Meteorite at margin of plate and sawed through both the vertical Meteorite at margin mm). × 110 reduction halo (110 diffuse horizontal directions. Large Strongly weathered, brownish meteorite in two red limestone blocks Strongly gray reduction large (460 × 220 50 and 470 mm). Very halo (230 × 160 mm). From the lowest s.k. Måcka bed. blocks/plates (300 × 110 × 31 mm blocks/plates (300 × 110 of the two of the meteorite is preserved and it occurs at margin blocks. Perhaps the most beautiful and pe A large rounded meteorite, with A large structures almost throughout the entire exposed meteorite surface. of an extraneous clast in Structure × 300 30 and 195 mm). One plate contains a not-so-nice of the meteorite. The two other plates contain cut through the margin the excellent cuts and texturally preserved surfaces through meteorite. The upper and lower part of a nautiloid shell is exposed on each of these two plates. Prominen Outer parts of meteorite have flaky appearance. Meteorite occurs in three plates plates (each 165 × 145 30 mm) with the characteristic reddish gray color of the Flora bed. 290 × 40 and 400 30 mm). Prominent fresh cracks through the meteorite part on the smaller plate. (each 730 × 180 65 mm). The saw has cut the blocks and meteorite perpendicularly relative to the sea fl Well displayed hardgrounds in blocks. One prominent hardground a Well few centimeters below meteorite. Meteorite itself not on hardground but has sunk into the originally soft sediment. (160 × 80 × 60 and 160 × 90 × 50 mm). The larger meteorite part on one (160 × 80 60 and 160 90 50 mm). The larger plate has three very sharp corners, like a triangle, but the “hypotenuse” is curved. The other smaller part on a separate plate represents cut of the meteorite. The shape this meteorite part is through the margin part: two areas, one round, trian- from the larger entirely different gular connected by a thin bridge. LundU-1 LundU-1 meteorite found by 2006. O Largest 20 × 15 LundU-1limes red in meteorite Dark 30 × 14 LundU-1 Small lip-shaped meteor 35 × 32 LundU-1 weathered brown meteorite in limestone block (300 × 280 Strongly 40 × 20 18 LundU-1meteorit brown rust Dark, 60 × 45; 50 LundU-1 65 × 44; 44 LundU-1“ugly” weathered, Dark 80 × 60 15; 85 × 70 30; 42 × 40 ×31 20 × 25; 16 26 LundU-1limestone two in meteorite square-shaped vaguely black, to gray Dark 50 × 25; 65 35 LundU-1rounded elliptical, Dark 210 × 65 41; 210 × 65 50 50 × 50; 65 45 LundU-1 Black meteorite (looks al Approximate sizes (cross sections in mm) Info Comments ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 13°26 Latitude (E) ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′ Longitude (N) Date of recovery A list of approved relict meteorites from Sweden. Continued. Österplana 041 Öst 041 1996 58°35 Österplana 040 Öst 040 10-Jun-2000 58°35 Österplana 039 Öst 039 11-Sep-2000 58°35 Österplana 038 Öst 038 15-Jun-1999 58°35 Österplana 037 Öst 037 2-Oct-1998 58°35 Österplana 036 Öst 036 24-Oct-1996 58°35 Österplana 035 Öst 035 20-Mar-1996 58°35 Österplana 034 Öst 034 2-Nov-1998 58°35 Österplana 033 Öst 033 12-Oct-2000 58°35 Österplana 032 Öst 032 11-Sep-2000 58°35 NameÖsterplana 031 Öst 031 Abbreviation 15-Sep-1998 58°35 Table 7. Table 1694 H. C. Connolly, Jr., et al. is not sawed, but exposed on a orite has somewhat rectangular meteorite in dark red limestone block two red Orthoceratite limestone blocks. tone block (170 × 130 48 mm). Meteorite- ay limestone plates (106 × 136 29 and 106 Surrounded by 5 cm reduction halo. 136 × 54 mm). Meteorite sawed in perpendicular direction relative to Orthoceratite shell (vertical cut) at the side above meteorite. sea floor. reduction halo (40 × 34 mm). Mete appearance, with two sharp corners on one of the short sides, but opposing side has rounded corners. exposed surface not sawed, but sides of block are sawed. Prominent gray reduction halo (90 × 70 mm). Medium-sized meteorite with very rusty appearance in red limestone × 85 55 mm). Some sides of block sawed, others rough block (115 rock surfaces. Meteorite sawed through both in vertical and horizontal directions. rough rock surface. Prominent gray reduction halo (120 × 130 mm). (280 × 300 80 mm). The meteorite 12 mm LundU-3 Almost round gray structure in 37 × 27; 31 20 LundU-1gr two in meteorite Dark 20 × 13 LundU-1 mm). Intense light Dark meteorite in red limestone plate (91 × 60 11 35 × 20 LundU-1limes red in meteorite Dark 50 × 40 LundU-1 15 × LundU-1 Small dark meteorite in red limestone plate (230 × 200 28 mm). 35 × 30 LundU-1round brown-weathered Strongly Approximate sizes (cross sections in mm) Info Comments ′ ′ ′ ′ ′ ′ ′ 13°48 13°26 13°26 13°26 13°26 13°26 13°26 Latitude (E) ′ ′ ′ ′ ′ ′ ′ Longitude (N) Date of recovery A list of approved relict meteorites from Sweden. Continued. Gullhögen 001 Gul 001 14-Jun-2000 58°23 Österplana 047 Öst 047 21-Nov-2002 58°35 Österplana 046 Öst 046 5-May-2002 58°35 Österplana 045 Öst 045 7-May-2002 58°35 Österplana 044 Öst 044 17-Mar-2002 58°35 Österplana 043 Öst 043 17-Feb-2002 58°35 NameÖsterplana 042 Öst 042 Abbreviation 11-Sep-2000 58°35 Table 7. Table