The Meteoritical Bulletin, No. 92, 2007 September · Dar al Gani 1048 27°12.10 ... NMBE by M. Ould...

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1647 © The Meteoritical Society, 2007. Printed in USA. 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 SMITH 4 , Gretchen BENEDIX 4 , Luigi FOLCO 5 , Kevin RIGHTER 6 , Jutta ZIPFEL 7 , Akira YAMAGUCHI 8 , and Hasnaa CHENNAOUI AOUDJEHANE 9 1 Department 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 2 Department of Earth and Planetary Science, American Museum of Natural History, Central Park West, New York, New York 10024, USA 3 Lunar and Planetary Laboratory, Department of Planetary Sciences, The University of Arizona, Tucson, Arizona 85721, USA 4 Department of Mineralogy, The Natural History Museum, Cromwell Road, London SW7 5BD, UK 5 Museo Nazionale Antartide, Via Laterina 8, I-53100 Siena, Italy 6 Code ST, NASA Johnson Space Center, Houston, Texas 77058, USA 7 Sektion Meteoritenforschung, Forschungsinstitut und Naturmuseum Senckenberg, Senckenberganlage 25, D-60325, Frankfurt am Main, Germany 8 Antarctic Meteorite Research Center, National Institute of Polar Research, 1-9-10 Kaga, Itabashi, Tokyo 173-8515, Japan 9 Université 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 Libya Dar al Gani 1048 27°12.10N, 16°18.67E Libya Find: June 28, 2001 Achondrite (lunar, feldspathic breccia) History: A tiny complete individual stone was recovered by an anonymous finder in June 2001 and purchased by N. Classen in 2003 in Vienna, Austria. Physical characteristics: A single 0.801 g medium gray stone with some diffuse whitish clasts. About 70% of the stone is covered by fusion crust. Petrography: (A. Irving and S. Kuehner, UWS) Predominantly very fine-grained mineral debris with some larger lithic clasts (up to 0.3 mm) and vesicular glassy matrix and veins. Minerals identified include pyroxene, plagioclase, olivine, ilmenite, kamacite, and troilite. Lithic clasts include gabbro (composed of plagioclase and pigeonite) and very fine grained, ophitic-textured basalt (composed of plagioclase and olivine with accessory orthopyroxene, troilite, metal, and rutile). Several glassy spheres were found. Geochemistry: Olivine (Fa 19.6–49.6 , FeO/MnO = 93–98), pigeonite (Fs 20.2–61.9 Wo 5.3–7.2 , FeO/MnO = 54.8–66.5), and plagioclase (An 97–98 Or 0 ). Classification: Achondrite (lunar, feldspathic breccia). This stone is likely paired with Dar al Gani 262 and Dar al Gani 996. Type specimens: A total of 0.33 g of sample is on deposit at UWS. Classen holds the main mass.

Transcript of The Meteoritical Bulletin, No. 92, 2007 September · Dar al Gani 1048 27°12.10 ... NMBE by M. Ould...

1647 © The Meteoritical Society, 2007. Printed in USA.

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, USA3Lunar 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, UK5Museo Nazionale Antartide, Via Laterina 8, I-53100 Siena, Italy

6Code ST, NASA Johnson Space Center, Houston, Texas 77058, USA7Sektion Meteoritenforschung, Forschungsinstitut und Naturmuseum Senckenberg,

Senckenberganlage 25, D-60325, Frankfurt am Main, Germany8Antarctic Meteorite Research Center, National Institute of Polar Research, 1-9-10 Kaga, Itabashi, Tokyo 173-8515, Japan9Université 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 (fromANSMET, PNRA, and PRIC expeditions), and 7 from Asia. The Meteoritical Bulletin announcesthe approval of four new names series by the Nomenclature Committee of the MeteoriticalSociety, 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 enstatitechondrites and aubrites. Approved are two falls from Africa, Bassikounou (Mauritania) andGashua (Nigeria). Approved from areas other than Antarctica are one lunar, two Martian, 32other achondrites, three mesosiderites, two pallasites, one CM, two CK, one CR2, two CV3, oneCR2, and four R chondrites. The Nomenclature Committee of the Meteoritical Society announces48 newly approved relict meteorites from two new name series, Österplana and Gullhögen (bothfrom Sweden).

AFRICA

Libya

Dar al Gani 1048 27°12.10′N, 16°18.67′ELibyaFind: June 28, 2001Achondrite (lunar, feldspathic breccia)

History: A tiny complete individual stone was recovered byan anonymous finder in June 2001 and purchased byN. Classen in 2003 in Vienna, Austria.Physical characteristics: A single 0.801 g medium graystone with some diffuse whitish clasts. About 70% of thestone is covered by fusion crust.Petrography: (A. Irving and S. Kuehner, UWS)Predominantly very fine-grained mineral debris with some

larger lithic clasts (up to 0.3 mm) and vesicular glassymatrix and veins. Minerals identified include pyroxene,plagioclase, olivine, ilmenite, kamacite, and troilite. Lithicclasts include gabbro (composed of plagioclase andpigeonite) and very fine grained, ophitic-textured basalt(composed of plagioclase and olivine with accessoryorthopyroxene, troilite, metal, and rutile). Several glassyspheres were found.Geochemistry: Olivine (Fa19.6–49.6, FeO/MnO = 93–98),pigeonite (Fs20.2–61.9Wo5.3–7.2, FeO/MnO = 54.8–66.5), andplagioclase (An97–98Or0).Classification: Achondrite (lunar, feldspathic breccia). Thisstone is likely paired with Dar al Gani 262 and Dar al Gani996.Type specimens: A total of 0.33 g of sample is on deposit atUWS. Classen holds the main mass.

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Mauritania

Bassikounou 15°47′N, 5°54′WBassikounou, Hodh Ech Chargui, MauritaniaFall: 16 October 2006, 04:00 UTCOrdinary chondrite (H5)

History: A fireball was witnessed in the area, but no recordsof the direction of movement were recorded. A single stone of3165 g was found by A. Salem El Moichine, a local resident,on the same day at 13:00 h local time, 11 km SE ofBassikounou. The sample for classification was provided toNMBE by M. Ould Mounir, Nouakchott, who obtained itfrom his cousin who recovered the meteorite. According toS. Buhl (Hamburg, Germany), more than 20 specimens werelater recovered by locals and meteorite finders. These findsdefine an 8 km long strewn field. The total recovered mass is46.00 kg. Physical characteristics: The 3165 g specimen is largelycovered by black fusion crust. The interior is light gray. Onthe surface of the fusion crust there is some adherent soilmaterial, some of which is bright red. Shortly after recovery,the stone was cut into two pieces of 1200 and 1950 g. Thelarger piece has a rectangular shape and shows indications offlow lines in the fusion crust.Petrography: (E. Gnos, MHNGE; B. Hofmann, NMBE,M. Eggimann, Bern/NMBE): Mean chondrule size0.35 mm (n = 53). Metal abundance is 8 vol%, troilite6.6 vol%. Mean plagioclase grain size is ~20 μm. Troiliteis polycrystalline, rich in silicate inclusions, and showsdiffuse boundaries to metal. Metal is partly rich insilicate and troilite inclusions. Rare metallic Cu (10 μm)occurs at kamacite-taenite boundaries and in troilite.Some shock veins and no weathering products wereobserved.Mineral compositions: Olivine (Fa18.6), pyroxene (Fs16.3Wo1.1), and plagioclase (An13.7).Cosmogenic radionuclides: (P. Weber, PPGUN) Gamma-spectroscopy performed in December 2006 and January 2007showed the presence of the following radionuclides: 48V, 46Sc,56Co, 54Mn, 58Co, 7Be, 51Cr, 57Co, 22Na, 26Al, and 60Co.Recalculated to 12 October 2006 22Na was 38.0 ± 2.2 and26Al 31.5 ± 2.1 (both dpm/kg), the activity ratio of 1.21 isfully consistent with a fall on that date.Classification: Ordinary chondrite (H5); S2, W0.Type specimens: A total of 115 g are on deposit at NMBE.Boudreaux holds the main mass.

Morocco

The Meteoritical Bulletin announces a new name seriesapproved by the Nomenclature Committee of the MeteoriticalSociety from a dense collection area near Al Haggounia,Morocco (Chennaoui et al. 2007), comprising approximately3 tons of material. It should be noted that the classification of

samples potentially from this area varies, ranging from EL3chondrite to aubrite.

Al Haggounia 001 27°30′N, 12°30′WAl Haggounia, MoroccoFind: 2006Achondrite (aubrite)

History: Several tons of this material have been found onthe ground or by digging near Al Haggounia, Morocco(see Chennaoui et al. 2007 for description of the strewnfield), and sold to several dealers. The coordinates aregiven for the center of the strewn field, which extends~40 km.Physical characteristics: It is impossible to preciselyassess the amount of material already (and to be)recovered, but according to dealers, collectors, and Jambon,it is about 3 metric tons composing many samples of variedsizes (from a few g to 50 kg). The largest stones wererecovered after excavating them from the ground. The outersurface is rusty brown due to severe alteration and lookslike a sedimentary breccia cemented by iron oxide andcarbonate. Color changes from bluish gray to rusty brownclosest to the fractures are observed. Yellow patches ofsulfur (alteration) are widespread. The rocks aresignificantly porous, with pore sizes from severalcentimeters to hundreds of microns.Petrography: (A. Jambon, O. Boudouma, and D. Badia.UPVI) Dominated by enstatite and plagioclase. Troilite,graphite daubreelite, oldhamite, kamacite rich in Si, andschreibersite are present.Mineral compositions: Enstatite (En98Fs1Wo1) andplagioclase (Ab78An16Or5).Classification: Achondrite (aubrite); extensive weathering.Similar to and likely paired with NWA 002, 1067, 2736, 2828,2965. Type specimens: A total of 50 g of sample and three polishedsections are on deposit at UPVI. Main masses: Beroud, 3886 g (26 pieces from 1185 g to5.8 g); P. Thomas, 4497 g (33 pieces from 11 to 1507 g);Hmani, about 500 kg; Ouzrou, about 500 kg.

The Meteoritical Bulletin announces a new name seriesapproved by the Nomenclature Committee of theMeteoritical Society, Istifane, located in the Istifane region ofMorocco.

Istifane 001 31°29.911′N, 5°43.045′WMoroccoFind: 24 July 2005 Ordinary chondrite (H4)

Physical characteristics: It consists of three separate piecesof 68.0, 51.8, and 11.8 g, with a total mass of 131.6 g. Thethree pieces fit together documenting that they are fragmentsof a single stone.

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Petrography: (A. Ibhi and H. Nachit IZU, H. ChennaouiAoudjehane UHAC) It is severely weathered with a darkorange-brown color. Metallic Fe-Ni and/or troilite grains arefrequently replaced by iron oxide. Plagioclase grains are up to100 μm in size.Mineral compositions: Olivine (Fa18.4–19.2), orthopyroxene(Fs16.2–17.5). Classification: Ordinary chondrite (H4); S3, W4. Type specimens: Three polished thin sections and threefragments totalling 104 g are on deposit at IZU.

Istifane 002 31°29.909′N, 5°43.044′WMoroccoFind: 17 August 2005Ordinary chondrite (H5)

Physical characteristics: One 40 g stone, brownish in color.Mineral compositions: (A. Ibhi and H. Nachit IZU,H. Chennaoui Aoudjehane UHAC) Olivine (Fa15.5±0.5) andlow-Ca pyroxene (Fs16.8±0.6).Classification: Ordinary chondrite (H5); S5, W3. Type specimens: One thin section and the main mass are ondeposit at IZU.

Istifane 003 31°29.150′N, 5°43.027′WMoroccoFind: 17 August 2005 Ordinary chondrite (L5)

Physical characteristics: It is an 18.5 g stone partly coveredby dark-brown fusion crust.Mineral compositions: (A. Ibhi and H. Nachit IZU,H. Chennaoui Aoudjehane UHAC) Olivine (Fa24.9±0.7),orthopyroxene (Fs21.4±0.6), feldspar (An11Or6), high-Capyroxene (Fs10.6Wo41).Classification: Ordinary chondrite (L5); S3, W2. Type specimens: Three thin sections and three fragmentstotaling 10.4 g are on deposit at IZU.

Istifane 004 31°30.165′N, 5°42.916′WMoroccoFind: 19 May 2006 Ordinary chondrite (H5)

History: A. Ibhi and M. El Mansouri found this meteoritewhile prospecting with a metal detector.Physical characteristics: It is a 10.8 g stone.Petrography: (A. Ibhi and H. Nachit IZU, H.Chennaoui Aoudjehane UHAC) The meteorite isdominated by olivine and low-Ca pyroxene. Plagioclase,troilite, and metallic Fe-Ni are also noted as major andminor minerals.Mineral compositions: Olivine (Fa19.1±0.5), low-Ca pyroxene(Fs15.4±0.9), feldspar (An2.5±0.3).Classification: Ordinary chondrite (H5); S2, W2. Type specimens: One thin section and the main mass are ondeposit at IZU.

Nigeria

Gashua 12°51′N, 11°02′EDapchi, NigeriaFall: April 1984 Ordinary chondrite (L6)

History: The meteorite fall was reported by anonymouseyewitnesses to have occurred around April 1984 (about thetime of the nearby Gujba fall) near the tiny desert settlementKolomari close to the town of Gashua, Dapchi district,Nigeria. Physical characteristics: A single stone of 4162 g wasrecovered and broken by villagers into many pieces at theplace of the fall. The pieces were stored by villagers until theywere collected in 2005 and sent to E. Twelker. Petrography: (A. Greshake, NHB) The meteorite is a weaklyweathered ordinary chondrite with recrystallized texture andfew poorly defined chondrules. Opaque and ofteninterconnecting shock veins are present. Mineral compositions: Olivine (Fa23.8) and pyroxene (Fs20).Classification: Ordinary chondrite (L6); S4, W1. Type specimens: A total of 40.4 g plus one polished thinsection are on deposit at MNB. Twelker holds the main mass.

A list of all meteorites recognized from countries and regionsin Africa other than the northeast and the northwest isprovided in Table 1.

Northwest Africa

Northwest Africa 801MoroccoFind: 2001Carbonaceous chondrite (CR2)

History: M. Farmer and G. Hupé recovered a total ofapproximately 5 kg of many individuals and fragmentsfrom Zagora, Morocco. Many whole and sliced specimenshave been sold over the last several years.Physical characteristics: Many whole stones and fragments,all with desert varnish and brown/orange color. Numerouschondrules, many on the order of ~1 mm in apparentdiameter, are visible. Petrography: (G. Benedix and C. Smith, NHM) The thinsection studied is dominated by millimeter-sized type I POand POP chondrules, which are often rimmed with and/orcontain metallic Fe-Ni blebs. Metallic Fe-Ni also occurs asrounded, millimeter-sized grains within the matrix. Interstitialto chondrules and metal is a fine-grained matrix rich inphyllosilicate. Two type II chondrules were also observed.Pervasive veins of rust occur throughout.Mineral compositions: Type 1 chondrule olivine (Fo98.2±1.3),low-Ca pyroxene (En96.2±0.9Wo2.0±2.2), and high-Ca pyroxene(En45.7±11.5Wo35.9±4.7). Type II chondrule olivine (Fo77.4±7.7)and low-Ca pyroxene (En73.8±1.8Wo2.1±2.4).

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Classification: Carbonaceous chondrite (CR2); moderate toextensive weathering. Type specimens: A total of 77.4 g of sample and twosections are on deposit at NHM. Farmer holds severalgrams, KCCU holds approximately 10 g, and AMNH holdsseveral grams.

Northwest Africa 1461Algeria or MoroccoFind: March 2002Achondrite (diogenite)

History: D. Gregory purchased the 252 g stone in Erfoud,Morocco, in March 2002.Physical characteristics: A single pale gray-green, brokenstone.Petrography: (A. Irving and S. Kuehner, UWS): Coarse-grained (clasts up to 7 mm) with a partly cataclastic texture.Predominantly orthopyroxene (with diffuse grain boundaries)and accessory chromite. Minor calcite is present along somegrain boundaries.Mineral compositions and geochemistry: Orthopyroxene(Fs13.5–13.7Wo0.7–0.9; FeO/MnO = 32.0–33.8). This specimen isdistinctive in the magnesian pyroxene it exhibits. Oxygenisotopes: (D. Rumble, CIW) Replicate analyses by laserfluorination yielded δ18O = 3.177, 3.584; δ17O = 1.410, 1.634;Δ17O = −0.2609, −0.2505 (all ‰).Classification: Achondrite (diogenite).Type specimens: A total of 23 g of sample is on deposit atUCLA. One polished thin section and 1.3 g are on deposit atUWS. Gregory holds the main mass.

Northwest Africa 1924Morocco or AlgeriaFind: January 2001Carbonaceous chondrite (CV3)

History: Purchased in January 2001 in Erfoud, Morocco forD. Gregory. Physical characteristics: A single stone weighing 255 g. Petrography: (A. Irving and S. Kuehner, UWS) Separatedolivine-rich chondrules (mostly micro-porphyritic) andsparse CAI (containing Al-Ti-rich clinopyroxene, Fe-richspinel, and anorthite) in a dark, relatively magnetite-richmatrix. Olivine, Cr-bearing magnetite, ilmenite,intermediate plagioclase, orthopyroxene, clinopyroxene, andpentlandite. Geochemistry: Olivine (Fa29.1), Ti-rich pyroxene(Wo70.3Fs0.05) with TiO2 = 16.2, Al2O3 = 17.8 (both wt%).Oxygen isotopes: (D. Rumble, CIW) Laser fluorinationanalyses of two samples (all ‰) δ18O = −3.01, −3.61; δ17O= −6.46, −7.04; Δ17O = −4.879, −5.139. Classification: Carbonaceous chondrite (CV3); S1, minimalweathering. Specimens: A total of 20.4 g of sample and one polished thinsection are on deposit at UWS. Gregory holds the main mass.

Northwest Africa 2044Morocco or AlgeriaFind: August 2003Carbonaceous chondrite (CV3)

History: Purchased in 2003 August in Erfoud, Morocco, forD. Gregory. Physical characteristics: A single stone weighing 661 g. Petrography: (A. Irving and S. Kuehner, UWS) Sparse, well-formed ovoid chondrules in a black matrix. Olivine,orthopyroxene, clinopyroxene with accessory troilite andmetal. Sparse CAI consisting mainly of Mg-Al spinel,gehlenite and perovskite, with rims of Al-Ti-richclinopyroxene. Veins of anorthite present. Geochemistry: Mafic silicates are very Mg-rich (mg >97), metal (5 wt% Ni). Oxygen isotopes: (D. Rumble,CIW) Analyses of two whole rock fragments by laserfluorination gave δ18O = −1.12, −2.71; δ17O = −4.45,−6.36; Δ17O = −3.860, −4.934 (all ‰). Classification: Carbonaceous chondrite (CV3); S1, minimalweathering. Specimens: A total of 22.4 g of sample and one polished thinsection are on deposit at UWS. Gregory holds the main mass.

Northwest Africa 3157Morocco or AlgeriaFind: September 2004 Ordinary chondrite (Type 3)

History: Purchased from a Moroccan dealer at the DenverMineral Show by A. Hupé in September 2004.Physical characteristics: A single 51.7 g light brown stonelacking fusion crust and with abundant, large chondrules.Petrography: (A. Irving and S. Kuehner, UWS) Closelypacked PO and POP chondrules (mean diameter 1.0 mm);some are ovoid. The matrix is a “lacework” of porous olivineand pyroxene with accessory kamacite, taenite and troilite. Thecontent of metal (+minor Fe hydroxide) is very low (modedetermined by BSE imaging of a whole thin section is 1 vol%).Geochemistry: Olivine (Fa0–60); orthopyroxene(Fs0.5–30Wo1.5). Oxygen isotopes: (D. Rumble, CIW) Analysesof two acid-washed whole rock fragments by laserfluorination gave, respectively, δ18O = 5.30, 4.85; δ17O =3.48, 3.29; Δ17O = 0.693, 0.742 (all ‰). Although these Δ17Ovalues are within the range for H chondrites, this specimen ispoorer in metal than typical H chondrites.Classification: Ordinary chondrite (Type 3); S2, W1/2.Specimens: A total of 10.6 g of sample and one polished thinsection are on deposit at UWS. G. Hupé holds the main mass.

Northwest Africa 3221MoroccoFind: 2002Achondrite (ureilite, polymict)

History: B. Fectay purchased a single stone of 38.5 g inRissani, Morocco, in 2002.

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Physical characteristics: A fragment with 45% fresh blackfusion crust with a typical polymict ureilite texture.Petrography: (H. Takeda, Chiba and A. Yamaguchi, NIPR).The sample is a fragmental breccia with lithic clasts andsubrounded mineral fragments embedded in a cataclasticmatrix of predominantly ureilitic material. One large clast is afine-grained carbonaceous chondrite 2.3 × 1.5 mm in size andanother is very heavily shocked ureilite. Mineral fragmentsinclude olivine up to 1.8 × 1.2 mm, pyroxene, Na-richplagioclase, rare K, Na-rich glassy grain.Mineral compositions: Pyroxene (Fs8Wo8-Fs44Wo10-Fs13Wo34; Cr2O3 of pigeonite = 0.8–1.2 wt%; augite = 1.8 =2.0 wt%), olivine (Fo74–90; CaO = 0.25–0.47 wt%; Cr2O3 =0.42–0.83 wt% [cores]) and plagioclase (An6–60). High K, Na-rich glassy materials (SiO2 = 66.5, Al2O3 = 11.3, FeO = 8.5,Na2O = 4.2, K2O = 2.1 [all wt%] observed). Coexistence ofunshocked olivine and a very heavily shocked ureilite clast4.4 × 3.2 mm in size (PTS 090,8) as in Dar al Gani 1023 withgranoblastic texture. Clast olivines (Fo70–78 [cores]). Classification: Achondrite (ureilite, polymict). Type specimen: A total of 7.7 g of sample and a thin sectionare on deposit at NIPR. Fectay hold the main mass.

Northwest Africa 3222MoroccoFind: 2000Achondrite (ureilite, monomict)

History: An anonymous finder recovered 79 g.Physical characteristics: A flattened individual stone withsandblasted crust on 80% of the surface.Petrography and mineral compositions: (H. Takeda, Chibaand A. Yamaguchi, NIPR). The texture shows slightlyrounded angular fragments (up to 2.5 × 1.2 mm) of olivine(Fo87–89 [cores]; Fo92–96[rims]) in a comminuted matrix.Small rounded to oval orthopyroxene (Fs11.2Wo4.8) and augite(Fs7Wo37) grains are poikilitically enclosed in olivinecrystals. Carbonaceous material with iron oxide-hydroxideoccur as narrower, intergranular veins in a crystalline clast (4× 4 mm). The olivine grains in this clast show mosaicism withtilt boundaries, but the olivine fragments in the breccia matrixare not shocked. This meteorite contains mostly olivine withminor inclusions of orthopyroxene and augite. Many olivinefragments in the matrix do not contain carbonaceous veins.Classification: Achondrite (ureilite, monomict); S2,moderate weathering.Type specimen: A total of 15.8 g of sample and one thinsection are on deposit at NIPR. Fectay hold the main mass.

Northwest Africa 3223MoroccoFind: 2002Achondrite (ureilite, polymict)

History: An anonymous finder recovered a single stone of51 g.

Physical characteristics: The sample is a subrounded stonewith 60% fusion crust and soft when cut.Petrography and mineral compositions: (H. Takeda, Chibaand A. Yamaguchi, NIPR). It is composed of medium tocoarse (up to 1.6 × 1.2 mm in size) olivine (Fo77–80, CaO =0.3–0.4; Cr2O3 = 0.65–0.9 [both wt%; cores]) and pigeonitegrains (Fs18.0Wo7.5; Cr2O3 = 1.1–1.3 wt%). Carbonaceousveins typical of ureilites are observed at parts of the thinsection and dusty patches of fine-grained opaque mineralsdecorate the rims of grains. Classification: Achondrite (ureilite, polymict); minimalshock with rare mosaicism in olivine. Type specimen: A total of 9.8 g of sample and one thinsection are on deposit at NIPR. Fectay hold the main mass.

Northwest Africa 3340Algeria or MoroccoFind: April 2006Carbonaceous chondrite (CM2, anomalous)

History: Purchased by F. Kuntz in April 2006 in Erfoud,Morocco, and subsequently acquired for the DuPontCollection at PSF.Physical characteristics: Two pieces from a very fresh,broken, black, porous stone (total weight 12.7 g) with shinyfusion crust on one side.Petrography: (A. Irving and S. Kuehner, UWS; T. Bunch,NAU) Sparse mineral grains, carbon-rich objects, dust-armored chondrules and rare refractory inclusion occur in aheterogeneous, very fine grained, porous matrix composedmainly of bladed phyllosilicates with some pentlandite andcalcite (clearly visible under incident UV light). Olivinegrains (up to 2 mm across) are commonly armored by fine,polycrystalline “dust” and contain inclusions of Ni-richtroilite, chromite, millerite, kamacite and taenite. Bothpentlandite and magnesian olivine occur as separate smaller,angular grains. The carbon-rich objects (up to 50 μm across)consist of either pure graphite or a chlorine-rich organicphase. Chondrules consist of PO and POP olivine, manyhaving a fine-grained polycrystalline “dust” rims. One smallrefractory inclusion is composed of Mg-Al spinel withinclusions of perovskite. Mineral compositions and geochemistry: Larger zonedolivine grains (e.g., Fa17.9-33.9, Fa39.9–66); smallerhomogeneous olivine grains (e.g. Fa1.5, Fa19.9); pentlandite(Ni = 26.2 wt%). Matrix phyllosilicate material could not beanalyzed quantitatively, but has very consistent proportions ofMg, Fe, Si and S. The chlorine-rich organic phase contains~17 wt% Cl and ~32 wt% C, but no detectable N and minorO. Oxygen isotopes: (D. Rumble, CIW) Replicate analyses bylaser fluorination gave, respectively, δ18O = 0.494, 1.166;δ17O = 6.224, 7.049; Δ17O = −2.780, −2.542 (all ‰).Classification: Carbonaceous chondrite (CM2, anomalous);minimal weathering. The presence of chlorine-rich carboncompounds, which may be enigmatic chlorinated

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hydrocarbons, makes this specimen potentially unique amongCM chondrites.Specimens: A total of 2.7 g of sample is on deposit at UWSand the remainder of the mass (10 g) is at PSF.

Northwest Africa 4223AlgeriaFind: December 2005Achondrite (diogenite, olivine-bearing)

History: G. Hupé purchased the stones in December 2005 inTagounite, Morocco.Physical characteristics: The meteorite comprises twodense, dark brown and partly fusion crusted stones with atotal weight of 329 g.Petrography: (A. Irving and S. Kuehner, UWS) Themeteorite is coarse-grained (≤4 mm) with a primarilyprotogranular texture, and some areas of cataclasis. Olivine(50 vol%) and orthopyroxene (45 vol%) are the dominantminerals with accessory chromite, troilite and metal(kamacite). Some veinlets of terrestrial calcite crosscut thespecimen.Mineral compositions and geochemistry: Olivine(Fa30.0–31.2; FeO/MnO = 44.8–48.2), orthopyroxene(Fs24.2–25.2Wo2.8–3.2; FeO/MnO = 28.8), chromite (Cr/[Cr +Al] = 0.703–0.715; Fe/[Fe+Mg] = 0.69–0.73, mean TiO2 =1.02 wt%). Oxygen isotopes: (D. Rumble, CIW) Analyses oftwo aliquots by laser fluorination gave, respectively, δ18O =3.08, 3.22; δ17O = 1.44, 1.48; Δ17O = −0.180, −0.214 (all ‰).Classification: Achondrite (diogenite, olivine-bearing).Type specimens: A total of 20.4 g of sample, one polishedthin section and a polished mount are on deposit at UWS.GHupé holds the main mass.

Northwest Africa 4230AlgeriaFind: December 2005Mesosiderite

History: G. Hupé purchased this stone in December 2005 inRissani, Morocco.Physical characteristics: The meteorite is a single 134 gstone containing abundant metal.Petrography: (A. Irving and S. Kuehner, UWS) In thinsection, the meteorite is texturally heterogeneous, mostlyfragmental with variable grain size (0.5–4 mm), but someregions have triple junctions among silicate grains. Abundantmetal (kamacite with taenite), orthopyroxene, plagioclase(some with included grains of silica polymorph andclinopyroxene), schreibersite, merrillite, and troilite. Onerounded clot composed of clinopyroxene, merrillite andkamacite was observed. Mineral compositions: Orthopyroxene (Fs30.9Wo2.7–2.9, FeO/MnO = 23.9–26.2), plagioclase (An89.5–94.8Or.0.2), kamacite (Ni= 5.4–5.9 wt%), and taenite (Ni = 36–49 wt%).Classification: Mesosiderite.

Specimens: A total of 20.1 g of sample, one polished thinsection and a polished mount are on deposit at UWS. GHupéholds the main mass.

Northwest Africa 4232Northwest AfricaFind: December 2005Enstatite chondrite (EL3)

History: G. Hupé purchased the specimens in December 2005in Tagounite, Morocco.Physical characteristics: The meteorite consists of two darkbrown stones weighing 105 and 19 g. Cut surfaces havesparse grains of fresh metal, and there are multiple subparalleland anastomosing thin veinlets filled with iron oxides/hydroxides and some calcite from terrestrial weathering.Petrography: (A. Irving and S. Kuehner, UWS)Predominantly granular texture with mostly equant and somebladed grains (0.5 to 1.5 mm). Composed mainly of pureenstatite with subordinate altered kamacite, altered troilite,plagioclase and accessory schreibersite and daubreelite (asblades in altered troilite). Sparse RP chondrules (0.2–0.8 mmin diameter) composed of radiating (and some subparallel)enstatite grain clusters.Mineral compositions: Enstatite (En97.9–98.4Wo1.3–1.4) andplagioclase (An15.2–16.0Or4.3–4.4).Classification: Enstatite chondrite (EL3); S1, W4/5. Thisspecimen is similar to NWA 002, NWA 1067, NWA 2736,NWA 2965, and NWA 4295. It may also be related to AlHaggounia 001.Specimens: A total of 20 g of sample and one polished thinsection are on deposit at UWS. GHupé holds the main mass.

Northwest Africa 4255 27°51′00′′N, 7°48′00′′WHamada du Draa, southwest AlgeriaFind: September 2002Achondrite (diogenite)

History: Nomads found the meteorite in September 2002 inHamada du Draa, southwest Algeria.Physical characteristics: The total mass is 6000 g and isfragmented into hundreds of pieces, some of which are partlycovered with fusion crust.Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine,J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. Lorand,MNHNP). Predominantly composed orthopyroxene withscarce inclusions of troilite, ilmenite, spinel, olivine, andmetallic Fe-Ni.Mineral compositions and geochemistry: Orthopyroxene(Fs25.3Wo1.5; Fe/Mn = 23–28 [atomic]), spinel (Cr =0.92 wt%), olivine (Fa30), Fe, Ni-rich metal (NiO = <1 wt%).Oxygen isotopes: δ18O = 3.25, δ17O = 1.31, Δ17O = −0.38(all ‰).Classification: Achondrite (diogenite); S2, minorweathering.Type specimens: A total of 21 g of sample is on deposit at

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MNHNP. Two thin sections are on deposit at UJM. Ananonymous finder holds the main mass.

Northwest Africa 4269 27°59′N, 7°35′WHamada du Draa, southwest AlgeriaFind: September 2004Achondrite (eucrite, monomict)

History: Nomads found a complete stone in September 2004in Hamada du Draa (southwest Algeria).Physical characteristics: The complete stone is fusioncrusted and weighs 54 g. Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine,J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. Lorand,MNHNP). The rock is compact, fine-grained and containsmm-sized metal grains. A heterogeneous granulitic matrixwith plagioclase and recrystallized pyroxene, associated withsilica, fayalite, Ca phosphate, iron metal (Ni% <0.1), sulfide,spinel, and ilmenite is observed. Some clasts display residualophitic texture (lath plagioclase with granular exsolvedpigeonite). Pyroxenes occur as ferro-pigeonites exsolved inferro-augite and ferro-hypersthene. Individual augite grainsare also observed in the matrix.Mineral compositions and geochemistry: Augite (En26–27Wo34–41), hypersthene (En29–30Wo6–5), and matrix augitegrains (En26Wo40). Pyroxene Fe/Mn (27 to 42 [atomic]),spinel (Fe-rich chromite, cr# = 0.91). Oxygen isotopes:(R. Greenwood, OU) δ17O = 1.718, δ18O = 3.762, Δ17O =0.238 (all ‰). Classification: Achondrite (eucrite, monomict); S3, minorweathering. Type specimens: A total of 19.2 g of sample is on deposit atMNHNP. Two inclusions and one powder aliquot (1.690 g)are on deposit at UJM. An anonymous finder holds the mainmass.

Northwest Africa 4271 27°57′N, 7°50′WHamada du Draa, southwest AlgeriaFind: February 2003Achondrite (eucrite, polymict)

History: The meteorite found by nomads in Hamada du Draa,southwest Algeria. Physical characteristics: The stone displays a fine fusioncrust and weighs 6 g. Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine,J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P. Lorand,MNHNP). The stone has a fine- to medium-grained,brecciated texture containing mineral fragments ofplagioclase, diogenitic pyroxenes, spinel, olivine, and silica.The rock also contains some basaltic fragments displayingboth ophitic and subophitic textures, formed by plagioclaseand pigeonite; some pigeonite grains also display augiteexsolution lamellae. Diogenitic fragments are low inabundance (<10%).Mineral compositions and geochemistry: Mineral

fragments: plagioclase (An88.4), diogenitic pyroxenes(En67.4–75.9, Wo2.0–3.0), spinel (cr# = 0.89), olivine(Fa67–80). Basaltic fragments: plagioclase (An85.8–93.6),pigeonite (En37.2,Wo7.7), pigeonite with augite lamellae(En39.6,Wo41.4). Oxygen isotopes: (R. Greenwood, OU) δ18O= 3.34 and δ17O = 1.25, Δ17O = −0.48 (all ‰).Classification: Achondrite (eucrite, polymict); moderateshock and minor weathering. Type specimens: A total of 2.55 g of sample is on deposit atMNHNP. One thin section, one inclusion and a powder aliquot(430 mg) are on deposit at UJM. An anonymous finder holdsthe main mass.

Northwest Africa 4272Northwest AfricaFind: December 2003Achondrite (diogenite)

History: An anonymous collector recovered a single,complete stone in the western part of the Sahara in December2003. Physical characteristics: The individual is 6768 g anddisplays a partial fusion crust and regmaglypts.Petrography: (A. Seddiki, Ud’OEA and UJM;M. Messaoudi, USTHB, Algeria; B. Moine, J. Y. Cottin, UJM;B. Devouard, UBP; M. Denise, V. Sautter, J. P. Lorand,MNHNP). The sample is composed of Ca-poor pyroxenecontaining small opaque inclusions of spinel, troilite, andmetallic Fe-Ni (Ni 0.3 wt%). Specimen is crosscut by thinveins (50 μm) of plagioclase and displays smallconcentrations of Ca-rich pyroxene.Mineral compositions: Ca-poor pyroxene (Fs21.6–22.2Wo1.6–2.9), spinel inclusions (cr# = 0.85). Vein material:plagioclase (An81.5–86.3), Ca-rich pyroxene (Fs7.75–8.1,Wo45.3–4537). Pyroxenes (Fe/Mn = 24.7 to 31.9 [atomic]).Oxygen isotopes: (R. Greenwood, OU) δ 18O = 3.78 and δ17O= 1.50, Δ17O = −0.46 (all ‰).Classification: Achondrite (diogenite); minor shock andweathering. Type specimens: A total of 20 g of sample is on deposit atMNHNP. One thin section is on deposit at UBP. Ananonymous finder holds the main mass.

Northwest Africa 4294Morocco or AlgeriaFind: February 2006 Ordinary chondrite (type 3)

History: Purchased from a Moroccan dealer at the TucsonGem and Mineral Show by A. Hupé in February 2006.Physical characteristics: A single 84.2 g light brown stonelacking fusion crust and with abundant, large chondrules.Petrography: (A. Irving and S. Kuehner, UWS) Closelypacked PO and POP chondrules with a mean diameter of1.2 mm. Chondrules contain accessory phases including Cr-bearing clinopyroxene, chromite, partially altered kamacite,

1654 H. C. Connolly, Jr., et al.

taenite, troilite, and terrestrial barite. The content of metal(+minor Fe hydroxide) is very low (mode determined by BSEimaging of a whole thin section is 3 vol%).Geochemistry: Olivine (mostly Fa2–25, with rimcompositions up to Fa95) Oxygen isotopes: (D. Rumble, CIW)Analyses of two acid-washed whole rock fragments by laserfluorination gave, respectively, δ18O = 5.38, 5.31; δ17O =3.34, 3.23; Δ17O = 0.508, 0.443 (all ‰). These oxygenisotopic compositions are closer to the TFL than to those of Hchondrites and far removed from those of LL chondrites.Classification: Ordinary chondrite (type 3); S1, W2.Specimens: A total of 22 g of sample and one polished thinsection are on deposit at UWS. AHupé holds the main mass.

Northwest Africa 4298Morocco or AlgeriaFind: September 2005 Ordinary chondrite (type 3)

History: Purchased from a Moroccan dealer in Erfoud byA. Hupé in September 2005.Physical characteristics: A single 18 g light brown stonelacking fusion crust and with abundant, large chondrules.Petrography: (A. Irving and S. Kuehner, UWS): Very wellformed and closely packed chondrules (mean diameter1.5 mm). Chondrules (PO and POP) contain euhedral olivineor orthopyroxene crystals with Fe-enriched rims enclosed inglassy groundmass. Accessory kamacite (some as sphericalgrains in chondrules), taenite and troilite. The content ofmetal (+minor Fe hydroxide) is very low (mode determinedby BSE imaging of a whole thin section is 2 vol%).Geochemistry: Olivine (Fa0–46) Oxygen isotopes:(D. Rumble, CIW) Analyses of two acid-washed whole rockfragments by laser fluorination gave, respectively, δ18O =5.96, 5.57; δ17O = 3.78, 3.51; Δ17O = 0.639, 0.573 (all ‰).Although these Δ17O values are within the range for Hchondrites, this specimen is much too poor in metal to be an Hchondrite.Classification: Ordinary chondrite (type 3); S1, W1/2.Specimens: A total of 4 g of sample and one polished thinsection are on deposit at UWS. AHupé holds the main mass.

Northwest Africa 4302AlgeriaFind: December 2005Achondrite (diogenite)

History: G. Hupé purchased the meteorite in December 2005in Tagounite, Morocco.Physical characteristics: The sample is composed of twovery fresh, yellowish-green, partly crusted stones (36 g and10.2 g) containing visible metal in cut slices.Petrography: (A. Irving and S. Kuehner, UWS) Themeteorite is coarse-grained and has a partly cataclastictexture. It is composed mostly of orthopyroxene with minorolivine, plagioclase, troilite, and kamacite.

Mineral compositions and geochemistry: Orthopyroxene(Fs25.2–25.4Wo3.4–3.7; FeO/MnO = 30.4–33.5), olivine (Fa29.7,FeO/MnO = 48.1), and plagioclase (An89.8Or0.4).Classification: Achondrite (diogenite).Type specimens: A total of 9.3 g of sample and one polishedthin section are on deposit at UWS. GHupé holds the mainmass.

Northwest Africa 4304Northwest AfricaFind: 2004Achondrite (ureilite, polymict)

History: An anonymous finder recovered the specimen in thewestern part of the Sahara. C. Anger purchased the meteoritein Baden, Austria, in 2004. Physical characteristics: Eighteen small fragments totaling22.97 g were recovered.Petrography: (A. Greshake, MNB and M. Kurz, Kurz)The meteorite is a polymict breccia with lithic andmineral clasts set into a ureilitic matrix dominated bylarge olivine and pigeonite crystals. Lithic clasts includeureilite material and chondritic lithologies withrecognizable chondrule fragments. The meteorite containsdiamonds. Mineral compositions and geochemistry: Ureilite material:Olivine (Fa1.1–22.4), pyroxene (Fs17.8Wo5.3). Chondriticlithologies: Olivine (Fa13.6–20.4), pyroxene (Fs12.9–14.4). Classification: Achondrite (ureilite, polymict); extensiveshocked, moderate weathering. Type specimens: A total of 4.6 g plus one polished thinsection are on deposit at MNB. Anger holds the mainmass.

Northwest Africa 4360Northwest AfricaFind: 2005 Rumuruti chondrite (R3.6)

History: The meteorite was recovered by an anonymousfinder in the western part of the Sahara and purchased by themain mass holder in Erfoud, Morocco, in 2005. Physical characteristics: Approximately 100 fragmentstotaling 308.5 g were found. Petrography: (A. Greshake, MNB) Clearly definedchondrules and chondrule and mineral fragments, allembedded into a fine-grained matrix. In thin section themeteorite appears unbrecciated. Mineral compositions: Olivine (Fa34±11; range Fa0.3–39.8),low-Ca pyroxene (Fs16.1±5.6; range Fs9.3–24.7), augite(Fs9.2Wo46.7).Classification: Rumuruti chondrite (R3.6); S4, moderateweathering. Type specimens: A total of 23.2 g plus one polished thinsection are on deposit at MNB. HSSH holds the mainmass.

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Northwest Africa 4362MoroccoFind: 2005Carbonaceous chondrite (CK5/6)

History: An anonymous finder collected the meteorite inthe western part of the Sahara. The main mass holderpurchased the sample in 2005 in Erfoud, Morocco. Physical characteristics: One oriented stone of 60.1 gcovered with fresh fusion crust was recovered. Petrography: (A. Greshake, MNB) The meteorite shows afine-grained texture with recrystallized matrix dominatingover rare and mostly poorly defined chondrules and mineralfragments. Feldspar is abundant in the matrix and minorphases include Cr-rich magnetite and Ca pyroxene. Mineral compositions and geochemistry: Olivine (Fa29.9),low-Ca pyroxene (Fs25.5). Oxygen isotopes (I. A. Franchi andR. C. Greenwood, OU): δ17O = −4.72, δ18O = −0.63, Δ17O =−4.39 (all ‰). Classification: Carbonaceous chondrite (CK5/6); minimalshock, moderate to extensive weathering. Type specimens: A total of 14.4 g plus one polished thinsection are on deposit at MNB. HSSH holds the main mass.

Northwest Africa 4372Northwest AfricaFind: 2005 Carbonaceous chondrite (CK4)

History: An anonymous finder recovered the meteorite in thewestern part of the Sahara. The main mass holder purchasedthe sample at a mineral fair in Munich, Germany, in 2005. Physical characteristics: One stone of 64.8 g was recovered.Petrography: (A. Greshake, MNB). The meteorite consists ofsharply defined chondrules, mineral fragments, and largeCAIs set into a fine-grained matrix. Minor phases includefeldspar, Cr-rich magnetite, and Ca-pyroxene. Mineral compositions: Olivine (Fa24.6–28.8); low-Capyroxene (Fs1.2–24.1). Oxygen isotopes: (I. A. Franchi andR. C. Greenwood, OU) δ17O = −3.26, δ18O = 0.40,Δ17O = −3.46 (all ‰). Classification: Carbonaceous chondrite (CK4); minimalshock, extensive weathering. Type specimens: A total of 13.5 g plus one polished thinsection are on deposit at MNB. HSSH holds the main mass.

Northwest Africa 4375Northwest AfricaFind: 2005Primitive achondrite (winonaite)

History: An anonymous finder collected the meteorite in thewestern part of the Sahara. The main mass holder purchasedthe sample at a mineral fair in Munich, Germany, in 2005. Physical characteristics: A small oval stone of 12.2 g wasrecovered. Petrography: (A. Greshake, MNB). The meteorite consists of

low-Ca pyroxene, Ca-pyroxene, olivine, plagioclase, metallicFe-Ni, and troilite. Silicate grains are often euhedral anddisplay an equigranular texture with abundant triplejunctions. Mineral compositions and geochemistry: Olivine (Fa4.4),low-Ca pyroxene (Fs5Wo1.5), Ca-pyroxene, (Fs2.3Wo46.2).Oxygen isotopes: (I. A. Franchi and R. C. Greenwood, OU)Mean of two replicates δ17O = 2.74, δ18O = 5.88,Δ17O = −0.31 (all ‰). Classification: Primitive achondrite (winonaite); minimalshock, moderate weathering. Type specimens: A total of 3.9 g of sample plus one polishedthin section are on deposit at MNB. HSSH holds the mainmass.

Northwest Africa 4380Northwest AfricaFind: 2006 Achondrite (diogenite)

History: An anonymous finder recovered the meteorite in thewestern part of the Sahara. The main mass holder acquired thesample in Erfoud, Morocco, in 2006. Physical characteristics: A total of 42 small fragments witha combined mass of 211.2 g were recovered. Petrography: (A. Greshake, MNB). The meteorite iscomposed of large blocky orthopyroxene crystals. Minorphases include FeS and Mg-Al-chromite. Mineral compositions: Low-Ca pyroxene (Fs22.9Wo1.5). Classification: Achondrite (diogenite); moderate shock,moderate to extensive weathering. Type specimens: A total of 22.5 g of sample plus onepolished thin section are on deposit at MNB. HSSH holds themain mass.

Northwest Africa 4391Northwest AfricaFind: 2005Achondrite (eucrite, polymict)

History: An anonymous finder recovered the meteorite innorthwest Africa. The main mass holder acquired thespecimen in 2005 in Midelt, Morocco. Physical characteristics: A single stone weighing 54.8 gwith a grayish color and little fusion crust present wasrecovered. Petrography: (A. Greshake, MNB). The meteorite is apolymict breccia consisting of coarse basaltic and mineralclasts set into an abundant fine-grained groundmass.Mineral fragments are dominantly large plagioclase andexsolved low-Ca pyroxene. Minor phases include silica,ilmenite, and Al,Ti-rich chromite. Mineral compositions: Plagioclase (An85.5–95.9) andpyroxene (Fs41.7–54Wo2.6–20.1). Classification: Achondrite (eucrite, polymict); moderateshock, moderate weathering.

1656 H. C. Connolly, Jr., et al.

Type specimens: A total of 11.4 g of sample plus onepolished thin section are on deposit at MNB. Ralew holds themain mass.

Northwest Africa 4396Northwest AfricaFind: 2006 Achondrite (eucrite, polymict)

History: An anonymous finder recovered the meteorite innorthwest Africa. The main mass holder purchased thesample in Tagounite, Morocco. Physical characteristics: A single stone of 680 g, partlycovered with fusion crust, was recovered.Petrography: (A. Greshake, MNB). The meteorite is apolymict breccia consisting of coarse- and fine-grainedbasaltic and mineral clasts set in a fine-grained clasticgroundmass. Mineral fragments are mostly large plagioclaseand exsolved low-Ca pyroxene. Minor phases include silica,ilmenite, and troilite.Mineral compositions: Plagioclase (An58.9–92.7) andpyroxene (Fs26.8–59.3Wo2.4–42.6). Classification: Achondrite (eucrite, polymict); minimalshock, moderate to extensive weathering. Type specimens: A total of 20 g of sample plus one polishedthin section are on deposit at MNB. Ralew holds the mainmass.

Northwest Africa 4397Northwest AfricaFind: 2006Achondrite (eucrite, polymict)

History: The meteorite was recovered by ananonymous finder in northwest Africa and purchasedby the main mass holder in Tagounite, Morocco. Physical characteristics: A single stone of 34 g wasrecovered. Petrography: (A. Greshake, MNB) The meteorite consists ofcoarse- and fine-grained basaltic and mineral clastsembedded in a fine-grained clastic matrix. Mineral fragmentsare mostly plagioclase and exsolved Ca-pyroxene. Minorphases include silica, ilmenite, and troilite. Mineral compositions: Plagioclase (An68.1–92.7) andpyroxene (Fs36.7–58.8Wo8–28). Classification: Achondrite (eucrite, polymict); minimumshock, moderate to extensive weathering. Type specimens: A total of 6.8 g of sample plus one polishedthin section are on deposit at MNB. Ralew holds the mainmass.

Northwest Africa 4398MoroccoFind: 2005Achondrite (eucrite, monomict)

History: The meteorite was recovered by an anonymous

finder in northwest Africa and purchased by the main massholder in Midelt, Morocco. Physical characteristics: A single stone of 228 g wasrecovered. Petrography: (A. Greshake, MNB). The meteoritedisplays a largely unbrecciated basaltic texture withcalcic plagioclase and exsolved low-Ca pyroxenebeing the major phases. Minor phases includesilica, ilmenite, and Al,Ti-rich chromite. Mineral compositions: Plagioclase (An78.2–87.2) andpyroxene (Fs31.2–61.1Wo4.6–40.5). Classification: Achondrite (eucrite, monomict); moderateshock, minimal weathering. Type specimens: A total of 20.3 g of sample plus onepolished thin section are on deposit at MNB. Ralew holds themain mass.

Northwest Africa 4399Northwest AfricaFind: 2005Achondrite (acapulcoite)

History: The meteorite was recovered in northwest Africa byan anonymous finder and purchased by Stefan Ralew inMidelt, Morocco, in 2005. Physical characteristics: Many small fragments totaling210 g were recovered. Petrography: (A. Greshake, MNB) The meteorite consistsdominantly of low-Ca pyroxene, olivine, augite, troilite,metallic Fe-Ni and plagioclase; minor phases includechromite and phosphates. It displays a completelyrecrystallized texture with abundant 120° triple junctions. Mineral compositions: Olivine (Fa7.3; range Fa6.5–7.8),low-Ca pyroxene (Fs8.7–9.2Wo2.2–3.2), augite, (Fs3.7–

4.4Wo41.3–44.3; up to Cr2O3 = 1.7 wt%). Oxygen isotopes: (I.A. Franchi and R. C. Greenwood, OU) δ17O = 1.61, δ18O= 4.87, Δ17O = −0.92 (all ‰). Classification: Achondrite (acapulcoite); minimal shock,extensive weathering. The sample may be paired with NWA2627. Type specimens: A total of 20.3 g of sample plus onepolished thin section are on deposit at MNB. Ralew holds themain mass.

Northwest Africa 4470AlgeriaFind: July 2006Achondrite (eucrite, basaltic, anomalous)

History: G. Hupé purchased the specimen in July 2006 inRissani, Morocco.Physical characteristics: The sample is made up of a total of48 broken gray stones with a combined weight of 631 g.Petrography: (A. Irving and S. Kuehner, UWS) Themeteorite is composed mainly of large, distinctively zonedlow-Ca pyroxene grains (≤0.8 mm) and interstitial

The Meteoritical Bulletin, No. 92 1657

plagioclase, with minor silica (associated with blebbytroilite), augite, chromite, and ilmenite. No metal wasobserved. Many pigeonite grains consist of multiplesubgrains, with narrow zones of ferroan olivine along theirboundaries.Mineral compositions and geochemistry: Orthopyroxenecores (Fs31.3–33.9Wo4.6–5.2, FeO/MnO = 26.8–27.4) havesharply defined boundaries against wider, much more Fe-richmantles of exsolved pigeonite (host orthopyroxeneFs59.1–60.3Wo2.9–3.9, FeO/MnO = 31.9–33.9); olivine alongsubgrain boundaries in pyroxene (Fa81.7, FeO/MnO = 42.3);plagioclase (An88.9Or0.3).Classification: Achondrite (eucrite, basaltic, anomalous).The ferroan olivine along grain boundaries and the gap inpyroxene compositions requires that this sample be classifiedas anomalous.Type specimens: A total of 20.1 g of sample and one polishedthin section are on deposit at UWS. GHupé holds the mainmass.

Northwest Africa 4473Northwest AfricaFind: July 2006Achondrite (diogenite)

History: G. Hupé purchased a total of 32 dark stones in July2006 in Laâyoune, Morocco.Physical characteristics: Cut-surfaces of the stones showpale yellowish-green angular clasts (see Fig. 1) and have acombined weight of 7020 g. No fusion crust was noted for anyof the specimens.Petrography: (A. Irving and S. Kuehner, UWS) Brecciacomposed of polycrystalline clasts (≤2 cm) set in a matrixderived from several different diogenite precursors. Nobasaltic eucrite clasts were observed. The sample is modallydominated by orthopyroxene with subordinate olivine, augite,chromite, silica polymorph, rare calcic plagioclase, troilite,pyrrhotite, and kamacite.Mineral compositions: Orthopyroxene compositions fallinto at least three distinct populations (median compositions)Fs17.2Wo1.0, FeO/MnO = 34.4; Fs21.6Wo2.1, FeO/MnO = 29.3;Fs37.2Wo3.5, FeO/MnO = 32.6). Olivine (Fa24.5, FeO/MnO =50.2). Classification: Achondrite (diogenite).Specimens: A total of 20.1 g of sample and one polishedmount are on deposit at UWS. GHupé holds the main mass.

Northwest Africa 4478AlgeriaFind: September 2006Achondrite (lodranite)

History: G. Hupé purchased the sample in September 2006 inZagora, Morocco.Physical characteristics: Two dense, brown stones (298 gand 146 g) lacking fusion crust.

Petrography: (A. Irving and S. Kuehner, UWS) Thisspecimen is composed of large mineral and polycrystallinelithologies (up to 8 mm across) with interstitial fine-grainedmaterial of the same phases. The large minerals consist ofeither olivine or orthopyroxene (with clinopyroxeneexsolution lamellae associated with blebs of Ni-free ironmetal). The polycrystalline lithology consists mainly ofinterlocking olivine grains (up to 3 mm across) and sparselarge chromite grains with interstitial clinopyroxene,orthopyroxene, kamacite, pyrrhotite, pentlandite, and troilite.The modal abundance of metal (+limonite after primarymetal) is 5 vol%. Plagioclase is absent. Olivine grains containnumerous blebby to worm-like polycrystalline inclusions, andclinopyroxene grains contain similar inclusions; someexamples exhibit symplectitic intergrowths of these variousphases. Some olivine grains contain multiple blade-likelamellae of olivine of a different composition. Narrowelongate zones or discontinuous veinlets of metal are presentwithin clinopyroxene, and adjacent to such metal thepyroxene has a more magnesian composition.Mineral compositions and geochemistry: Olivine(Fa10.6–10.9; FeO/MnO = 22.1–23.9), clinopyroxene(Fs3.9Wo41.9; FeO/MnO = 10.2), orthopyroxene lamella inclinopyroxene (Fs9.1Wo1.3; FeO/MnO = 11.9) and chromite(Cr/[Cr + Al] = 0.822–0.825; Mg/[Mg + Fe] = 0.506–0.520,TiO2 = 0.31–0.37 wt%). Oxygen isotopes: (D. Rumble, CIW)Quadruplicate analyses by laser fluorination gave,respectively, δ18O = 2.23, 2.43, 2.23, 2.40; δ17O = 0.14,0.30, 0.07, 0.11; Δ17O = −1.034, −0.984, −1.107, −1.147(all ‰).Classification: Achondrite (lodranite). Type specimens: A total of 20.1 g of sample and one polishedthin section are on deposit at UWS. GHupé holds the mainmass.

Northwest Africa 4480AlgeriaFind: Summer 2006Achondrite (Martian, basaltic shergottite)

History: The sample was recovered in Algeria in the summer

Fig. 1. An image of a handsample of Northwest Africa 4473.

1658 H. C. Connolly, Jr., et al.

of 2006. G. Hupé purchased it in Tagounite, Morocco, inSeptember 2006. Physical characteristics: The meteorite is a single, veryfresh 13 g ellipsoidal stone, mostly coated by dark brownfusion crust. Maskelynite, yellow-green olivine and tan-colored pyroxene are visible on cut face.Petrography: (A. Irving and S. Kuehner, UWS) The stone ismostly a relatively fine-grained (mean grain size 0.15 mm)basaltic rock, but with several coarser grained,glomerocrystic regions. The dominant matrix consists ofplagioclase laths (maskelynite), olivine and complexly zonedclinopyroxene with accessory Ti-chromite, ilmenite, Mg-Fe–bearing merrillite and rare Si-rich glass or silica polymorph.Glomerocryst regions are composed of coarser (0.5–0.8 mm)plagioclase (maskelynite) and olivine with interstitialpigeonite and ilmenite.Mineral compositions and geochemistry: Matrix-clinopyroxene is patchily zoned from augite cores(Fs24.9–31.2Wo35.3–31.1, FeO/MnO = 30–32) to pigeonite rims(Fs55.4–56.4Wo17.5–15.4, FeO/MnO = 36); olivine (Fa67.9–79.2,FeO/MnO = 49–52); plagioclase (An58.40–61.0 Or1.6).Plagioclase in glomerocryst regions is consistently morecalcic (An66.3–68.5Or0.3). Bulk composition (R. Korotev,WUSL): INAA of two ~37 mg whole fragments of matrixgave Na 1.40 wt%, Fe 15.8 wt%, and (in ppm) Sc 39.7, Cr1027, Ni <60, La 1.85, Sm 2.69, Eu 0.86, Tb 1.05, Yb 4.16,Hf 3.16, Th 0.24; the REE pattern shows moderate light REEdepletion, elevated heavy REE abundances and a negative Euanomaly.Classification: Achondrite (Martian, basaltic shergottite).Type specimens: A total of 2.6 g of sample is on deposit atUWS. PSF holds the main mass (6.63 g).

Northwest Africa 4482AlgeriaFind: August 2006Pallasite (main group)

History: G. Hupé purchased the sample in August 2006 inTagounite, Morocco.Physical characteristics: The meteorite consists of a total of30 dark, magnetic fragments containing yellowish-greensilicate in a dark brown matrix. The fragments have acombined weight of 5816 g.Petrography: (A. Irving and S. Kuehner, UWS) Large olivinegrains (up to 8 mm across) with interstitial, porous, bandediron hydroxides enclosing sparse angular grains of terrestrialquartz, and accessory chromite, schreibersite and fresh metal(both kamacite and taenite).Mineral compositions and geochemistry: Olivine(Fa12.2–13.0, FeO/MnO = 41.1–42.5). Oxygen isotopes:(D. Rumble, CIW) analysis of acid-washed handpickedolivine by laser fluorination gave δ18O = 3.65, δ17O = 1.72,Δ17O = −0.198 (all in ‰).Classification: Pallasite (main group). The original metal in

this specimen is almost entirely weathered to ironhydroxides.Specimens: A total of 20.1 g of sample, one polished thinsection and one polished mount are on deposit at UWS.GHupé holds the main mass.

Northwest Africa 4484AlgeriaFind: June 2006Achondrite (eucrite, basaltic)

History: S. Ralew purchased the specimens in June 2006 inRissani, Morocco.Physical characteristics: The meteorite consists of sevenbroken fragments of a dark gray stone with a combinedweight of 140 g.Petrography: (A. Irving and S. Kuehner, UWS) The thinsection studied shows an ophitic texture, with large(≤1.3 mm) pyroxene grains (composed of orthopyroxene withfine augite exsolution lamellae or patchy intergrowths oforthopyroxene with augite) and distinctive, thin plagioclaselaths (commonly in radiating clusters). Interstitial mesostasisregions contain silica, ilmenite, troilite, and minor Ni-freekamacite (partly altered to brown iron hydroxides).Mineral compositions and geochemistry: Augite(Fs32.4–32.8Wo41.2–41.3; FeO/MnO = 32.7–36.7), orthopyroxene(Fs64.9Wo2.9; FeO/MnO = 32.2) and plagioclase(An86.0–90.5Or0.2–0.5).Classification: Achondrite (eucrite, basaltic). Type specimens: A total of 20 g of sample and one polishedthin section are on deposit at UWS. Ralew holds the mainmass.

Northwest Africa 4486Morocco or AlgeriaFind: September 2005 Ordinary chondrite (type 3)

History: Purchased at the Denver Mineral Show by A. Hupéin September 2004.Physical characteristics: A single 21.3 g light brown stonelacking fusion crust and with abundant, small chondrules.Petrography: (A. Irving and S. Kuehner, UWS): Closelypacked, round PO and POP chondrules (mean diameter0.8 mm) with accessory, partially altered kamacite, troiliteand pentlandite. The content of metal (+minor Fe hydroxide)is very low (mode determined by BSE imaging of a wholethin section is 2 vol%).Geochemistry: Olivine (Fa5–29), orthopyroxene(Fs0.5–30Wo1.6). Oxygen isotopes: (D. Rumble, CIW) analysesof two acid-washed whole rock fragments by laserfluorination gave, respectively, δ18O = 5.11, 5.51; δ17O =3.15, 3.29; Δ17O = 0.465, 0.400 (all ‰). These oxygenisotopic compositions are closer to the TFL than those of Hchondrites and far removed from those of LL chondrites.Classification: Ordinary chondrite (type 3); S1, W1/2.

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Specimens: A total of 4.6 g of sample and one polished thinsection are on deposit at UWS. AHupé holds the main mass.

Northwest Africa 4506 Northwest Africa Find: October 2006 Pallasite (main group)

History: Michael Farmer purchased the sample in Denver,Colorado, in October 2006. Physical characteristics: The meteorite was a fragment witha total mass of 23.12 g. The exterior color of the meteoritewas orange and contains numerous by dark veins, as it wasmainly olivine with veins of oxidized metallic Fe-Ni. Petrography: (D. Schrader, M. Killgore, and D. Lauretta,UAz) The meteorite contains olivine, Fe, Ni-rich metal,chromite, sulfide, and FeO. The olivine (2.2–3.2 mm) grainsare surrounded by weathered remnant metal veins. Mineral compositions and geochemistry: (D. Schrader,M. Killgore, D. Lauretta, K. Domanik, and D. Hill at UAz)Olivine (Fo86.3–86.8; average = Fo86.5±0.2), kamacite (averageNi = 4.96 ± 1.60 [3.47 to 7.76] and average Co = 0.86 ± 0.04[0.81–0.92] all wt%) and one taenite analysis (Ni = 20.75 andCo = 0.54 [both wt%]). Reliable analyses on chromite andtroilite were not possible due to weathering.Classification: Pallasite (main group).Type specimens: A total of 8.17 g of sample is on deposit atUAz (UA2059). Farmer holds the main mass.

Northwest Africa 4507MoroccoFind: 2005Achondrite (ureilite)

History: Purchased in 2006 at the Tucson Gem and MineralShow.Physical characteristics: Total mass, 85.0 g, a deformedparallel piped piece with smaller top surface, 68 × 24 ×24 mm in size, external color is dark brown and no fusioncrust is apparent.Petrography: (H. Takeda, Chiba). The sample consists ofolivine (up to 2.3 × 1.7 mm in size) and pyroxene. One PTSshows a typical ureilite texture with carbonaceous veins, inwhich Fe metal and sulfide are present. Approximately one-third of mafic silicates are pigeonite. A part of carbonaceousveins intrudes into an olivine crystal as a plate. Olivine crystalshave minor cracks, but shock effect is minor. Some pigeonitegrains show a twin texture. Mineral compositions: Olivine Fo79–82 (core) and >Fo90(rims). Major pyroxenes have pigeonite compositions(Fs19Wo10). A large olivine crystal contains a small ellipsoidalinclusion of pigeonite, 0.26 × 0.20 mm, with small regions ofhigh-Ca (Fs14Wo35) and low-Ca (Fs17.3Wo4.8). Pyroxenesenclosed in thick rims of the small ellipsoidal inclusion ofpigeonite within the olivine grain; another ellipsoidalinclusion (0.16 × 0.09 mm) has low-Ca pyroxene composition

(Fs18.5Wo4.6). Microscopic observations and Raman analyses(T. Nakamuta, KyuU) show tiny diamond crystals occurringin blade-shaped graphite crystals. Classification: Achondrite (ureilite); minimum weathering,minimum shock.Type specimen: A total of 17.22 g of sample and one thinsection are on deposit at NSMT. Hori holds the mainmass.

Northwest Africa 4508Northwest AfricaFind: 2001 Achondrite (ureilite)

History: Purchased in Rissani, Morocco in April 2001. Physical characteristics: One subrounded blocky mass (5 ×3 × 2 cm) of 182 g and covered with dark brown, moderatelyweathered fusion crust.Petrography: (H. Takeda, Chiba and A. Yamaguchi, NIPR).The sample contains fine-grained, granoblastic olivine, partlydarkened pyroxene with carbonaceous (graphite) veins atgrain boundaries. Minor weathering and heavily shocked. Afew grains of pyroxene or olivine crystals form larger grains(0.7 × 0.4 to 3 × 1 mm). An original olivine crystal is brokeninto many very fine crystallites to show a granoblastic texture.There is an unusual texture of pyroxene crystals found in oneof the sections studied.Mineral compositions and geochemistry: Olivine(Fo83–86 [cores], up to Fo89 [rims]); pigeonite (Fs14Wo7; Wo6–

10 range). Oxygen isotopes: (M. Kusakabe, OkaU) δ17O =2.97, δ18O = 7.66 (both ‰).Classification: Achondrite (ureilite).Type specimen: A total of 20.2 g of sample and one thinsection are on deposit at NIPR. Fectay holds the mainmass.

Northwest Africa 4519 MoroccoFind: 2001Achondrite (ureilite)

History: Purchased in Zagora, Morocco in 2001. Physical characteristics: The deformed conical shaped mass(114 g; 6.5 × 3.5 cm) is partially fusion-crusted.Petrography: (H. Takeda, Chiba and A. Yamaguchi, NIPR).It contains olivine and pyroxene with carbonaceous veins atgrain boundaries. Mafic silicate crystals seem to show apreferred orientation, two to three crystals up to 4.2 × 1.4 mmin size are joined with common elongation direction withoutcarbonaceous veins to form a large aggregate (~4.2 × 3.8 mm)with carbonaceous materials around it. Mineral compositions and geochemistry: Olivine(Fo83–80 [cores]; Fo89 [rims]), pyroxene (Fs16.7Wo8.6). Oxygenisotopes: (M. Kusakabe, OkaU), δ17O = 3.29, δ18O = 8.20(both ‰).Classification: Achondrite (ureilite); minimal weathering.

1660 H. C. Connolly, Jr., et al.

Type specimen: A total of 20 g of sample and two thinsections are on deposit at NIPR. Fectay holds the main mass.

Northwest Africa 4523Al Nif, MoroccoFind: April 2001Achondrite (eucrite, basaltic)

History: Carine and Bruno Fectay purchased the rock in AlNif, Morocco in April 2001. Physical characteristics The very fresh stone weights 174 gand is nearly covered with fusion crust. The interior of thestone is light gray in color and displays a brecciated texturewith dark clasts ranging from a few mm to about 1.5 cm.Petrography: (J. A. Barrat and M. Bohn, IUEM;A. Yamaguchi, NIPR) Two types of clasts are found in a fine-grained recrystallized matrix: medium-grained ophitic/subophitic and fine-grained clasts. Medium-grained clasts(~1–2 mm) display a subophitic texture, and are composed ofplagioclase, pyroxene (pigeonitic core and augitic rim), silica,ilmenite, chromite, and recrystallized mesostasis. Fine-grained clasts consist of pyroxene phenocrysts (~150 μm indiameter) in a fine-grained groundmass that consists ofplagioclase, pigeonite, augite, silica, ilmenite, troilite, andK-feldspar.Geochemistry: (J. A. Barrat, M. Benoit, J. Cotton, IUEM andA. Yamaguchi, NIPR). Mineral phases in clasts and matrixhave identical composition; pyroxenes (Mg35.9Ca4.7Fe59.4 toEn30.2Wo43.3Fs26.5; FeO/MnO = 34 [n = 265]) and plagioclase(An90–71). Bulk composition: FeOtotal/MgO = 2.84 (ICP-AES)close to typical main group eucrites but exhibits the highestconcentrations in K2O = 0.15 wt% measured in eucrites.Moreover, it is richer in TiO2 = 1.35 wt% (ICP-MS) andincompatible trace elements relative to Stannern. Its REEelement pattern is flat (Lan/Ybn = 1.29) and displays a markednegative Eu anomaly (Eu/Eu* = 0.62). Bulk oxygen isotopic:(R. C. Greenwood, I. A. Franchi, OU) composition is δ17O =1.757 ± 0.004, δ18O = 3.791 ± 0.013, Δ17O = −0.230 ± 0.003(all ‰).Classification: Achondrite (eucrite, basaltic) and lies on theStannern trend.Type specimens: A total of 21 g of sample and one thicksection are on deposit at IUEM. Fectay holds the mainmass.

Northwest Africa 4527AlgeriaFind: Summer 2006Achondrite (Martian, basaltic shergottite)

History: The stones were recovered in Algeria in summer2006, and G. Hupé purchased them in M’Hamid, Morocco, inJuly 2006. Physical characteristics: The meteorite consists of twobroken, brown stones weighing 10.06 g. The stones haveweathering rinds ~2 mm thick.

Petrography: (A. Irving and S. Kuehner, UWS) Olivineoccurring with either prismatic low-Ca pyroxene phenocrystsor chromite microphenocrysts is set in a matrix of pigeonite,maskelynite, Ti-chromite, ilmenite, merrillite, and pyrrhotite.Minor veinlets of calcite and barite are present.Mineral compositions: Olivine phenocrysts are zoned fromFa19.8–22.4 (cores) to Fa49.2–50.9 (rims) (FeO/MnO = 41–56);pyroxene phenocrysts are zoned from orthopyroxene cores(Fs22.8Wo4.1, FeO/MnO = 40) to pigeonite rims (Fs40.1Wo11.9,FeO/MnO = 40); olivine microphenocrysts Fa32.7 (FeO/MnO = 51); maskelynite (An53.7–66.4 Or0.7–0.1); matrixchromite is relatively Ti-rich, whereas chromite occurring asmicrophenocrysts and as inclusions in olivine phenocrysts isTi-poor and Mg-rich.Classification: Achondrite (Martian, basaltic shergottite). Type specimens: A total of 2.1 g of sample and one thinsection are on deposit at UWS. GHupé holds the main mass.

Northwest Africa 4531Morocco or AlgeriaFind: September 2005 Ordinary chondrite (type 3)

History: Purchased at the Denver Mineral Show by A. Hupéin September 2005.Physical characteristics: Three light brown stones (totalweight 38.9 g) lacking fusion crust and with abundant largechondrules.Petrography: (A. Irving and S. Kuehner, UWS) Closelypacked PO and POP chondrules with a mean diameter1.0 mm. Chondrules contain accessory phases such aspartially altered kamacite, taenite, and troilite. The content ofmetal (+minor Fe hydroxide) = 2 vol%.Geochemistry: Olivine (Fa4–27) Oxygen isotopes:(D. Rumble, CIW) Analysis of an acid-washed whole rocksample by laser fluorination gave δ18O = 5.25, δ17O = 3.47,Δ17O = 0.709 (all ‰). Although these Δ17O values are withinthe range for H chondrites, this specimen is much too poor inmetal to be an H chondrite.Classification: Ordinary chondrite (type 3); S1, W1/2.Specimens: A total of 7.8 g of sample and one polished thinsection are on deposit at UWS. AHupé holds the main mass.

Northwest Africa 4587AlgeriaFind: September 2006Achondrite (ungrouped)

History: G. Hupé purchased the rock in September 2006 inErfoud, Morocco.Physical characteristics: The meteorite comprises a single,dense stone (530 g) without fusion crust. The mainconstituent (pyroxene) is a distinctive deep brown color andseveral large opaque grains are visible.Petrography: (A. Irving and S. Kuehner, UWS) Granulartexture with large pyroxene grains (pigeonite with numerous

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fine, parallel exsolution lamellae of clinopyroxene), andinterstitial polycrystalline plagioclase (with rims of silicaagainst pyroxene). Accessory minerals are skeletal ilmenite,merrillite, Ni-bearing pyrrhotite and rare kamacite. One largeoikocryst of ilmenite + Ti-chromite contains numerouschadacrysts of plagioclase and has narrow rims of fayaliticolivine adjacent to surrounding pyroxene.Mineral compositions: Pyroxene consists of host pigeonite(Fs63.4Wo6.9 FeO/MnO = 67.6, TiO2 = 0.49 wt%) and lamellaeof clinopyroxene (Fs35.4Wo38.9, FeO/MnO = 69.4, TiO2 =0.90 wt%); plagioclase (An85); olivine rim adjacent toilmenite (Fa81.9, FeO/MnO = 112).Classification: Achondrite (ungrouped). This very freshstone is essentially identical to NWA 011, NWA 2400, andNWA 2976, and evidently is paired with them.Specimens: A total of 20 g of sample is on deposit at UWS.GHupé holds the main mass.

Northwest Africa 4590 30°19.025′N, 4°56.573′WMorocco/AlgeriaFind: June 2006Achondrite (angrite)

History: Scattered fragments from a small stone whichappears to have shattered upon landing recently wererecovered from an area of ~40 m2 in the Morocco-Algeriaborder zone, 21 km SSW of Tamassint oasis and 18 km S ofAgoult, Morocco. G. Hupé purchased all the recoveredmaterial in June 2006 in Tagounite, Morocco. He thentraveled to Tamassint and was shown the location by theoriginal find and measured GPS coordinates. Physical characteristics: Fragments totaling 212.8 g of avery friable specimen composed of coarse yellow-green,black and white grains; very fresh with preserved shiny, blackfusion crust on some pieces, and minor pale orange terrestrialweathering coatings on some broken surfaces.Petrography: (A. Irving and S. Kuehner, UWS) Coarse-grained (mostly 0.6–1.6 mm, but some olivine grains up to12 mm) with a cumulate texture and composed ofclinopyroxene (33 vol%, with rare pigeonite exsolutionlamellae), pure anorthite (28 vol%), olivine (14 vol%, withprominent subparallel exsolution lamellae 10–50 micronswide of kirschsteinite), kirschsteinite (5 vol%, with thinexsolution lamellae of olivine), ulvöspinel (18 vol%), andaccessory glass, troilite merrillite, Ca silicophosphate, andkamacite (making up the remaining 5 vol%). Some anorthiteoccurs as subhedral grains partially enclosed within largeulvöspinel grains, but most occurs as intercumulus aggregates.Clinopyroxene is strongly zoned with paler-colored, corrodedcores surrounded by darker purple-brown mantles and distinctrims. Thin (5–50 μm wide) discontinuous, curvilinear zones ofglass are present on some grain boundaries (notably thosebetween anorthite and ulvöspinel, but also around and cuttingacross troilite grains), and are associated with secondaryclinopyroxene, kirschsteinite, olivine, anorthite, and troilite

grains; these films of glass + daughter minerals truncatekirschsteinite exsolution lamellae in adjacent olivine. Thisangrite is unlike other known specimens, having neither afine-grained quench or ophitic/intersertal basaltic texture nor acoarse metamorphic texture.Mineral compositions and geochemistry: Clinopyroxene(Fs20.8–33.3Wo53–54.9; FeO/MnO = 85–278), olivine host(Fa72.6–74.7Ln3.5–3.6; FeO/MnO = 70–87), kirschsteinitelamellae (Fa44.7–45.4Ln46–47.2; FeO/MnO = 73–82),kirschsteinite host (Fa46.6–47.5Ln43.6–45.5; FeO/MnO = 63–68),olivine lamellae (Fa75–76.7Ln2.7–2.8; FeO/MnO = 71–74).Oxygen isotopes: (D. Rumble, CIW) Analyses of two aliquotsof acid-washed mineral fragments by laser fluorination gave,δ18O = 3.845, 3.881; δ17O = 1.927, 1.967; Δ17O = 0.0956,0.0745 (all ‰).Classification: Achondrite (angrite).Specimens: A total of 20.01 g of sample, two polished thinsections and two polished mounts are on deposit at UWS, and4 g at PSF. GHupé holds the main mass.

Northwest Africa 4615Northwest AfricaFind: 2006Rumuruti chondrite (R3.4)

History: The meteorite was recovered by an anonymoushunter in the western part of the Sahara and purchased byJ. Nauber in Morocco in 2006. Physical characteristics: A 10.5 g stone. Petrography: (A. Greshake, MNB) Various textural types ofchondrules with clearly defined outlines as well as chondruleand mineral fragments, all embedded in a dark, fine-grainedmatrix. The meteorite appears unbrecciated in the thin sectionstudied. Mineral compositions: Olivine (Fa23.9±14.7; range Fa2.4–41.5),low-Ca pyroxene (Fs14.5±6.9; range Fs3.8–25.3). Classification: Rumuruti chondrite (R3.4); S2, moderateweathering. Type specimens: A total of 2.9 g of sample plus one polishedthin section are on deposit at MNB. JNMC holds the mainmass.

Northwest Africa 4619Northwest AfricaFind: 2006Rumuruti chondrite (R3–5)

History: The meteorite was collected by an anonymousfinder in the western part of the Sahara and bought byJ. Nauber in Morocco in 2006. Physical characteristics: A 704 g stone. Petrography: (A. Greshake, MNB) A brecciated chondritewith dark and brighter lithologies ranging from petrologicaltype 3 to 5. Mineral compositions: Olivine (Fa36; range Fa23–39), low-Capyroxene (Fs18.2; range Fs9.7–29.6).

1662 H. C. Connolly, Jr., et al.

Classification: Rumuruti chondrite (R3–5); S2, moderateweathering. Type specimens: A total of 20.8 g of sample plus onepolished thin section are on deposit at MNB. JNMC holds themain mass.

Northwest Africa 4624Northwest AfricaFind: 2006Achondrite (eucrite)

History: The meteorite was recovered by an anonymouscollector in the northern part of the Sahara and bought byJürgen Nauber in Ensisheim, France, in 2006. Physical characteristics: Two stones totaling 175 g. Petrography: (A. Greshake, MNB). An unbrecciatedachondrite mainly consisting of exsolved pyroxene and calcicplagioclase displaying a cumulate texture. Minor phasesinclude chromite, pyrrhotite, troilite, and SiO2. The meteoritecontains several dark shock veins. Mineral compositions: Pyroxene (Fs35.5–43.3Wo2.7–15.6) andplagioclase (An91.1–93). Classification: Achondrite (eucrite); extensive shock;moderate weathering. Type specimens: A total of 21.5 g of sample plus onepolished thin section are on deposit at MNB. JNMC holds themain mass.

Northwest Africa 4636Northwest Africa Find: 2005 Mesosiderite

History: The meteorite was collected by an anonymousfinder in the western part of the Sahara and bought by themain mass holder at a meteorite fair in Germany from twodifferent dealers. Physical characteristics: Several dark stones totaling2850 g.Petrography: (A. Greshake, MNB and M. Kurz, Kurz). Thestony portion of the meteorite consists of dominant pyroxene,plagioclase, and phosphates. Minor phases include troilite,silica, and small metallic Fe-Ni grains. Metal is mostlykamacite. Mineral compositions and geochemistry: Pyroxene(Fs31.1–35.0 Wo4.8–9.1), plagioclase (An94.5; range An91.8–95.5).Oxygen isotopes: (I. A. Franchi and R. C. Greenwood, OU)The mean of two replicates δ17O = 2.09, δ18O = 4.38, Δ17O =−0.19 (all ‰). Classification: Mesosiderite; minimal shock and moderateweathering. Type specimens: A total of 29 g of sample plus one polishedthin section are on deposit at MNB. The anonymous purchaserholds the main mass.

Northwest Africa 4677Northwest AfricaFind: July 2006Achondrite (eucrite, monomict)

History: F. Béroud purchased the meteorite in July 2006 atSte Marie-aux-Mines, France. According to the Moroccanseller, the meteorite was found in the Sahara and other pieceshad been previously sold.Physical characteristics: A single, complete, partiallycrusted stone weighing 156.4 g. Petrography: (A. Seddiki, Ud’OEA and UJM; B. Moine,J. Y. Cottin, UJM; B. Devouard, UBP and M. Denise,MNHNP). The rock is brecciated and transected by impactmelt veins. Undeformed clasts mostly consist of pyroxeneand plagioclase grains (1–4 mm) with a cumulative texture.The pyroxenes are pigeonites with very fine (<1 μm)exsolution lamellae. These clasts are embedded in a finergrained clastic matrix of the same nature. Accessory phasesinclude spinel and taenite-kamacite-troilite assemblages andsilica. Mineral compositions and geochemistry: Spinel (Fe,Ti-richchromite, Cr2O3 = 45 wt%), plagioclase (An91), pigeonite(Fs41.20–42.40Wo7–10), pyroxene (Fe/Mn = 27–32). Kamacite(Ni = 4.9) and taenite (Ni = 38.5–44.6, both wt%). Classification: Achondrite (eucrite, monomict); S3, minimalweathering. The meteorite is similar to Dhofar 007 and EET92023. Type specimens: A type specimen of 20.2 g is on deposit atMNHNP and two sections are kept at UBP. Béroud holds themain mass.

Northwest Africa 4678MoroccoFind: August 2006Achondrite (diogenite)

History: F. Béroud purchased the meteorite in August 2006 inRissani, Morocco. Physical characteristics: A 3.60 g individual, oriented,nearly complete stone with black fusion crust overapproximately 90% of the specimen.Petrography: (A. Seddiki, UO and UJM; B. Moine, J. Y.Cottin, UJM; B. Devouard, UBP; M. Denise, MNHNP). Thestone is composed predominantly of Ca-poor pyroxene withsmall inclusions of spinel and troilite. Mineral compositions and geochemistry: Ca-poorpyroxene (Fs29.8–28.6Wo3.5–4.1), pyroxene (Fe/Mn = 26.4–31.8 [atomic]). Spinel Ti-poor chromite (Cr2O3 =56 wt%).Classification: Achondrite (diogenite); minimum shock andweathering. Type specimens: The main mass of 3.34 g is deposited atMNHNP and one thin section is kept at UBP.

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Northwest Africa 4693MoroccoFind: 2006Rumuruti chondrite (R3–6)

History: The meteorite was recovered by an anonymousfinder in western part of the Sahara and bought by the mainmass holder in Erfoud, Morocco, in 2006. Physical characteristics: One stone weighting 866.2 g. Petrography: (A. Greshake, MNB). A brecciated chondritewith pronounced dark and brighter lithologies ranging frompetrological type 3 to 6. Mineral compositions: Olivine (Fa24.3; range Fa4.6–39.2) andlow-Ca pyroxene (Fs30; range Fs2.3–34.7). Classification: Rumuruti chondrite (R3–6); S2, moderateweathering. Type specimens: A total of 24.3 g of sample plus onepolished thin section are on deposit at MNB. HSSH holds themain mass.

Northwest Africa 4747MoroccoFind: 2001Mesosiderite

History: Purchased in Alnif, Morocco, in 2001 by B. Fectay.Physical characteristics: A single rounded stone of 1.2 kgwith no fusion crust. Petrography: (A. Yamaguchi, NIPR). The thin sectionreveals a breccia composed of silicate fragments (<1 mm)(~80 vol%) in a matrix of Fe, Ni-rich metal and minor troilite.There are a few large nodules of metallic Fe-Ni(<several mm). The silicate fragments are mainly pyroxene,plagioclase, and minor silica minerals. Mineral compositions: (A. Yamaguchi, NIPR). Low-Capyroxene (Fs28.3–32.5Wo0.8–2.6; FeO/MnO = ~30) andplagioclase (An87.9–90.7). Classification: Mesosiderite. Type specimens: A total of 20.9 g of sample and one thinsection is on deposit at NIPR. Fectay holds the main mass.

A list of all meteorites approved from Northwest Africa ispresented in Table 2.

THE AMERICAS

North America

Richland (Fredericksburg)A 47 kg iron meteorite was reportedly found nearFredericksburg, Texas. Chemical analysis (Wasson et al.2007) showed that it is indistinguishable from Richland, a13.6 kg IIAB iron that was found ~300 km away. It is likelythat these meteorites are paired and that one (or both) masseswere transported by humans from their original find locations.Henceforth, the name Fredericksburg shall be an unofficial

synonym for Richland. The new mass may be referred to as“Richland (Fredericksburg).” A total of 213 g is on deposit atUCLA.

South America

Peru

Cerro La Tiza 14°31′59.56′′S, 75°46′30.40′′WCerro La Tiza, Ica, PeruFind: September 14, 2002Ordinary chondrite (H4)

History: K. Hönninger and N. Diaz Zegarra recovered thismeteorite in the course of an expedition. Physical characteristics: The meteorite consists of threepieces with a total mass of 3740 g (3475 g, 235 g, and 30 g).Fragments are irregularly formed, shiny and of brownishcolor with very small black patches of fusion crust left. Petrography: (S. P. Schwenzer, MPI and J. Zipfel, SNG)Sharply defined chondrules up to 0.8 cm in diameter. In rarechondrules turbid glass is observed. Fragments are fractured.Along cracks weathering is more pronounced. Mineral compositions and geochemistry: Olivine(Fa17.9±0.2) and pyroxene (Fs15.9±0.4), both homogeneous.Classification: Ordinary chondrite (H4); S3, W3.Type specimens: A total of 97 g of sample and one thinsection on deposit at MPI. The finders hold the main mass.

ANTARCTICA

ANSMET

Meteorites collected by Antarctic Search for Meteorites(ANSMET) teams and their collaborators between 1976 and1981 officially have the letter A before their number, e.g.,Allan Hills A77307, abbreviated ALHA77307. However,the use of this letter A is henceforth to be consideredoptional. Thus, Allan Hills 77307, abbreviated ALH 77307,is equally correct and equivalent to the official name andabbreviation.

Table 3 lists 1213 meteorites recovered from Antarctica bythe ANSMET program during the 2003 through 2005seasons. For more information on these meteorites, pleasevisit the curation home page of the Johnson Space Center,National Aeronautic and Space Administration, at http://curator.jsc.nasa.gov.

PNRA

Table 4 lists meteorites collected by the Italian team,Programma Nazionale Ricerche in Antartide (PNRA)recovered from the Allan Hills blue ice field (Victoria Land,Antarctica) in November 2006. Mineralogy and classification

1664 H. C. Connolly, Jr., et al.

performed by L. Folco (MNA-SI) and P. Rochette (CEREGE).Magnetic classification was conducted according to Rochetteet al. (2003) and Folco et al. (2006) using a SM30susceptivimeter. All main masses and type specimens are ondeposit at MNA-SI.

PRIC

Table 5 lists meteorites collected by the Chinese AntarcticExpedition to Grove Mountains, Antarctica, in 2006 andsubmitted through the Polar Research Institute of China(PRIC).

Grove Mountains 052049 72°46′23′′N, 75°20′8′′EGrove Mountains, AntarcticaFind: January 16, 2006Ordinary chondrite (L5)

History: X. Liu recovered the stone in a large moraine west tothe northern part of Gale Escarpment in Grove Mountains.Physical characteristics: It is a round stone mostly coveredwith fusion crust. The meteorite weights 96.7 g. Magneticsusceptibility: logχ = 4.60 × 10−9 m3/kg.Petrography: (Y. Lin, B. Miao, S. Hu, and L. Feng,IGGCAS). It contains large melt veins (>3 mm thick) withabundant rounded silicate clasts embedded inmicrocrystalline matrix. Olivine grains in the melt veinscommon have FeO-rich ringwoodite rims and FeO-poorwadsleyite interiors. Chondrules in the unmolten parts arerecognized.Mineral compositions: olivine (Fa24.0±0.4); low Ca-pyroxene(Fs20.6±0.5).Classification: Ordinary chondrite (L5); S6, W1Type specimen: All of the mass is on deposit at PRIC.

Grove Mountains 055364 72°59′36′′N, 75°13′6′′EGrove Mountains, AntarcticaFind: January 9, 2006Mesosiderite

History: X. Chen recovered the meteorite in a large morainewest of the middle of the Gale Escarpment in GroveMountains. Physical characteristics: A 396.4 g meteorite with a roundshape and many concaved areas. Part of the black fusion crustremains.Petrography: (Y. Lin, B. Miao, S. Hu, and L. Feng,IGGCAS). It contains 23.9 vol% metallic Fe-Ni. The silicatepart consists mainly of low-Ca pyroxene (61.8 vol%),plagioclase (32.3 vol%), and silica (5.9 vol%), with minorolivine, chromite, and phosphates. Olivine occurs as clastswith embayed outlines and is surrounded by layers of low-Capyroxene and fine-grained chromite. Low-Ca pyroxene grainsare nearly homogeneous, without exsolved lamellae of Ca-pyroxene. Phosphates commonly occur along the boundariesof Fe,Ni-rich metal with minor schreibersite.

Mineral compositions and geochemistry: Olivine(Fa27.9±3.1; FeO/MnO = 37 ± 3), low Ca-pyroxene (Fs29.5±3.8;FeO/MnO = 22 ± 2), and plagioclase (An88.7–90.3Ab9.0–11.1).

Classification: Mesosiderite; minimal weathering. Type specimens: The entire sample is on deposit atPRIC.

ASIA

Arabian PeninsulaThe Meteoritical Bulletin announces a new name series,Arabian Peninsula (AP), approved after considerable debateby the Nomenclature Committee of the Meteoritical Society.

The five approved meteorites listed below, along withreportedly 18 ordinary chondrites, were recovered near theRub al-Khali Desert (Empty Quarter) by workers in 2005 and2006. They were all sent to an anonymous American collectorfor verification in August 2006.

Arabian Peninsula 001United Arab EmiratesFind: 2006Achondrite (diogenite)

History and physical characteristics: This 145 g stone isvery fresh with black crust and flow ridges.Petrography: (T. Bunch and J. Wittke, NAU) Unbrecciatedmedium-grained orthopyroxenite with inclusions of euhedralchromite crystals. Contains 94 vol% orthopyroxene, 4 vol%chromite, 2 vol% FeS, and trace olivine. Orthopyroxeneexhibits heavy undulatory extinction, shear zones showintense granulation and distortion of minerals.Mineral compositions and geochemistry: Orthopyroxene(Fs21.6Wo2.0; FeO/MnO = 29), olivine (Fa27.3, FeO/MnO = 45)and chromite (Cr/[Cr + Al] = 79).Classification: Achondrite (diogenite); moderate shock,minimum weathering.Type specimen: A 21 g sample is on deposit at NAU. Themain mass holder is anonymous.

Arabian Peninsula 002United Arab EmiratesFind: 2006Achondrite (eucrite)

Physical characteristics: A dark, 54 g completely crustedstone.Petrography: (T. Bunch and J. Wittke, NAU). Eucritebreccia with ophitic to subophitic textures. Containspigeonite, augite, plagioclase, FeS, metal, and SiO2.Pigeonite cores are rimmed by subcalcic augite. Pigeonitebasal sections show well-developed twinning andplagioclase has extensive Carlsbad-albite twinning.Mesostasis pockets consist of fine-grained intergrowths ofplagioclase, SiO2, and FeS.

The Meteoritical Bulletin, No. 92 1665

Mineral compositions and geochemistry: Pigeonite cores(Fa41.4Wo8.2; FeO/MnO = 30), subcalcic augite rims(Fs46Wo21.6; FeO/MnO = 29) and plagioclase (An84.2–92.2).Classification: Achondrite (eucrite); minimal shock, minimalweathering with minor carbonate/ iron oxide veins.Type specimen: A 10.8 g sample is on deposit at NAU. Themain mass holder is anonymous.

Arabian Peninsula 003United Arab EmiratesFind: 2006Achondrite (diogenite)

Physical characteristics: A 56 g stone that has been heavilysandblasted, no crust remains.Petrography: (J. Wittke and T. Bunch, NAU) Unbrecciatedwith well-developed preferred orientation of orthopyroxene.Large chromite crystals (<2 mm) are surrounded by a corona-like “necklace” of very small orthopyroxene and olivinegrains. Chromite also has very tiny (<0.01 mm) inclusions ofpigeonite, diopside, plagioclase, and FeS. Small grains ofFeS, metal, and clusters of olivine occur as inclusions incumulate orthopyroxene.Mineral compositions and geochemistry: Orthopyroxene(Fs23.5Wo2.3; FeO/MnO = 28), orthopyroxene inclusions(Fs21Wo2.7; FeO/MnO = 28), olivine (Fa25.5; FeO/MnO = 43),diopside inclusions (Fs11.1Wo42), and chromite (Cr/[Cr + Al]= 0.76). Classification: Achondrite (diogenite); minimal shock,weathering in the interior is minimal. Type specimen: A 11.2 g sample is on deposit at NAU. Themain mass holder is anonymous.

Arabian Peninsula 004United Arab EmiratesFind: 2006Achondrite (diogenite)

Physical characteristics: A 31 g stone that is partiallycovered with a dull black fusion crust.Petrography: (T. Bunch and J. Wittke, NAU) Protogranulartexture with several poikilitic grains of orthopyroxene hostand rounded olivine inclusions. Mineral modes (vol%):orthopyroxene = 94, olivine = 4, chromite, metal, and FeS = 2.Mineral compositions and geochemistry: orthopyroxene(Fs24.3Wo3.7; FeO/MnO = 28), olivine (Fa30.3; FeO/MnO =45), chromite (Cr/[Cr + Al] = 66), metal (Ni = 3.1 wt%).Classification: Achondrite (diogenite); minimal shock,minimal weathering. Type specimen: A 7 g sample is on deposit at NAU. The mainmass holder is anonymous.

Arabian Peninsula 005United Arab EmiratesFind: 2005Achondrite (eucrite, monomict breccia)

Physical characteristics: A brownish 146 g stone,

with no fusion crust, partially desert-etched bysandblasting.Petrography: (J. Wittke and T. Bunch, NAU) Porphyroclastictexture of relict cumulate basalt clasts surrounded by a fine-grained matrix of recrystallized basalt. Thin, shock-melt veinstranscend the sample. Prominent iron oxide stainingsurrounds metal grains.Mineral characteristics and geochemistry: Pigeonite(Fs52.5Wo8.7; FeO/MnO = 33), augite (Fs42.8Wo27.2), chromite(Cr/[Cr + Al] = 75), and plagioclase (An90.5).Classification: Achondrite (eucrite, monomict breccia);moderate shock and weathering. Type specimen: A 21 g sample is on deposit at NAU. Themain mass holder is anonymous.

Arabian Peninsula 006United Arab EmiratesFind: 2005Achondrite (eucrite, monomict breccia)

Physical characteristics: A 67 g stone that has somewhatweathered fusion crust and desert staining.Petrography: (J. Wittke and T. Bunch, NAU) A fine-grained,eucrite monomict breccia. Ophitic- to subophitic-textured,plagioclase contains numerous, tiny (<0.02 mm) orientedeuhedral pyroxene crystals. Has a moderate degree ofundulatory extinction in plagioclase and pyroxenes. Containsorthopyroxene, pigeonite, augite, plagioclase, ilmenite,chromite, FeS, and metal.Mineral compositions and geochemistry: Orthopyroxenehost (Fs56.6Wo2.2; FeO/MnO = 29), augite exsolution lamellae(Fs28.8Wo43.6), pigeonite (Fs52Wo8.7; FeO/MnO = 33), andchromite (Cr[Cr + Al] = 84).Classification: Achondrite (eucrite, monomict breccia);minimal shock and weathering.Type specimen: A 13.5 g sample is on deposit at NAU. Themain mass holder is anonymous.

China

Weikengquan 40°16′N, 99°49′EJiuquan City, Gansu Province, ChinaFind: November 2, 2006Ordinary chondrite (H5, breccia)

History: The stone lay on sand close to dunes at thenorthwestern boundary of the Badanjilin Desert. H. Zangrecovered the stone on the way from the base toWeikengquan.Physical characteristics: The stone is 665 g, roughly ball-shaped and ~10 cm in diameter. It has a complete fusion crustwith many cracks penetrating inside. Sand grains adhere onthe crust.Petrography: (Y. Lin, B. Miao and S. Hu, IGGCAS) It is abrecciated chondrite, consisting of numerous almond-likeclasts cemented by fine-grained impact melt. In the clastschondrules are readily recognized, and troilite is much more

1666 H. C. Connolly, Jr., et al.

abundant than metallic Fe-Ni. In the melt breccias, metallicFe-Ni and troilite occur as small spheres, and there arenodule-like clasts with ringwoodite rims and wadsleyiteinterior.Mineral compositions: Olivine (Fa19.4±0.4) and low Ca-pyroxene (Fs17.1±0.2) are homogeneous, but plagioclase showsvariation An11.7–20.6Ab69.8–85.5Qr1.5–10.6). Magneticsusceptibility: logχ = 4.45 × 10−9 m3/kg.Classification: Ordinary chondrite (H5, breccia); S6, W3.Type specimens: A sample of 359 g is on deposit at IGGCAS.The finder holds 306 g.

Oman

Dhofar 1427 19°6.771′N, 54°49.126′EQitbit, Dhofar, OmanFind: January 17, 2001Achondrite (ureilite)

History: A meteorite was found by an anonymous finder inthe Omani desert about 34 km ESE of Qitbit on January 17,2001. Physical characteristics: The meteorite is a single darkbrown stone of 12.92 g with a magnetic susceptibility oflogχ = 4.57 × 10−9 m3/kg. Petrography: (Bartoschewitz, Bart) Coarse-grained texturewith triple junctions and curved grain boundaries formed bylarge (1–2 mm) elongated recrystallized olivines and minorpyroxenes (<1 mm). Grain boundaries are outlined by darkcarbonaceous matrix material with finely dispersed metal. Mineral composition and geochemistry: (Bartoschewitz,Bart and P. Appel, B. Mader, Kiel) Olivines (Fo74.2–79.8, CaO= 0.34, and Cr2O3 = 0.64 [all in wt%], Fe/Mn = 51); andpyroxenes, Fs13.0–21.6, Wo1.4–9.1, Cr2O3 = 0.97 (in wt%). Classification: Achondrite (ureilite) with mosaicised typicaltexture. Type specimens: A total of 2.6 g of sample is on deposit at

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′′EOman, Al WustaFind: February 13 and November 6, 2004Carbonaceous chondrite (CH3)

History: Sixty-four fragments were discovered within adistance of ~10 m by Rainer and Claudia Bartoschewitzduring a natural science expedition on a gravel plateau ofMiocene fresh-water limestone of Middle Fars group about35 km SSW of Ghaba Resthouse (Adam County).Physical characteristics: Sixty-four fragments weighingbetween 0.2 to 888 g amount to a total of 1.796 kg.Petrography: The meteorite is mostly composed of smallchondrules (<20 μm) of various textural types, ~15% fine-grained metal, few small “matrix lumps,” and rare refractoryinclusions.Mineral composition and geochemistry: (R. Bartoschewitz,Bart, P. Appel and B. Mader, Kiel, M.I. Prudêncio, ITN,U. Krähenbühl, Bern) Pyroxene (Fs3.99–5.16 Wo3.01–1.80; Al2O3= 1.90, Cr2O3 = 0.62 [wt%]), Ti-rich pyroxene (Fs2.88Wo19.66;Al2O3 = 10.40, Cr2O3 = 1.27 [wt%]), olivine (Fa1.88–0.83, CaO= 0.43–0.27, Al2O3 = 0.27, Cr2O3 = 0.47 [all wt%]), sulfide(Ni = 0.4–21.7 [wt%]), kamacite (Ni = 3.7–8.0, Co = 0.35–0.56, Si = 0.02–0.15, Cr = 0.08–0.40 [all wet%]), tetrataenite(Ni = 59.2, Co = 1.45 [wt%]). Whole rock siderophile,chalcophile, and lithophile element abundances similar toother CHs. Magnetic susceptibility: logχ = 5.2 × 10−9 m3/kg.Noble gas isotopes (J. Park and K. Nagao, UTokE, Japan,R. Okazaki, KyuU) high concentrations of solar noble gases.O isotopes (M. Kusakabe, OkaU) 17O = 1.91‰, 18O = 5.71‰.Classification: Carbonaceous chondrite (CH3); moderateweathering. Type specimens: A total of 20.1 g are on deposit UTokE. Bartholds 1500 g and one thin section.

Table 6 lists all approved meteorites from Asia.

EUROPE

Sweden

The Nomenclature Committee has recognized the newcategory of relict meteorites. From the Guidelines forMeteorite Nomenclature, http://www.meteoriticalsociety.org/bulletin/nc-guidelines.htm#s77, a relict meteorite is definedin such a fashion that special provisions are made for highlyaltered materials that may have a meteoritic origin,designated relict meteorites, which are dominantly (>95%)composed of secondary minerals formed on the body onwhich the object was found. Examples of such material mayinclude some types of “meteorite shale,” “fossil meteorites,”and fusion crust (as defined in section 1.2 of the guidelines).

Fig. 2. An image of Österplana 002.

The Meteoritical Bulletin, No. 92 1667

The naming of relict meteorites is defined in section 7.7 of theguidelines. A special type of name should be assigned to relictmeteorites. The documentation required for these names mustinclude a description of the material, the location and date ofthe find, the approximate mass or size, the location of themain mass, and the type of meteoritic material it is suspectedto represent. The name must conform to all applicable parts ofsections 2–6 of the guidelines, and must be approved by theNomenclature Committee prior to publication. Relictmeteorite names may be converted to formal meteorite namesby a second vote of the committee, subject to the requirementsof section 7.1 of the guidelines.

Reported in Table 7 are two new name series, Österplana andGullhögen. Both are relict of ordinary chondrites recoveredfrom strata of Ordovician age.

ERRATA

Errata to previous editions of The Meteoritical Bulletin.

The Meteoritical Bulletin, No. 85, 2001

In Table 4, NWA 265 is listed with coordinates of recovery.However, these coordinates should be disregarded and, aspublished, they are unknown.

The Meteoritical Bulletin, No. 88, 2004

In Table 5, Dhofar 607 is listed with coordinates of recoveryas 10°43.728′N, 54°11.432′E. The correct coordinates are18°43.728′N, 54°11.432′E.

The description for Maromandia reports coordinates ofrecovery as 48.1°S 14.2°E. The correct coordinates ofrecovery should be 14.2°S 48.1°E.

The Meteoritical Bulletin, No. 89, 2005

In Table 2, Little Spring Creek is listed as having a mass of29,500 g. The correct mass is 2950 g.

To Table 5, the following changes are made: Dhofar 543: H6,S3, W2; Fa19.7±0.14; Fs17.2±0.25, Wo1.13±0.02; Chromite (Al2O3 =7.8, 2.6% MgO = 2.6, MnO = 0.9 [all wt%]). Whitlockite isobserved. Dhofar 545: LL4 (breccia), S2, W2; Fa31.4±1.02;Fs25.6±0.73; Wo2.45±0.08.

In Table 7, NWA 774 is listed with a mass of 523 g, purchasedin Tucson in 2001, and the main mass is located at the SWML.The correct mass is 1440 g, it was purchased from ananonymous collector in 2000, and Tobin holds the main mass.

In Table 7, NWA 775 is listed with a mass of 1440 g and the

main mass as located at the SWML. The correct mass is3280 g and Tobin holds the main mass.

In Table 7, NWA 2738 and 2739 are reported as beingclassified by Ted Bunch with the type specimen at NAU. Itshould read that V. Moggi-Cecchi and G. Pratesi of MSP asclassifiers with the type specimen at MSP.

The Meteoritical Bulletin, No. 90, 2006

In Table 2, NWA 2457 is classified as an impact melt clast butit should be listed as an impact melt breccia. Furthermore, thefollow additions to NWA samples should be printed withinthe comment column of Table 2: NWA 3347: breccia; NWA3349: shock veins; NWA 3351: breccia, impact-shock brecciaclasts; NWA 3352: calcite veins; NWA 3353: shock veins,ringwoodite, partly S6; NWA 3355: calcite vein; NWA 3356:shock veins; NWA 3357: shock veins, breccia, shockdarkening; NWA 3359: An79±6, shock veins, breccia,polymict, impact-melt clasts, impact melt breccia clasts;NWA 3360: breccia, impact-melt clasts; NWA 3361: shockveins, breccia, impact melt breccia clasts; NWA 3362: shockveins, breccia, shock darkening; NWA 3363: shock veins,breccia, shock darkening; NWA 3364: breccia; NWA 3365:shock veins, breccia; NWA 3367: breccia, shock veins.

In Table 5, Dhofar 1301 is printed on June 15, 2006; however,this sample was shown to be the same as Dhofar 1286. Dhofar1301 is thus not a valid name and is not official.

In Table 6, Minas Gerais b is incorrectly listed. It should belisted as Minas Gerais (b).

The Meteoritical Bulletin, No. 91, 2007

In Table 1, Tanezrouft 88 and 89 should be 088 and 089.

In Table 2, NWA 969 is listed as an LL7. It should be LL6/7.

In Table 2, NWA 2748 is listed as L 3.4. It should be listed asLL 3.4.

In Table 2, NWA 2954 is listed as having a 145 g. This shouldbe 1246 g. The main mass is listed as being held by Reed;however, Martinez holds the main mass.

In Table 3, Santa Vitoria do Palmar is incorrectly spelled asSanta Vitorio do Palmar. It is also listed with a mass of5910.0 g but this should be 50,360 g. The correct coordinatesof recovery, both in the write-up and in Table 3, are33°30′34′′S, 53°24′39′′W.

In Table 5, Dhofar 962 was recovered on January 6, 2004.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 onJanuary 10, 2004. Dhofar 1400 was recovered onNovember 25, 2003. UAE 001 was recovered on January18, 2005.

REFERENCES

Chennaoui Aoudjehane H., Jambon A., and Rjimati E. 2007. AlHaggounia (Morocco) strewn field (abstract #5329). Meteoritics& Planetary Science 42:A30.

Folco L., Rochette P., Gattacceca J., and Perchiazzi N. 2006. In situidentification, pairing, and classification of meteorites fromAntarctica through magnetic susceptibility measurements.Meteoritics & Planetary Science 41:343–353.

Irving A. J., Kuehner S. M., Korotev R. L., and Hupé G. M. 2007a.Petrology and bulk composition of primitive enriched olivinebasaltic shergottite Northwest Africa 4468 (abstract #1526). 38thLunar and Planetary Science Conference. CD-ROM.

Kuehner S. M. and Irving A. J. 2007. Grain boundary glasses in theTamassint plutonic angrite: Evidence for rapid decompressivepartial melting and cooling on Mercury (abstract #1522)? 38thLunar and Planetary Science Conference. CD-ROM.

Kuehner S. M., Irving A. J., Korotev R. L., Hupé G. M., and Ralew S.2007. Zircon-baddeleyite-bearing silica + K-feldspargranophyric clasts in KREEP-rich lunar breccias NorthwestAfrica 4472 and 4485 (abstract #1516). 38th Lunar and PlanetaryScience Conference. CD-ROM.

Rochette P., Sagnotti L., Bourot-Denise M., Consolmagno G.,Folco L., Osete M. L., and Pesonen L. 2003. Magneticclassification of stony meteorites: 1. Ordinary chondrites.Meteoritics & Planetary Science 38:251–268.

Wasson J. T., Huber H., and Malvin D. J. 2007. Formation of IIABiron meteorites. Geochimica et Cosmochimica Acta 71:760–781.

ABBREVIATIONS

Classifiers, Type Specimen Locations, Finders, andHolders of Main Masses

A key to abbreviations for addresses used in the MeteoriticalBulletin is found at our web site, http://tin.er.usgs.gov/meteor/MetBullAddresses.php.

Listed throughout most of the tables within the “Info” columnare relevant data on who classified the samples, where thetype specimen is located, etc. Below is a key to theabbreviations used within this edition.

AMSA-1: Pickard, Williams, and McKinnon. Type specimen,AMAS. Main mass: Bessy.

AMSA-2: Classified: Pickard, Williams, and McKinnon, AMAS.Type specimen, AMAS. Main mass: Bathurst.

AMSA-3: Classified: Pickard, Williams and McKinnon, AMAS.Type specimen, AMAS. Main mass: Anonymous.

IZU-1: Classified: A. Ibhi, H. Nachit, IZU; H. ChennaouiAoudjehane, UHAC. Main mass: IZU.

LundU-1: Classified: B. Schmitz and M. Tassinari, LundU. Typespecimen: LundU. Main mass: LundU.

LundU-2: Classified: B. Schmitz and M. Tassinari, LundU. Typespecimen: LundU. Main mass: Undisclosed.

LundU-3: Classified: B. Schmitz. Type specimen: LundU. Mainmass: LundU.

MNA-SI-1: Classified: L. Folco, MNA-SI. Type specimen: OAM.Main mass: OAM.

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:MNHNP. Main mass: Goueslain and Parodi.

MNHNP-3: Classified: M. Bourot-Denise, MNHNP. Type specimen:MNHNP. Main mass: P. Thomas.

MNHNP-4: Classified: M. Bourot-Denise, MNHNP. Type specimen:MNHNP. Main mass: Giessler.

MSP-1: Classified: V. Cecchi Moggi and G. Pratesi MSP. Typespecimen: MSP. Main mass: MSP.

MNB-1: Classified: A. Greshake, MNB. Type specimen: MNB. Mainmass: Anonymous.

MNB-2: Classified: A. Greshake, MNB. Type specimen: MNB. Mainmass: Stehlik.

MNB-3: Classified: A. Greshake, MNB. Type specimen: MNB. Mainmass: HSSH.

MNB-4: Classified: A. Greshake, MNB. Type specimen: MNB. Mainmass: Ralew.

NAU-1: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Farmer.

NAU-2: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Aaronson.

NAU-3: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Cimala.

NAU-4: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Hall.

NAU-5: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Boswell.

NAU-6: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Reed.

NAU-7: Classified: T. Bunch, NAU. Type specimen: NAU. Mainmass: Oaks.

NAU-8: Classified: T. Bunch and Wittke, NAU. Type specimen:NAU. Main mass: Boswell.

NAU-9: Classified: T. Bunch and Wittke, NAU. Type specimen:NAU. Main mass: Aaronson.

NIPR-1: Classified: A. Yamaguchi, NIPR. Type specimen: NIPR.Main mass: Fectay.

Ud’OEA-1: Classified: A. Seddiki, Ud’OEA and UJM;B. Moine, J. Y. Cottin, UJM; M. Denise, V. Sautter, J. P.Lorand, MNHNP. Type specimen: MNHNP and UJM. Mainmass: Anonymous.

UWS-1: Classified: A. Irving, UWS. Type specimen: UCLA andUWS. Main mass: Gregory.

UWS-2: Classified: A. Irving, UWS. Type specimen: UWS. Mainmass: Gregory.

UWS-3: Classified: A. Irving, UWS. Type specimen: UWS. Mainmass: PSF.

UWS-4: Classified: A. Irving, UWS. Type specimen: UWS. Mainmass: GHupé.

UWS-5: Classified: A. Irving, UWS. Type specimen: UWS. Mainmass: AHupé.

UWS-6: Classified: A. Irving, UWS. Type specimen: UWS. Mainmass: Ralew.

UWS-7: Classified: A. Irving, UWS. Type specimen: UAz. Mainmass: Farmer.

UWS-8: Classified: A. Irving, UWS. Type specimen: UAz. Mainmass: Jirasek.

The Meteoritical Bulletin, No. 92 1669

Additional Abbreviations Used in the Text

For chondrule textural types: PO = porphyritic olivine, POP =porphyritic olivine pyroxene, PP = porphyritic pyroxene.

Abbreviations for the location meteorites recovered by ANSMET:

ALH = Allan Hills, CRS = Mount Cranfield, CMS = CumulusHills; DOM = Dominion Range; GRO = Grosvenor Mountains;LAP = LaPaz Icefield; LAR = Larkman Nunatak; MAC =MacAlpine Hills; MCY = MacKay Glacier; MIL = Miller Range;PRA = Mount Pratt, RBT = Roberts Massif, SAN = SandfordCliffs, and TYR = Taylor Glacier.

1670 H. C. Connolly, Jr., et al.

Tabl

e 1.

A li

st o

f met

eorit

es re

cove

red

from

spe

cific

loca

tions

with

in A

fric

a.

Nam

eLo

catio

n of

reco

very

Dat

e of

re

cove

ryFi

nd/

Fall

Latit

ude

(N)

Long

itude

(E

)

Tota

l kn

own

mas

s (g

)N

o. o

f pi

eces

Cla

ss

Type

sp

ecm

en

mas

s (g

)SS

WG

Fa (mol

%)

Fs (mol

%)

Wo

(mol

%)

Mag

netic

su

s(lo

g χ)

Info

Com

men

ts

Alg

eria

Acf

er 3

86Ta

man

ghas

set,

Alg

eria

Jan-

2004

Find

27°2

1.61

′03

°42.

00′

200

1L5

20.4

32

24.5

21.7

1.4

MSP

-1A

cfer

387

Tam

angh

asse

t, A

lger

iaJa

n-20

04Fi

nd27

°33.

48′

04°0

0.90

′17

76

H4-

622

.83

318

.514

.01.

2M

SP-1

Bre

ccia

ted

Acf

er 3

88Ta

man

ghas

set,

Alg

eria

Jan-

2004

Find

27°3

7′03

°52′

1072

1H

424

.61

318

.914

.71.

2M

SP-1

Acf

er 3

89Ta

man

ghas

set,

Alg

eria

Jan-

2004

Find

27°3

0.24

′03

°40.

90′

397

3H

521

.82

218

.616

.41.

2M

SP-1

Acf

er 3

90Ta

man

ghas

set,

Alg

eria

Jan-

2004

Find

27°3

0.15

′03

°41.

58′

578

1H

422

.32

119

.420

.41.

1M

SP-1

Ilafe

gh 0

17A

drar

, Alg

eria

Jan-

2004

Find

21°3

5.44

′01

°31.

45′

1063

7H

521

.52

218

.616

.61.

4M

SP-1

Plat

eau

du

Tade

mai

t 06

Adr

ar, A

lger

iaJa

n-20

04Fi

nd27

°22.

22′

00°4

2.37

′29

9524

LL6

23.8

14

30.7

24.9

2.1

MSP

-1

Sile

tTa

man

ghas

set,

Alg

eria

(R

ocky

des

ert)

Jan-

2004

Find

22°4

7′04

°09′

971

4L5

20.8

34

25.1

21.1

1.4

MSP

-1

Egy

ptG

reat

San

d Se

a 02

2A

l Wad

i al J

adid

, Egy

pt19

94Fi

nd25

°55′

25°4

0′0.

91

H6

0.7

S2W

219

.216

.8M

SP-1

Gre

at S

and

Sea

023

Al W

adi a

l Jad

id, E

gypt

1996

Find

25°1

0′25

°40′

1.5

1H

51.

4S4

/5W

318

.516

.2M

SP-1

Bre

ccia

ted

Gre

at S

and

Sea

024

Al W

adi a

l Jad

id, E

gypt

1996

Find

25°1

6.99

′25

°36.

50′

7.8

1H

57.

6S2

W1

18.8

16.5

MSP

-1G

reat

San

d Se

a 02

5A

l Wad

i al J

adid

, Egy

pt20

05Fi

nd25

°22.

41′

25°4

2.37

′10

.91

L510

.9S3

W3

23.8

20.1

MSP

-1

Lib

yaD

ar a

l Gan

i 104

3D

ar a

l Gan

i, Li

bya

12-D

ec-2

005

Find

27°2

6′

16°0

0′

32.1

1LL

630

S2W

430

.126

.1M

NA

-SI-

1D

ar a

l Gan

i 104

4D

ar a

l Gan

i, Li

bya

Nov

-200

6Fi

nd27

°27′

02′′

16°1

1′30

′′23

52

LL5

235

S3W

129

.123

.9M

NA

-SI-

1D

ar a

l Gan

i 104

7D

ar a

l Gan

i, Li

bya

16-M

ay-1

999

Find

27°0

2′09

′′16

°23′

07′′

49.8

1U

re10

.2M

odM

od3.

6–22

.43.

7–22

.4M

NB

-1Po

lym

ict

brec

cia

with

fin

e-gr

aine

d ch

ondr

itic

litho

logi

esD

ar a

l Gan

i 104

8D

ar a

l Gan

i, Li

bya

28-J

un-2

001

Find

27°1

2.10

′16

°18.

67′

0.80

11

Luna

r0.

33Se

e se

para

te

entry

Mau

rita

nia

Ada

m T

alha

Ada

m T

alha

, Mau

ritan

ia

(see

IGN

map

1/2

0000

0 fe

uille

NF-

29-X

IV)

28-J

an-2

005

Find

22°5

9.61

′10

°09.

22′W

259.

32

LL3.

221

S4W

20.

72–3

6.8

(10.

36 ±

12.

19)

1.22

–27.

46

(5.3

6 ±

10.8

6)4.

64M

NH

NP-

1

Bas

siko

unou

11 k

m S

E of

B

assi

koun

ou, H

odh

Ech

Cha

rgui

, Mau

ritan

ia

12-O

ct-2

006

Fall

15°4

7′

5°54

′W29

560

>20

H5

115

S2W

018

.616

.3Se

e se

para

te

entry

Rha

ll A

man

e 00

1R

hall

Am

ane,

M

aurit

ania

(see

IGN

m

ap 1

/000

000

Oua

dane

N

E-29

-30)

27-J

an-2

005

Find

23°1

7.55

′10

°10.

49′W

224

1H

420

.53

S3W

219

.89

± 0.

4817

.3 ±

0.3

1M

NH

NP-

2

Rha

ll A

man

e 00

2R

hall

Am

ane,

M

aurit

ania

(see

IGN

m

ap 1

/000

000

Oua

dane

N

E-29

-30)

25-J

an-2

005

Find

23°2

3.44

′9°

56.4

1′W

383

1LL

620

S2W

225

.81

± 0.

3922

.3 ±

0.5

6M

NH

NP-

2

Suei

lila

Suei

lila,

Mau

ritan

ia (s

ee

IGN

Map

1/1

0000

00

Cap

Boj

ador

NG

28)

10-F

eb-2

005

Find

24°3

8.18

′14

°42.

98′W

1326

61

LL6

61S1

W1

25.7

0 ±

0.28

21.8

6 ±

0.48

MN

HN

P-2

Mor

occo

Al H

aggo

unia

001

All

Hag

goun

ia,

Mor

occo

2006

Find

27°3

0′12

°30′

W~3

met

ric

tons

Man

yA

ubSe

e se

para

te

entry

Istif

ane

001

Istif

ane

regi

on,

sout

heas

tern

Mor

occo

17-A

ug-2

005

Find

31°2

9.91

1′5°

43.0

45′W

131.

63

H4

104

S3W

418

.4–1

9.2

16.2

–17.

5Se

e se

para

te

entry

Istif

ane

002

Istif

ane

regi

on,

sout

heas

tern

Mor

occo

17-A

ug-2

005

Find

31°2

9.90

9′5°

43.0

44′W

401

H5

40S5

W3

15.5

16.8

See

sepa

rate

en

tryIs

tifan

e 00

3Is

tifan

e re

gion

, so

uthe

aste

rn M

oroc

co17

-Aug

-200

5Fi

nd31

°29.

150′

5°43

.027

′W18

.51

L518

.5S5

W2

24.9

21.4

See

sepa

rate

en

tryIs

tifan

e 00

4Is

tifan

e re

gion

, so

uthe

aste

rn M

oroc

co19

-May

-200

6Fi

nd31

°30.

165′

5°42

.916

′W10

.81

H5

10.8

S2W

219

.115

.4Se

e se

para

te

entry

The Meteoritical Bulletin, No. 92 1671

Nig

eria

Gas

hua

Nea

r des

ert s

ettle

men

t K

olom

ari,

Gas

hua,

D

apch

i dis

trict

, Nig

eria

Apr

-198

4Fa

ll~1

2°51

′ ~1

1°02

′ 41

621

L640

.4S4

W1

23.8

20Se

e se

para

te

entry

For c

lass

(whi

ch re

fers

to c

lass

ifica

tion)

: Aub

= a

ubrit

e; U

re =

ure

ilite

.Sh

ock

stag

e (S

S): M

in =

min

imal

, Mod

= m

oder

ate;

Ext

= e

xten

sive

; IM

= im

pact

mel

t.W

eath

erin

g gr

ade

(WG

): M

in =

min

imal

, Mod

= m

oder

ate;

Ext

= e

xten

sive

.

Tabl

e 2.

A li

st o

f all

appr

oved

met

eorit

es fr

om n

orth

wes

t Afr

ica.

Nam

e

Dat

e of

re

cove

ry or

pu

rcha

seLo

catio

n of

reco

very

or

pur

chas

e

Tota

l kno

wn

mas

s (g

)N

o. o

f pi

eces

Cla

ss

Type

sp

ecim

en

mas

s (g

)SS

WG

Fa m

ol%

Fs m

ol%

Wo

mol

%M

agne

tic su

s (lo

g χ)

Info

rmat

ion

Com

men

ts

NW

A 8

0120

01Za

gora

, Mor

occo

5,00

0M

any

CR

277

.4Se

e se

para

te e

ntry

NW

A 1

461

Mar

-200

2Er

foud

, Mor

occo

252

1D

io23

+ 1

.3Se

e se

para

te e

ntry

NW

A 1

924

Jan-

2001

Efro

ud, M

oroc

co25

51

CV

320

.4Se

e se

para

te e

ntry

NW

A 2

044

Aug

-200

3Ef

roud

, Mor

occo

661

1C

V3

22.4

See

sepa

rate

ent

ryN

WA

276

420

05Ef

roud

, Mor

occo

134

1Eu

c20

.1N

AU

-7Fs

5 3.0

–57.

8Wo 2

.1–4

.5;

Fs48

.3W

o 14.

5N

WA

295

620

05Ef

roud

, Mor

occo

161

1Eu

c22

Mod

Min

NA

U-9

Fs37

–46.

3.3W

o 3.9

–5.6

; Fs

32.5

–36W

o 17.

7–39

.7; b

asal

ticN

WA

295

920

05Ef

roud

, Mor

occo

121

1Eu

c21

.1M

inM

inN

AU

-8Fs

55.2

Wo 2

.0; F

s 14.

3Wo 4

2.7

NW

A 3

157

2004

Den

ver,

Col

orad

o U

SA51

.71

OC

(typ

e 3)

10.6

See

sepa

rate

ent

ryN

WA

322

120

02R

issa

ni, M

oroc

co38

.51

Ure

7.7

See

sepa

rate

ent

ryN

WA

322

220

00M

oroc

co79

1U

re15

.8Se

e se

para

te e

ntry

NW

A 3

223

2002

Mor

occo

511

Ure

9.8

See

sepa

rate

ent

ryN

WA

334

0A

pr-2

006

Alg

eria

or M

oroc

co12

.72

CM

2-an

2.7

See

sepa

rate

ent

ryN

WA

422

3D

ec-2

005

Alg

eria

329

2D

io24

See

sepa

rate

ent

ryN

WA

422

6D

ec-2

005

Alg

eria

617

1H

720

.118

.5–1

9.2

16.3

3.5–

3.9

UW

S-4

δ18O

= 3

.03,

3.3

3; δ

17O

=

4.33

, 4.9

5; Δ

17O

= 0

.752

, 0.

726

(all

‰)

NW

A 4

229

Dec

-200

5Ta

goun

ite, M

oroc

co43

91

H7

20.3

18.4

–18.

716

.43.

1–4.

2U

WS-

4δ18

O =

2.9

5, 3

.11;

δ17

O =

4.

29, 4

.52;

Δ17

O =

0.6

93,

0.73

2 (a

ll ‰

)N

WA

423

0D

ec-2

005

Ris

sani

, Mor

occo

134

1M

eso

20.1

See

sepa

rate

ent

ryN

WA

423

2D

ec-2

005

Tago

unite

, Mor

occo

124

2EL

320

See

sepa

rate

ent

ryN

WA

425

5Se

p-20

02H

amad

a du

Dra

a60

00M

any

hund

reds

Dio

21Se

e se

para

te e

ntry

NW

A 4

269

Sep-

2004

Ham

ada

du D

raa

541

Euc

19.2

See

sepa

rate

ent

ryN

WA

427

1Fe

b-20

03H

amad

a du

Dra

a6

1Eu

c2.

55Se

e se

para

te e

ntry

NW

A 4

272

Dec

-200

3N

orth

wes

t Afr

ica

6,76

81

Dio

20Se

e se

para

te e

ntry

NW

A 4

292

Sep-

2005

Den

ver,

Col

orad

o, U

SA12

,000

1L6

21S2

W2

25.1

–25.

621

1.3

UW

S-5

NW

A 4

293

Sep-

2005

Den

ver,

Col

orad

o, U

SA25

,000

1H

620

.2S4

W2

18.6

–19.

216

.4–1

7.0

1.5

UW

S-5

NW

A 4

294

Feb-

2006

Tucs

on, A

rizon

a, U

SA84

1O

C (t

ype

3)22

See

sepa

rate

ent

ryN

WA

429

8Se

pt-2

005

Efro

ud, M

oroc

co18

1O

C (t

ype

3)4

See

sepa

rate

ent

ryN

WA

430

0M

ar-2

006

Erfo

ud, M

oroc

co45

,200

1H

541

.4S2

W3

19.5

17.1

1.5

UW

S-5

NW

A 4

302

Dec

-200

5Ta

goun

ite, M

oroc

co46

.22

Dio

9.3

See

sepa

rate

ent

ryN

WA

430

420

04B

aden

, Aus

tria

22.9

718

Ure

4.6

See

sepa

rate

ent

ryN

WA

431

220

04Za

gora

, Mor

occo

481

H6

10.6

S4W

117

.114

.5M

NB

-2N

WA

431

320

04Za

gora

, Mor

occo

118

1L6

20.8

S4W

323

.620

.6M

NB

-2C

onta

ins s

hock

vei

nsN

WA

431

920

04Za

gora

, Mor

occo

681

L615

.6S3

W3/

422

.719

.3M

NB

-2

Tabl

e 1.

Con

tinue

d. A

list

of m

eteo

rites

reco

vere

d fr

om s

peci

fic lo

catio

ns w

ithin

Afr

ica.

Nam

eLo

catio

n of

reco

very

Dat

e of

re

cove

ryFi

nd/

Fall

Latit

ude

(N)

Long

itude

(E

)

Tota

l kn

own

mas

s (g

)N

o. o

f pi

eces

Cla

ss

Type

sp

ecm

en

mas

s (g

)SS

WG

Fa (mol

%)

Fs (mol

%)

Wo

(mol

%)

Mag

netic

su

s(lo

g χ)

Info

Com

men

ts

1672 H. C. Connolly, Jr., et al.

NW

A 4

320

2004

Zago

ra, M

oroc

co16

01

H3

22.2

S2W

41.

4–13

.03.

0–9.

0M

NB

-2N

o sh

ock

vein

s and

no

ringw

oodi

te a

re o

bser

ved

NW

A 4

323

2004

Zago

ra, M

oroc

co70

2L4

14.8

S3W

121

.94.

2–21

.2M

NB

-2C

onta

ins s

hock

vei

nsN

WA

432

520

04Za

gora

, Mor

occo

180

1H

521

.4S2

W2

16.8

15.2

MN

B-2

NW

A 4

328

2004

Zago

ra, M

oroc

co28

1L

type

Imr

6.6

IMW

323

.419

.7M

NB

-2N

WA

432

920

04Za

gora

, Mor

occo

261

H3/

46

S2W

312

.5–1

7.9

3.6–

18.1

MN

B-2

NW

A 4

331

2004

Zago

ra, M

oroc

co21

1H

3/4

4.8

S2W

113

.3–1

6.1

2.6–

17.0

MN

B-2

NW

A 4

334

2004

Zago

ra, M

oroc

co83

1H

/L3

17.4

S3W

12.

0–30

.04.

3–17

.2M

NB

-2N

WA

433

720

02Za

gora

, Mor

occo

421

L59.

4S3

W2

26.4

22M

NB

-2N

WA

433

820

02Za

gora

, Mor

occo

531

H5

11.8

S2W

217

.415

.7M

NB

-2N

WA

433

920

02Za

gora

, Mor

occo

401

L38.

2S2

W2

0.4–

32.2

8.4–

26.9

MN

B-2

NW

A 4

343

2002

Zago

ra, M

oroc

co23

1H

35.

8S2

W0/

10.

4–17

.41.

0–17

.7M

NB

-2N

WA

435

120

02Za

gora

, Mor

occo

4500

12L

type

Imr

36.6

IMW

0/1

21.9

18.3

MN

B-2

NW

A 4

353

2003

Erfo

ud, M

oroc

co23

01

L5/6

21.9

S3W

223

.319

.8M

NB

-1N

WA

435

420

04Er

foud

, Mor

occo

1891

1L6

Imb

21.5

W2

23.9

20.2

MN

B-1

NW

A 4

357

2005

Erfo

ud, M

oroc

co26

4.7

1H

/L3

30S4

W1

3.7–

31.1

2–24

.3M

NB

-3N

WA

436

020

05Er

foud

, Mor

occo

308.

5m

any

R3.

623

.2Se

e se

para

te e

ntry

NW

A 4

362

2005

Erfo

ud, M

oroc

co60

.11

CK

5/6

14.4

See

sepa

rate

ent

ryN

WA

436

320

05Er

foud

, Mor

occo

244.

41

H4/

522

.4S2

W3

17.3

15.4

MN

B-3

NW

A 4

364

2005

Erfo

ud, M

oroc

co23

2.8

1L4

/524

.5S4

S223

.119

.3M

NB

-3N

WA

436

520

05Er

foud

, Mor

occo

474.

31

L4/5

25.4

S3W

422

.219

.1M

NB

-3N

WA

436

620

05Er

foud

, Mor

occo

274.

11

H6

28.4

S2W

3/4

17.6

15.6

MN

B-3

NW

A 4

367

2005

Erfo

ud, M

oroc

co51

.51

H4/

530

.5S2

W3

17.8

15.5

MN

B-3

NW

A 4

371

2005

Mun

ich,

Ger

man

y33

9.7

1H

4 Im

b20

.7S4

-IM

W2

17.8

15.1

–18.

6M

NB

-3N

WA

437

220

05M

unic

h, G

erm

any

64.8

1C

K4

13.5

See

sepa

rate

ent

ryN

WA

437

320

05M

unic

h, G

erm

any

56.8

1H

4/5

14.2

S2W

417

.715

.9M

NB

-3N

WA

437

420

05M

unic

h, G

erm

any

33.1

1H

58.

2S2

W3/

417

.816

.1M

NB

-3N

WA

437

520

05M

unic

h, G

erm

any

12.2

1W

in3.

9Se

e se

para

te e

ntry

NW

A 4

377

2005

Stut

tgar

t, G

erm

any

49.2

1L/

LL5

11.1

S3W

027

.122

.1M

NB

-3N

WA

437

820

05St

uttg

art,

Ger

man

y42

.11

LL5/

69.

4S4

W2

30.3

24.8

MN

B-3

Con

tain

s sho

ck v

eins

NW

A 4

379

2005

Erfo

ud, M

oroc

co49

4.4

1C

V3

20.6

S2W

2/3

0.1–

750.

9–1.

5M

NB

-3N

WA

438

020

06Er

foud

, Mor

occo

211.

2m

any

Dio

22.5

See

sepa

rate

ent

ryN

WA

438

920

05M

idel

t, M

oroc

co55

1U

re12

.1Lo

wM

od22

.819

.8M

NB

-4R

educ

ed ri

m:

Fa5.

1–16

.6N

WA

439

120

05M

idel

t, M

oroc

co54

.81

Euc

11.4

See

sepa

rate

ent

ryN

WA

439

220

05K

refe

ld, G

erm

any

490

1R

421

.7S2

W3

38.4

9–17

.5M

NB

-4N

WA

439

620

06Ta

goun

ite, M

oroc

co68

01

Euc

20Se

e se

para

te e

ntry

NW

A 4

397

2006

Tago

unite

, Mor

occo

341

Euc

6.8

See

sepa

rate

ent

ryN

WA

439

820

05Ta

goun

ite, M

oroc

co22

81

Euc

20.3

See

sepa

rate

ent

ryN

WA

439

920

05Ta

goun

ite, M

oroc

co21

0m

any

Acp

20.3

See

sepa

rate

ent

ryN

WA

442

420

06B

ir G

andu

z ar

ea,

Wes

tern

Sah

ara

756.

01

LL5

23.6

3S3

W4

25.4

6 ±

0.31

21.6

5 ±

0.33

4.19

MN

HN

P-3

~21°

36′N

, 16°

30′W

NW

A 4

426

2006

Erfo

ud, M

oroc

co/

Alg

eria

bor

der

757.

01

H5

37.5

6S2

W4

18.7

2 ±

0.43

17.5

8 ±

1.16

4.73

MN

HN

P-3

NW

A 4

427

2006

Erfo

ud, M

oroc

co/

Alg

eria

bor

der

158.

01

H5

38.5

2S2

W4

19.1

± 0

.35

16.9

1 ±

0.22

4.91

MN

HN

P-3

NW

A 4

470

Jul-2

006

Ris

sani

, Mor

occo

631

48Eu

c20

.1Se

e se

para

te e

ntry

NW

A 4

473

July

-200

6La

âyou

ne, M

oroc

co32

1D

io20

.1Se

e se

para

te e

ntry

NW

A 4

475

Aug

-200

5Ta

goun

ite, M

oroc

co9,

990

1L5

30S2

W1

24.1

20.9

1.2

UW

S-4

NW

A 4

478

Sep-

2006

Alg

eria

, Mor

occo

444

2Lo

d20

.1Se

e se

para

te e

ntry

NW

A 4

479

Apr

-200

4Ta

goun

ite, M

oroc

co55

22

H6

20.9

S2W

219

.1–1

9.6

16.4

1.3

UW

S-4

Tabl

e 2.

Con

tinue

d. A

list

of a

ll ap

prov

ed m

eteo

rites

from

nor

thw

est A

fric

a.

Nam

e

Dat

e of

re

cove

ry or

pu

rcha

seLo

catio

n of

reco

very

or

pur

chas

e

Tota

l kno

wn

mas

s (g

)N

o. o

f pi

eces

Cla

ss

Type

sp

ecim

en

mas

s (g

)SS

WG

Fa m

ol%

Fs m

ol%

Wo

mol

%M

agne

tic su

s (lo

g χ)

Info

rmat

ion

Com

men

ts

The Meteoritical Bulletin, No. 92 1673

NW

A 4

480

Sept

-200

6Ta

goun

ite, M

oroc

co13

1M

artia

nSe

e se

para

te e

ntry

NW

A 4

482

Aug

-200

6Ta

goun

ite, M

oroc

co5,

812

30Pa

l20

.1Se

e se

para

te e

ntry

NW

A 4

484

Jun-

2006

Ris

sani

, Mor

occo

140

7Eu

c20

See

sepa

rate

ent

ryN

WA

448

6Se

pt-2

004

Den

ver,

Col

orad

o, U

SA21

.31

OC

(typ

e 3)

4.6

See

sepa

rate

ent

ryN

WA

450

6 O

ct-2

006

Den

ver,

Col

orad

o, U

SA23

.21

Pal

8.17

See

sepa

rate

ent

ryN

WA

450

720

06Tu

cson

, Ariz

ona,

USA

851

Ure

17.2

2Se

e se

para

te e

ntry

NW

A 4

508

2001

Ris

sani

, Mor

occo

182

1U

re20

.2Se

e se

para

te e

ntry

NW

A 4

519

2001

Zago

ra, M

oroc

co11

41

Ure

20Se

e se

para

te e

ntry

NW

A 4

523

2001

Al N

if, M

oroc

co17

41

Euc

21Se

e se

para

te e

ntry

NW

A 4

524

Sep-

2006

Tago

unite

, Mor

occo

185.

51

L420

.1S2

W1

25.4

–25.

720

.8–2

1.1

1.1–

1.2

UW

S-4

NW

A 4

526

Sep-

2006

Tago

unite

, Mor

occo

52,8

5052

H4

33.8

S2W

2/3

19.1

–19.

716

.21.

2U

WS-

4N

WA

452

7Ju

ly-2

006

M’H

amid

, Mor

occo

10

2M

artia

n2.

1Se

e se

para

te e

ntry

NW

A 4

528

Sep-

2006

Tago

unite

, Mor

occo

239,

976

60H

527

.1S2

W2/

319

.1–1

9.8

15.7

1.5

UW

S-4

NW

A 4

531

Sept

-200

5D

enve

r, C

olor

ado,

USA

391

OC

(typ

e 3)

7.8

See

sepa

rate

ent

ryN

WA

453

2Se

p-20

05D

enve

r, C

olor

ado,

USA

68.7

1H

414

S1W

117

.4–1

7.7

14.9

0.8

UW

S-5

NW

A 4

533

Sep-

2005

Den

ver,

Col

orad

o, U

SA1,

245

1H

432

.8S2

W2

19.1

16.8

1.3

UW

S-5

NW

A 4

535

Sep-

2005

Den

ver,

Col

orad

o, U

SA1,

490

1H

522

.4S2

W3

19.5

171.

3U

WS-

5N

WA

454

620

06Er

foud

, Mor

occo

7200

man

yH

464

S2W

218

.516

.41.

7N

AU

-1O

lv o

f Pyx

? Fe

O/M

nO =

41

NW

A 4

547

2006

Erfo

ud, M

oroc

co36

00m

any

L425

S3-5

W2

23.7

21.4

1.8

NA

U-1

FeO

/MnO

= 5

3N

WA

454

820

06Er

foud

, Mor

occo

9132

man

yL4

28S2

W2

22.8

202.

1N

AU

-1Fe

O/M

nO =

47

NW

A 4

552

2006

Erfo

ud, M

oroc

co28

03

LL6

22S4

W2

32.6

25.8

1.8

NA

U-2

FeO

/MnO

= 6

2N

WA

455

420

06Er

foud

, Mor

occo

500

1L5

23S2

W2

25.2

21.1

2.9

NA

U-3

NW

A 4

555

2006

Erfo

ud, M

oroc

co13

131

H4

20.6

S2W

319

.117

2N

AU

-3N

WA

455

720

06Er

foud

, Mor

occo

250

1L4

18.7

S3-5

W1

2319

.82.

4N

AU

-3Sh

ock

dark

ened

NW

A 4

558

2006

Erfo

ud, M

oroc

co90

01

L425

.7S2

W2

24.5

21.6

1.8

NA

U-3

NW

A 4

559

2006

Erfo

ud, M

oroc

co90

04

LL5

20.5

S3-5

W2

31.8

252.

1N

AU

-3N

WA

456

219

98A

qalm

im, M

oroc

co44

01

L420

.7S2

W2

22.9

20.2

1.8

NA

U-3

NW

A 4

563

1998

Aqa

lmim

, Mor

occo

891

H4

17.8

S2W

219

17.1

1.6

NA

U-3

NW

A 4

564

2006

Erfo

ud, M

oroc

co50

01

LL5

23S2

W2

27.8

23.4

2N

AU

-3N

WA

456

520

05Er

foud

, Mor

occo

871

L418

S3-5

W1

24.1

20.6

1.5

NA

U-4

Shoc

k da

rken

edN

WA

456

720

05Er

foud

, Mor

occo

307

1H

422

.1S2

W1

17.7

15.6

2.4

NA

U-5

NW

A 4

570

2005

Erfo

ud, M

oroc

co24

31

L420

.1S3

-5W

123

.820

.51.

4N

AU

-4Sh

ock

dark

ened

NW

A 4

587

July

-200

6Er

foud

, Mor

occo

530

1A

ch-u

ng20

See

sepa

rate

ent

ryN

WA

458

820

05A

gadi

r15

301

L526

.1S5

W0

23.8

–24.

620

.0–

20.8

2.4–

2.5

UW

S-8

Oliv

ine

(FeO

/MnO

= 4

5–48

)N

WA

459

0Ju

ne-2

006

Tago

unite

, Mor

occo

213

man

yA

ng20

.01

See

sepa

rate

ent

ryN

WA

461

520

06M

oroc

co10

.51

R3.

42.

9Se

e se

para

te e

ntry

NW

A 4

619

2006

Mor

occo

704

1R

3-5

20.8

See

sepa

rate

ent

ryN

WA

462

420

06En

sish

eim

, Fra

nce

175

2Eu

c21

.5Se

e se

para

te e

ntry

NW

A 4

636

2005

Ger

man

y28

50>2

Mes

o29

See

sepa

rate

ent

ryN

WA

464

920

06Er

foud

, Mor

occo

3200

1LL

635

S3W

228

.824

AM

SA-1

NW

A 4

653

2006

Erfo

ud, M

oroc

co84

31

L522

S2W

123

.821

.62

NA

U-2

Poly

mic

t; th

ick

mel

t vei

ns<3

mm

NW

A 4

656

2006

Erfo

ud, M

oroc

co50

001

H4

34S2

218

.616

.12.

2N

AU

-6N

WA

467

7Ju

l-200

6Fr

ance

156.

41

Euc

20.2

See

sepa

rate

ent

ryN

WA

467

8A

ug-2

006

Ris

sani

, Mor

occo

3.6

1D

io3.

34Se

e se

para

te e

ntry

NW

A 4

680

Nov

-200

6Er

foud

, Mor

occo

3830

1L4

-6

23S3

W1

24.2

20.5

AM

SA-1

Bre

ccia

ted

NW

A 4

681

2006

Erfo

ud, M

oroc

co39

941

L538

S3W

424

.721

AM

SA-2

NW

A 4

682

2006

Erfo

ud, M

oroc

co29

201

L530

S4W

323

.320

AM

SA-2

NW

A 4

683

2006

Erfo

ud, M

oroc

co15

521

H4

22S3

W2

18.9

16.5

± 1

AM

SA-2

Tabl

e 2.

Con

tinue

d. A

list

of a

ll ap

prov

ed m

eteo

rites

from

nor

thw

est A

fric

a.

Nam

e

Dat

e of

re

cove

ry or

pu

rcha

seLo

catio

n of

reco

very

or

pur

chas

e

Tota

l kno

wn

mas

s (g

)N

o. o

f pi

eces

Cla

ss

Type

sp

ecim

en

mas

s (g

)SS

WG

Fa m

ol%

Fs m

ol%

Wo

mol

%M

agne

tic su

s (lo

g χ)

Info

rmat

ion

Com

men

ts

1674 H. C. Connolly, Jr., et al.

NW

A 4

684

2006

Erfo

ud, M

oroc

co36

501

H5

24S4

W4

18.9

16.5

± 1

AM

SA-1

NW

A 4

686

May

-200

6Er

foud

, Mor

occo

851

4H

422

S2W

2-3

17.7

15.5

± 1

AM

SA-3

Bre

ccia

ted

NW

A 4

687

May

-200

6Er

foud

, Mor

occo

703

1H

622

S3W

319

.717

± 1

AM

SA-3

NW

A 4

688

May

-200

6Er

foud

, Mor

occo

2184

481

H5

22S3

W3

18.9

16.5

± 1

AM

SA-3

481

piec

es ra

nge

from

1.7

g to

20

gN

WA

469

3N

ov-2

006

Erfo

ud, M

oroc

co86

61

R3–

624

.3Se

e se

para

te e

ntry

NW

A 4

695

2006

Mor

occo

20.2

0 1

H6

4.6

S3W

218

16.6

MN

B-1

NW

A 4

727

Mar

-200

6A

gadi

r, M

oroc

co60

5L6

57S5

W2

24.9

8 ±

0.24

21.7

1 ±

0.75

4.44

MN

HN

P-4

Mos

tly in

divi

dual

s, so

me

frag

men

ts; d

ark-

light

br

ecci

a; m

elt-f

illed

vei

nsN

WA

474

720

01Er

foud

, Mor

occo

1200

1M

eso

20.9

See

sepa

rate

ent

ryFo

r cla

ss (w

hich

refe

rs to

cla

ssifi

catio

n): A

cp =

aca

pulc

oite

; Ang

= a

ngrit

e; A

ung

= ac

hond

rite,

ung

roup

ed; B

ra =

bra

chin

ite; D

io =

dio

geni

te; E

uc =

euc

rite;

How

= h

owar

dite

; Im

b =

impa

ct-m

elt b

recc

ia; I

mr =

impa

ct-m

elt r

ock;

Mes

=m

esos

ider

ite.

Shoc

k st

age

(SS)

: Min

= m

inim

al, M

od =

mod

erat

e; E

xt =

ext

ensi

ve; I

M=

impa

ct m

elt.

Wea

ther

ing

grad

e (W

G):

Min

= m

inim

al, M

od =

mod

erat

e; E

xt =

ext

ensi

ve.

All

met

eorit

es a

re fi

nds a

nd p

urch

ased

unl

ess o

ther

wis

e st

ated

.

Tabl

e 2.

Con

tinue

d. A

list

of a

ll ap

prov

ed m

eteo

rites

from

nor

thw

est A

fric

a.

Nam

e

Dat

e of

re

cove

ry or

pu

rcha

seLo

catio

n of

reco

very

or

pur

chas

e

Tota

l kno

wn

mas

s (g

)N

o. o

f pi

eces

Cla

ss

Type

sp

ecim

en

mas

s (g

)SS

WG

Fa m

ol%

Fs m

ol%

Wo

mol

%M

agne

tic su

s (lo

g χ)

Info

rmat

ion

Com

men

ts

The Meteoritical Bulletin, No. 92 1675

Tabl

e 3.

A li

st o

f all

met

eorit

es a

ppro

ved

from

the

2003

to 2

005

AN

SMET

se

ason

s.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

Alla

n H

ills (

AL

H)

ALH

035

41H

5 10

53.5

BA

tA

LH 0

3542

L6

20.4

B/C

A/B

tC

ranf

ield

Pea

k (C

RA

)C

RA

035

40L3

15

1.9

BE

A/B

0–26

tG

rosv

enor

Mou

ntai

ns (G

RO

)G

RO

030

03L5

10

,640

CE

CG

RO

030

04L5

24

70B

/CE

B/C

tG

RO

030

05L5

25

76B

/CE

B/C

tG

RO

030

06L5

11

61.6

B/C

EB

/Ct

GR

O 0

3008

L5

1693

B/C

EB

/Ct

GR

O 0

3009

L5

1112

.9B

/CE

B/C

tG

RO

030

10L5

13

97.5

B/C

Bt

GR

O 0

3011

L5

1257

.6B

/CE

B/C

tG

RO

030

12L5

11

84A

/BE

B/C

tG

RO

030

18L5

15

54B

EB

tG

RO

030

26L5

56

1.2

B/C

Bt

GR

O 0

3030

L5

895.

3B

/CE

A/B

G

RO

030

34LL

5 27

4.6

A/B

At

GR

O 0

3040

H5

150.

4B

/CA

tG

RO

030

41L5

18

3.8

A/B

A/B

tG

RO

030

42L5

28

8.3

A/B

A/B

tG

RO

030

43L5

27

4.5

A/B

A/B

tG

RO

030

44L5

27

5.5

B/C

A/B

tG

RO

030

45L5

25

6.1

B/C

A/B

tG

RO

030

46L5

19

6.1

BA

tG

RO

030

47L5

28

2B

/CE

At

GR

O 0

3048

L5

394.

4B

/CA

/Bt

GR

O 0

3049

L5

311.

3B

/CA

/Bt

GR

O 0

3055

L4

384.

4B

/CA

2320

tG

RO

030

56H

5 42

2.5

BA

/Bt

GR

O 0

3057

L5

662.

9B

/CA

/Bt

GR

O 0

3058

L5

420.

7B

/CA

/Bt

GR

O 0

3059

L5

625.

3A

/BE

A/B

tG

RO

030

64LL

5 39

2.5

BA

/BG

RO

030

65L5

30

3.9

B/C

BG

RO

030

66L5

26

5.1

A/B

AG

RO

030

67L5

14

0.1

BA

GR

O 0

3068

L5

288.

2B

/CE

A/B

GR

O 0

3069

L5

219.

3B

/CE

A/B

GR

O 0

3075

LL5

294.

2A

/BA

tG

RO

030

76H

5 25

7.7

B/C

At

GR

O 0

3077

L5

201.

1B

/CE

A/B

tG

RO

030

78LL

5 23

9.8

A/B

At

GR

O 0

3079

LL5

165.

4A

/BA

t

GR

O 0

3110

L5

111.

5B

/CA

tG

RO

031

15LL

5 86

.1A

At

GR

O 0

3116

CR

2 10

8.3

B/C

A/B

1–37

1–8

tG

RO

031

17L5

87

.5B

/CA

/Bt

GR

O 0

3118

L5

64.1

B/C

A/B

tG

RO

031

19L5

75

.4B

/CA

/Bt

LaP

az Ic

efie

ld (L

AP)

LAP

0355

1L6

27

03.4

A/B

ALA

P 03

552

L6

3521

.5A

/BA

/BLA

P 03

554

H4

4201

.2B

A/B

LAP

0355

5L5

45

8.8

A/B

At

LAP

0355

6L5

18

23A

/BA

LAP

0355

7L5

15

05.1

A/B

ALA

P 03

558

L4

1521

.1B

ALA

P 03

559

L6

1839

.1A

/BA

LAP

0356

0L6

17

80A

/BA

/BLA

P 03

561

L5

1853

.2B

A/B

LAP

0356

2H

5 83

3.5

B/C

BLA

P 03

563

L6

868.

5A

/BA

LAP

0356

4H

4 85

3.8

BA

LAP

0356

5L5

11

98.7

BA

tLA

P 03

566

L6

1454

.4A

/BA

/BLA

P 03

567

L6

1009

.5A

/BA

/BLA

P 03

568

LL6

514.

9A

/BA

/BLA

P 03

570

LL4

801.

6B

At

LAP

0357

1L5

79

6.9

B/C

ALA

P 03

574

LL6

580.

7A

/BA

LAP

0357

5LL

5 64

3B

ALA

P 03

576

LL4

561

BA

LAP

0357

7LL

6 55

6.2

A/B

A/B

LAP

0357

8L5

47

1.6

A/B

A/B

tLA

P 03

579

LL4

411.

8B

/CA

/Bt

LAP

0358

0LL

6 58

2.9

A/B

A/B

tLA

P 03

581

LL4

541

BA

/Bt

LAP

0358

2LL

5 40

8.6

BB

tLA

P 03

584

LL5

311.

4B

Bt

LAP

0358

5L5

28

9A

/BA

/Bt

LAP

0358

6L5

34

3.9

A/B

At

LAP

0358

8L5

20

9.6

A/B

A/B

tLA

P 03

589

H4

232.

7B

At

LAP

0359

0LL

5 34

2.6

A/B

A/B

tLA

P 03

591

L6

235.

6B

BLA

P 03

592

LL5

192

CB

/CLA

P 03

594

L5

297

BB

LAP

0359

5LL

5 17

5.4

BC

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1676 H. C. Connolly, Jr., et al.

LAP

0359

6LL

5 39

7.1

BA

/BLA

P 03

597

LL4

245.

2B

BLA

P 03

598

L5

327.

2B

BLA

P 03

599

LL6

413.

2A

/BA

/BLA

P 03

600

LL5

353

AA

/B29

23LA

P 03

601

H4

331.

7A

/BA

tLA

P 03

602

L6

420.

8A

/BA

tLA

P 03

603

L5

305.

4B

/CA

tLA

P 03

604

L5

392.

3A

/BA

tLA

P 03

606

LL6

486.

1A

/BA

tLA

P 03

607

L5

359.

2A

/BA

tLA

P 03

608

H4

330.

7B

At

LAP

0360

9L5

45

1B

At

LAP

0361

0L5

44

7.2

A/B

At

LAP

0361

1LL

6 37

6.1

A/B

A/B

tLA

P 03

612

H6

206.

2B

/CA

/Bt

LAP

0361

3L5

22

9.8

A/B

At

LAP

0361

4LL

6 98

.4A

/BA

tLA

P 03

615

H4

120.

9B

/CA

tLA

P 03

616

H5

99.5

B/C

A/B

tLA

P 03

617

L5

173.

8A

/BB

tLA

P 03

618

L5

165

B/C

At

LAP

0361

9L4

16

4.3

A/B

A23

14–1

9t

LAP

0362

0L6

12

1.8

BB

tLA

P 03

621

L5

173.

5A

/BA

LAP

0362

2L5

12

7.1

AA

LAP

0362

3L5

14

7.8

A/B

A/B

LAP

0362

5L6

14

4.7

B/C

BLA

P 03

626

L4

145.

2B

/CA

/BLA

P 03

627

L6

155.

5B

/CA

LAP

0362

8L5

10

3.3

BA

/BLA

P 03

629

L6

56A

/BA

/BLA

P 03

633

L5

261.

5B

/CA

LAP

0363

4L5

10

3.3

AA

tLA

P 03

635

LL5

124.

3A

/BA

tLA

P 03

636

L5

190

A/B

At

LAP

0363

8L5

13

4.8

A/B

At

LAP

0363

9R

13

9.9

A/B

A19

–38

13–2

9t

LAP

0364

0H

4 16

8.7

BA

tLA

P 03

641

H6

212.

1B

/CA

tLA

P 03

642

H6

175.

8B

/CE

At

LAP

0364

3L5

23

0.2

B/C

At

LAP

0364

4LL

5 12

6.4

A/B

At

LAP

0364

6L5

20

7.8

A/B

At

LAP

0364

7LL

5 21

9.5

A/B

At

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

LAP

0364

8LL

5 21

4.7

A/B

At

LAP

0364

9L5

14

9.4

A/B

A/B

tLA

P 03

650

LL4

150.

7B

A/B

tLA

P 03

651

L5

162

A/B

ALA

P 03

652

L5

98.6

A/B

ALA

P 03

653

L5

75.6

A/B

A/B

LAP

0365

4LL

5 89

.3B

ALA

P 03

655

L5

49.6

B/C

ALA

P 03

656

LL6

74.6

A/B

ALA

P 03

657

L5

87B

/CA

LAP

0365

8LL

6 79

.7A

/BA

LAP

0365

9L6

95

.3A

/BA

/BLA

P 03

660

L5

96A

/BA

LAP

0366

1L5

10

3.1

A/B

A/B

tLA

P 03

662

LL5

68.1

A/B

A/B

tLA

P 03

663

L5

64.1

A/B

At

LAP

0366

4LL

6 61

.4A

A/B

tLA

P 03

665

L5

40.8

AB

/Ct

LAP

0366

6L5

86

.9A

/BA

/Bt

LAP

0366

7L5

42

.4A

/BA

tLA

P 03

668

LL5

42A

/BA

tLA

P 03

669

L4

96.1

A/B

At

LAP

0367

0H

6 85

.7C

EA

/Bt

LAP

0367

1L5

73

BB

tLA

P 03

672

H4

45.8

B/C

At

LAP

0367

3L4

76

.4B

/CA

tLA

P 03

674

L5

38.1

B/C

EA

tLA

P 03

675

L5

35.7

BB

tLA

P 03

676

LL5

52B

Bt

LAP

0367

8L5

58

B/C

A/B

tLA

P 03

679

L5

75.3

B/C

Bt

LAP

0368

0L6

55

.8A

/BA

tLA

P 03

681

L4

126.

2B

ALA

P 03

682

L5

123.

7A

/BA

LAP

0368

3L5

57

.7A

/BA

LAP

0368

4L4

61

.5B

ALA

P 03

685

H5

54.8

B/C

ALA

P 03

686

L5

42A

/BA

LAP

0368

7L5

54

.5A

/BA

LAP

0368

8H

5 86

.8B

/CA

/BLA

P 03

689

L5

95.4

BA

LAP

0369

0LL

5 69

.1A

/BA

LAP

0369

1L5

88

.3A

/BA

tLA

P 03

692

H5

78.4

B/C

EA

tLA

P 03

693

LL5

71A

/BA

t

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1677

LAP

0369

4L5

83

.1A

/BA

tLA

P 03

695

H6

44B

/CE

At

LAP

0369

6LL

6 39

A/B

At

LAP

0369

7LL

5 58

.7A

/BA

tLA

P 03

698

LL5

84.5

A/B

At

LAP

0369

9H

5 89

.5A

/BA

tLA

P 03

700

H4

85.8

BA

/Bt

LAP

0370

1L5

57

.7A

A/B

LAP

0370

2H

4 58

.3B

/CB

LAP

0370

3L5

97

.2A

/BA

/BLA

P 03

704

H6

61.4

CA

LAP

0370

5L5

59

.4A

ALA

P 03

706

L6

30.5

B/C

BLA

P 03

707

H5

84.6

AA

LAP

0370

8L6

39

.3A

ALA

P 03

709

LL6

41.3

B/C

BLA

P 03

710

H6

40.2

CB

LAP

0371

1H

6 63

.5C

Bt

LAP

0371

2L5

84

.9B

Bt

LAP

0371

3H

5 69

.1C

Bt

LAP

0371

4L4

80

.7A

/BA

/B23

13–1

8t

LAP

0371

5LL

5 53

A/B

A/B

tLA

P 03

716

LL6

25.7

BB

tLA

P 03

717

LL5

58.6

BB

tLA

P 03

720

LL5

51.4

B/C

Bt

LAP

0372

1U

re87

.5B

B/C

9–25

LAP

0372

2U

re29

.6B

B/C

4–25

LAP

0372

3L6

97

.5B

BLA

P 03

724

H5

60.5

CA

/BLA

P 03

725

LL6

45.7

BB

LAP

0372

6L6

57

.9B

/CA

/BLA

P 03

727

LL5

30B

BLA

P 03

728

L6

62.1

A/B

A/B

LAP

0372

9LL

5 58

B/C

BLA

P 03

730

L5

47B

BLA

P 03

731

R

56B

A36

29t

LAP

0373

2L5

89

.3B

Bt

LAP

0373

3L5

31

.2C

A/B

tLA

P 03

734

H6

19.2

BB

/Ct

LAP

0373

5L5

13

0.1

BB

tLA

P 03

736

LL6

68B

Bt

LAP

0373

7L5

23

.2B

Bt

LAP

0373

8L5

30

.2A

/BB

tLA

P 03

739

L5

63.3

BA

tLA

P 03

740

LL5

35.5

A/B

EA

/Bt

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

LAP

0374

1L5

70

.1A

/BA

tLA

P 03

742

L5

38.1

BA

tLA

P 03

743

L5

46.3

BA

tLA

P 03

744

L6

79.4

BA

tLA

P 03

745

H5

40.7

B/C

EA

tLA

P 03

746

L6

49A

/BA

tLA

P 03

747

H6

55.4

B/C

EA

/Bt

LAP

0374

8H

5 65

.9B

/CA

/Bt

LAP

0374

9L5

22

.5A

/BA

tLA

P 03

750

LL6

29.6

A/B

A/B

tLA

P 03

751

L5

49.5

A/B

A/B

tLA

P 03

752

H6

49.3

CB

tLA

P 03

753

H6

27.9

CC

tLA

P 03

754

LL6

36.7

A/B

A/B

tLA

P 03

755

LL5

28.4

A/B

A/B

tLA

P 03

756

L5

56.1

BA

/Bt

LAP

0375

7LL

6 25

BB

tLA

P 03

758

L4

28.1

AA

/Bt

LAP

0375

9H

4 48

.8C

At

LAP

0376

0H

6 8.

6C

Bt

LAP

0376

1L5

26

.1B

/CB

tLA

P 03

762

L5

34.5

BB

tLA

P 03

763

H6

50.7

CE

Bt

LAP

0376

4L5

33

.6B

Bt

LAP

0376

5H

4 73

.7B

A/B

tLA

P 03

766

L5

23B

Bt

LAP

0376

7L5

38

.8B

/CB

tLA

P 03

768

L5

84.3

BB

tLA

P 03

769

H4

61.1

B/C

Bt

LAP

0377

0L5

35

.4B

Bt

LAP

0377

1H

5 55

.3C

BLA

P 03

772

L5

102.

6B

BLA

P 03

773

L5

55.7

A/B

BLA

P 03

774

L5

58.2

BA

LAP

0377

5L6

23

A/B

A/B

LAP

0377

6L6

14

.6B

/CB

LAP

0377

7H

5 71

.9C

A/B

LAP

0377

8L5

91

.2B

A/B

LAP

0377

9L5

41

.5B

BLA

P 03

781

Dio

35B

A/B

222

LAP

0378

3L6

17

.3C

B/C

LAP

0378

6C

M2

22.4

A/B

A1–

406

LAP

0378

9L6

20

.8B

/CA

LAP

0379

0L5

37

.8A

/BA

/BLA

P 03

791

L5

16.6

BA

/Bt

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1678 H. C. Connolly, Jr., et al.

LAP

0379

2H

6 7.

4C

A/B

tLA

P 03

793

R

15B

EA

/B35

28t

LAP

0379

4H

4 8.

5C

A/B

tLA

P 03

795

H6

3.2

CC

tLA

P 03

796

Dio

16.5

BA

/B23

tLA

P 03

797

H6

4.6

CB

tLA

P 03

798

H6

4.5

CA

tLA

P 03

799

L5

6.9

BB

tLA

P 03

822

L-m

etal

1.7

CA

2420

tLA

P 03

824

L-m

etal

1.5

CA

2420

LA

P 03

900

L5

8.9

B/C

B

LAP

0390

1L5

8.

6B

/CB

tLA

P 03

902

R

6.2

A/B

A37

11–2

1t

LAP

0390

3L5

12

.7C

Bt

LAP

0390

4H

6 13

.8C

A/B

tLA

P 03

905

L5

15.4

BB

tLA

P 03

906

L4

11.9

BA

/Bt

LAP

0390

7L5

5.

8C

A/B

tLA

P 03

908

L5

6.4

CA

/Bt

LAP

0390

9H

6 6.

6C

Bt

LAP

0395

0H

5 7.

8B

/CA

tLA

P 03

991

H5

10.5

CC

1715

LAP

0310

00D

io27

.9B

A/B

222

LA

P 03

1037

FC0.

1A

/BA

/B

LAP

0310

43C

M2

8.1

A/B

A/B

1–48

LAP

0310

46H

5 14

.6C

C19

17

LAP

0310

47L-

IM16

.5A

A23

17

LAP

0310

62Eu

c-br

ecci

ated

12.3

A/B

A/B

17–4

1

LAP

0310

79C

M1

1.8

CC

LA

P 03

1109

Ure

14.5

B/C

A9–

25LA

P 03

1113

Euc-

brec

ciat

ed2.

2A

A21

–64

LA

P 03

1117

CO

3 4.

2B

A/B

1–36

1

LAP

0311

20L5

6.

2B

B

LAP

0311

21L5

11

.9B

Bt

LAP

0311

22L5

6.

1B

Bt

LAP

0311

23L5

19

.6B

Bt

LAP

0311

24L5

10

.4B

Bt

LAP

0311

25H

-IM

7B

A17

16t

LAP

0311

26LL

6 8.

5A

At

LAP

0311

27LL

6 33

.8A

/BA

tLA

P 03

1128

LL6

32.5

AA

tLA

P 03

1129

H6

13.5

CE

A/B

tLA

P 03

1140

LL6

5.5

B/C

Bt

LAP

0311

42L5

9.

9B

A/B

LAP

0311

44R

2.

5C

A/B

16–4

27–

19

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

LAP

0311

46H

5 4.

9B

/CA

/B

LAP

0311

47LL

6 5.

5B

ALA

P 03

1148

H6

3.6

CA

LAP

0311

49H

6 2.

3C

ALA

P 03

1160

L5

38.9

CA

/BLA

P 03

1161

L5

18.6

CB

tLA

P 03

1162

L4

25.1

BB

tLA

P 03

1163

L4

37.3

A/B

A/B

tLA

P 03

1164

L5

32.2

BB

tLA

P 03

1165

CM

2 27

BB

1–51

tLA

P 03

1166

CM

1-2

15.1

BB

0–1

tLA

P 03

1167

L5

10.7

CB

tLA

P 03

1168

L5

11.7

B/C

Bt

LAP

0311

69L4

7.

5C

Bt

LAP

0311

90Eu

c-br

ecci

ated

4.7

AA

25–5

7t

LAP

0311

91L5

5.

3B

/CE

Bt

LAP

0311

92L5

1.

6B

/CB

tLA

P 03

1193

L4

3.1

B/C

Bt

LAP

0311

94H

6 2.

4C

Bt

LAP

0311

95C

M2

0.6

BB

1–33

2–22

tLA

P 03

1196

L5

5.2

CB

tLA

P 03

1197

H6

0.5

BB

tLA

P 03

1198

L5

5.6

B/C

Bt

LAP

0311

99H

6 1.

4B

Bt

LAP

0312

00H

6 15

.4C

A/B

tLA

P 03

1201

H4

24.3

BA

/Bt

LAP

0312

02H

6 18

.1C

A/B

tLA

P 03

1203

L5

25.2

BA

tLA

P 03

1204

H6

23.2

CA

/Bt

LAP

0312

05L5

14

.4B

A/B

tLA

P 03

1206

H6

26.8

B/C

A/B

tLA

P 03

1207

L5

19.7

BA

/Bt

LAP

0312

08L4

26

BA

/Bt

LAP

0312

09L5

29

.5B

A/B

tLA

P 03

1220

EH4

3.1

CB

0–2

tLA

P 03

1221

LL6

7.2

AA

/B

LAP

0312

22H

6 5.

4C

ALA

P 03

1223

L3

4.8

B/C

B1–

273–

19LA

P 03

1224

LL6

7A

/BA

/B

LAP

0312

25LL

6 3.

3B

A/B

LAP

0312

26LL

6 2.

7B

A/B

LAP

0312

27L5

4.

5C

ALA

P 03

1228

L5

2.4

B/C

A/B

LAP

0312

29LL

5 5.

2B

A/B

LAP

0312

30H

5 12

.9C

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1679

LAP

0312

31LL

6 12

.8B

A/B

tLA

P 03

1232

L5

14C

Bt

LAP

0312

33L5

35

.2B

/CB

tLA

P 03

1234

L5

11.9

B/C

Bt

LAP

0312

35H

6 33

.6C

At

LAP

0312

36L5

13

CB

tLA

P 03

1237

H6

9.6

CB

/Ct

LAP

0312

38L5

9.

4B

Bt

LAP

0312

39L5

8.

7B

Bt

LAP

0312

50L6

1.

1B

A/B

tLA

P 03

1252

CM

1 0.

8B

EB

LAP

0312

53L5

1

BB

LAP

0312

54H

6 1.

3B

A/B

LAP

0312

57L5

1.

4B

BLA

P 03

1258

H5

2.1

CB

LAP

0312

59L5

1.

6C

BLA

P 03

1260

H5

11.8

CC

LAP

0312

61L5

6.

8B

A/B

tLA

P 03

1262

L5

11.1

B/C

Bt

LAP

0312

63L5

15

.6B

A/B

tLA

P 03

1264

L5

8.1

BA

/Bt

LAP

0312

65L6

8

A/B

A/B

tLA

P 03

1266

H5

4.4

CB

tLA

P 03

1267

L5

16.6

BB

tLA

P 03

1268

CM

2 15

.4B

B1–

381–

5t

LAP

0312

70H

6 3.

2C

A/B

tLA

P 03

1271

LL5

8C

BLA

P 03

1272

LL6

3C

BLA

P 03

1273

H6

3.6

BA

LAP

0312

74L6

5.

5C

ALA

P 03

1275

R

6.1

B/C

A17

–42

24LA

P 03

1276

L5

6.2

CA

LAP

0312

77LL

6 2.

2C

BLA

P 03

1278

L5

2.5

CB

LAP

0312

90LL

5 5.

3B

/CB

LAP

0312

91LL

5 13

.7B

Bt

LAP

0312

92LL

6 2.

1B

Bt

LAP

0312

93H

5 1.

1A

/Bt

LAP

0312

94H

5 4.

4C

A/B

tLA

P 03

1295

LL5

1.7

BB

tLA

P 03

1296

LL5

1.9

BB

tLA

P 03

1297

LL5

2.1

BB

tLA

P 03

1298

L6

5.5

CB

tLA

P 03

1299

CM

2 6.

9B

B1–

431–

38t

LAP

0313

00LL

5 9.

4B

/CB

t

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

LAP

0313

01L5

6.

6C

Bt

LAP

0313

02LL

5 23

B/C

B/C

tLA

P 03

1303

LL5

4B

/CB

tLA

P 03

1304

L5

1.3

BB

tLA

P 03

1305

LL5

6.5

B/C

Bt

LAP

0313

06LL

5 18

.8B

Bt

LAP

0313

07L4

45

.8B

A/B

tLA

P 03

1308

H

-IM

8.7

CC

1916

tLA

P 03

1309

Dio

14.1

BA

23t

LAP

0313

10H

4 11

.4C

B18

11–2

2t

LAP

0313

11L5

14

.7B

/CA

/Bt

LAP

0313

12LL

6 11

.4A

/BA

/Bt

LAP

0313

13H

5 18

.4C

Bt

LAP

0313

14L5

20

.4B

/CA

/Bt

LAP

0313

15L5

34

BA

/Bt

LAP

0313

16Eu

c-br

ecci

ated

25.8

BA

/B27

–84

tLA

P 03

1317

L5

16.1

BA

/Bt

LAP

0313

18L5

17

.3B

/CB

tLA

P 03

1319

H6

17.5

BA

/Bt

LAP

0313

21L-

met

al1.

3C

B24

20t

LAP

0313

30LL

5 10

.7B

A/B

tLA

P 03

1331

LL5

17.7

BA

/Bt

LAP

0313

32LL

5 12

.8C

B/C

tLA

P 03

1333

H6

8.5

CC

tLA

P 03

1334

L5

5.5

CB

tLA

P 03

1335

LL5

8.7

A/B

A/B

tLA

P 03

1336

L5

19.3

CB

tLA

P 03

1337

LL6

9.4

BA

/Bt

LAP

0313

38LL

6 22

.9B

B/C

tLA

P 03

1339

L4

75.5

B/C

Bt

LAP

0313

40H

6 2.

7C

Bt

LAP

0313

41H

6 1.

5C

Bt

LAP

0313

42U

re3.

2C

A/B

2–21

tLA

P 03

1343

L5

3.6

CA

/Bt

LAP

0313

44LL

5 6.

2B

Bt

LAP

0313

45H

5 7.

3C

A/B

tLA

P 03

1346

L3

5.4

B/C

B5–

404–

16t

LAP

0313

47L3

9

CB

0–33

2–5

tLA

P 03

1348

LL5

5.7

B/C

Bt

LAP

0313

49H

5 6.

1C

Bt

LAP

0313

50LL

6 2.

4A

/BA

tLA

P 03

1351

L6

2.6

BA

tLA

P 03

1352

L5

1.5

B/C

Bt

LAP

0313

53H

5 4.

7C

A/B

tLA

P 03

1354

L5

8.2

B/C

Bt

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1680 H. C. Connolly, Jr., et al.

LAP

0313

55L6

9.

2B

/CA

tLA

P 03

1356

L5

3.2

CC

tLA

P 03

1357

H6

2.9

CA

/Bt

LAP

0313

58H

5 4.

3C

A/B

tLA

P 03

1359

L6

2.5

B/C

Bt

LAP

0313

60H

5 10

.8C

A/B

tLA

P 03

1361

H6

12.3

CB

tLA

P 03

1362

H5

4.7

CB

tLA

P 03

1363

L4

9.1

BB

tLA

P 03

1364

L5

5.4

CB

tLA

P 03

1365

H5

11.8

CB

tLA

P 03

1366

H5

12.8

CB

tLA

P 03

1367

LL6

3.7

A/B

A/B

tLA

P 03

1368

H5

10.1

CB

tLA

P 03

1369

L6

3.2

B/C

Bt

LAP

0313

71C

M2

8.8

BB

1–36

1–30

tLA

P 03

1373

LL5

15.1

CB

/C

LAP

0313

74LL

5 6.

5C

BLA

P 03

1375

L5

4.5

BB

tLA

P 03

1376

H5

2C

B/C

tLA

P 03

1377

L5

2.2

CB

/Ct

LAP

0313

78L5

1.

5C

B/C

tLA

P 03

1379

Euc-

brec

ciat

ed4.

3A

/BA

/B25

–57

tLA

P 03

1380

L5

1.1

BA

/Bt

LAP

0313

82H

6 0.

4B

/CA

/Bt

LAP

0313

83LL

6 1.

4A

/BA

/Bt

LAP

0313

84LL

5 0.

2B

A/B

tLA

P 03

1385

H6

0.6

B/C

A/B

tLA

P 03

1386

H6

0.3

B/C

A/B

tLA

P 03

1387

R

1.1

BA

/B1–

381–

30t

LAP

0313

88H

6 0.

8B

/CA

/Bt

LAP

0313

89H

5 1

BA

/Bt

LAP

0313

91LL

6 1.

7A

/BA

tLA

P 03

1392

H5

3.3

B/C

ALA

P 03

1393

H6

1.1

BA

LAP

0313

94H

5 1.

7B

/CA

LAP

0313

95H

6 3

B/C

ALA

P 04

750

L5

5.9

B/C

A/B

LAP

0475

1H

-IM

2.8

B/C

A/B

1916

LAP

0475

2L5

1.

4B

BLA

P 04

753

L5

5.2

CA

LAP

0475

5L6

4.

3B

A/B

LAP

0475

6LL

5 6.

7C

A/B

LAP

0475

7A

cp12

.8C

B13

12–1

7LA

P 04

758

L6

7.5

CB

/C

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

LAP

0475

9H

4 6.

3C

B19

16LA

P 04

770

H5

1.1

BB

1916

LAP

0477

1C

M2

0.6

BB

1–50

2LA

P 04

772

L5

1.6

B/C

ALA

P 04

773

Acp

8.3

CA

/B13

13–1

6LA

P 04

774

L5

5.4

CA

LAP

0477

5L6

4.

1B

B24

21LA

P 04

776

L5

3.8

BB

LAP

0477

7L5

3.

4B

BLA

P 04

778

L5

7.9

CA

/BLA

P 04

779

Ure

1.8

CB

/C4–

22LA

P 04

830

LL5

4.3

BA

/B4–

22LA

P 04

831

L6

0.3

BA

LAP

0483

2H

6 0.

9C

BLA

P 04

833

L6

0.5

CC

LAP

0483

4H

5 0.

9B

BLA

P 04

835

L6

0.8

BB

LAP

0483

6D

io26

3.1

BA

23LA

P 04

837

Dio

542

BA

23LA

P 04

838

How

323.

5B

A/B

23–5

4LA

P 04

839

Dio

569.

4B

A23

LAP

0484

1Lu

nar-b

asal

t56

A/B

A/B

27–7

5LA

P 04

845

R

1.1

BA

/B13

–38

8–16

LAP

0484

6Eu

r (br

ecci

ated

)0.

5B

A/B

12–4

1L

arkm

an N

unat

ak (L

AR

)LA

R 0

4328

H5

15,8

50B

/CA

/BLA

R 0

4360

H6

15.2

CA

BLA

R 0

4361

H6

7.2

CA

/BLA

R 0

4363

H6

31.4

CB

LAR

043

65H

6 14

.6C

BLA

R 0

4366

H6

5.9

CA

/BLA

R 0

4367

H6

12.3

CB

LAR

043

68LL

6 4.

3A

ALA

R 0

4370

H6

15.5

CB

LAR

043

71H

6 17

.1C

BLA

R 0

4372

L5

9.2

CB

LAR

043

73H

6 16

.3C

BLA

R 0

4374

L4

20.2

CA

/BLA

R 0

4375

L6

17.3

B/C

A/B

LAR

043

76H

5 12

.5B

/CA

/BLA

R 0

4377

LL6

24B

A/B

LAR

043

78L6

36

.2C

BLA

R 0

4379

H6

9.2

CB

LAR

043

81H

6 14

.7C

ALA

R 0

4383

L5

2.4

CB

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1681

LAR

043

84L4

10

.1B

/CB

LAR

043

85H

6 43

.9C

B/C

LAR

043

86H

6 24

.1C

BLA

R 0

4387

H6

6.2

CA

/BLA

R 0

4388

H6

25.6

CA

LAR

043

89LL

6 9.

6B

BM

acA

lpin

e H

ills (

MA

C)

MA

C 0

4990

L5

0.2

BB

MA

C 0

4991

L5

0.6

BB

MA

C 0

4992

L5

0.6

BB

MA

C 0

4994

L5

0.5

BB

MA

C 0

4995

L5

0.4

BB

MA

C 0

4101

0L5

0.

9B

BM

AC

041

011

L5

0.4

BB

MA

C 0

4101

2L5

0.

8B

BM

AC

041

013

L5

0.4

BB

MA

C 0

4101

4L5

0.

6B

BM

AC

041

015

L5

0.4

BB

MA

C 0

4101

6L5

0.

7B

BM

AC

041

017

L5

1.1

BB

MA

C 0

4101

8L5

1.

2B

BM

AC

041

019

L5

0.8

BB

MA

C 0

4107

0L5

0.

7B

BM

AC

041

071

L5

1B

BM

AC

041

072

L5

1.2

BB

MA

C 0

4107

3L5

0.

6B

BM

AC

041

074

L5

0.3

BB

MA

C 0

4112

0L5

0.

9B

BM

AC

041

121

L5

0.9

BB

MA

C 0

4112

2L5

0.

5B

BM

AC

041

123

L5

0.8

BB

MA

C 0

4112

4H

5 0.

5B

BM

AC

041

125

L5

0.5

BB

MA

C 0

4112

6L5

0.

6B

BM

AC

041

127

H4

0.5

BB

195–

21M

AC

041

128

H5

0.5

BB

MA

C 0

4112

9L5

0.

7B

BM

AC

041

130

LL5

0.3

BB

MA

C 0

4113

1L5

0.

6B

BM

AC

041

132

L5

0.2

BB

MA

C 0

4113

3L5

0.

4B

BM

AC

041

134

L5

0.7

BB

MA

C 0

4113

5L5

0.

4B

BM

AC

041

136

L5

1.2

BB

MA

C 0

4113

7H

5 0.

6B

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

MA

C 0

4113

8H

5 0.

9B

BM

AC

041

139

L5

0.6

BB

MA

C 0

4114

0L5

0.

3B

BM

AC

041

141

L5

0.5

BB

MA

C 0

4114

2L5

0.

6B

BM

AC

041

143

L5

0.7

BB

MA

C 0

4114

4H

4 0.

9B

BM

AC

041

145

L5

0.9

BB

MA

C 0

4114

6L5

0.

7B

BM

AC

041

147

L5

0.7

BB

MA

C 0

4114

8L5

0.

8B

BM

AC

041

149

L5

0.4

BB

MA

C 0

4115

0L4

1.

3B

BM

AC

041

151

L5

0.5

BB

MA

C 0

4115

2H

5 0.

3B

BM

AC

041

153

L5

0.5

BB

MA

C 0

4115

4L5

0.

2B

BM

AC

041

155

L5

0.3

BB

MA

C 0

4115

6H

5 0.

4B

BM

AC

041

157

H5

0.9

BB

MA

C 0

4115

8L5

0.

5B

BM

AC

041

159

L5

0.3

BB

MA

C 0

4118

0L5

0.

6B

BM

AC

041

181

L5

1.1

BB

MA

C 0

4118

2L5

0.

9B

BM

AC

041

183

L5

1.1

BB

MA

C 0

4118

4L4

1.

6B

BM

AC

041

185

L5

0.8

BB

MA

C 0

4118

6H

5 0.

2B

BM

AC

041

187

L6

0.5

BB

MA

C 0

4118

8L5

0.

9B

BM

AC

041

189

L5

0.7

BB

MA

C 0

4119

0L4

1.

2B

BM

AC

041

191

L5

0.4

BB

MA

C 0

4119

2L5

0.

4B

BM

AC

041

193

Acp

/Lod

1.3

BA

/B11

11M

AC

041

194

H5

0.5

BB

MA

C 0

4119

5LL

5 0.

9B

BM

AC

041

196

L5

0.5

BB

MA

C 0

4119

7L6

1.

4B

BM

AC

041

198

L5

0.8

BB

MA

C 0

4119

9L5

1

BB

MA

C 0

4120

0L5

0.

5B

BM

AC

041

201

L4

0.8

BB

MA

C 0

4120

2L5

0.

5B

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1682 H. C. Connolly, Jr., et al.

MA

C 0

4120

3L5

0.

2B

BM

AC

041

204

H5

1B

BM

AC

041

205

L5

1.3

BB

MA

C 0

4120

6L5

0.

9B

BM

AC

041

207

L5

0.8

BB

MA

C 0

4120

8L5

0.

5B

BM

AC

041

209

L5

0.4

BB

MA

C 0

4121

0L5

0.

5B

BM

AC

041

211

L5

0.4

BB

MA

C 0

4121

2L5

1

BB

MA

C 0

4121

3L5

0.

4B

BM

AC

041

214

L5

0.2

BB

MA

C 0

4121

5H

5 1

BB

MA

C 0

4121

6LL

6 0.

7B

BM

AC

041

217

L5

1.8

BB

MA

C 0

4121

8L5

0.

9B

BM

AC

041

219

CM

2 0.

5B

B1–

38M

AC

041

220

L5

0.8

BB

MA

C 0

4122

1L5

0.

5B

BM

AC

041

222

L5

0.9

BB

MA

C 0

4122

3L5

0.

9B

BM

AC

041

224

L5

0.8

BB

MA

C 0

4122

5L5

0.

4B

BM

AC

041

226

L5

1.1

BB

MA

C 0

4122

7L5

0.

5B

BM

AC

041

228

L5

1.5

BB

MA

C 0

4122

9L5

1.

3B

BM

AC

041

230

L5

1.2

BB

MA

C 0

4123

1L5

1.

5B

BM

AC

041

232

L5

1B

BM

AC

041

233

L5

1.1

BB

MA

C 0

4123

4L5

1.

1B

BM

AC

041

235

L5

1.8

BB

MA

C 0

4123

6L3

1.

5B

BM

AC

041

237

L5

1.5

BB

MA

C 0

4123

8L5

1.

6B

BM

AC

041

239

L5

1.5

BB

Mac

Kay

Gla

cier

(MC

Y)

MC

Y 0

5200

LL5

3532

.3A

/BA

MC

Y 0

5201

L5

1917

.7A

/BE

A/B

MC

Y 0

5202

L5

1178

.1A

/BE

AM

CY

052

03LL

6 10

78.4

A/B

EA

/BM

CY

052

04LL

6 89

4.3

AB

MC

Y 0

5205

L6

350.

9B

A/B

MC

Y 0

5206

LL6

247.

2B

A/B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

MC

Y 0

5207

L6

210.

9B

/CA

/BM

CY

052

08L6

16

7.2

B/C

B/C

MC

Y 0

5209

LL6

104.

7A

/BA

/BM

CY

052

10LL

5 42

6.4

A/B

AM

CY

052

11LL

5 34

4.8

A/B

AM

CY

052

12L5

31

9.7

B/C

AM

CY

052

13LL

5 35

2.3

A/B

AM

CY

052

14L4

30

6.1

B/C

A/B

MC

Y 0

5215

LL5

254.

3B

AM

CY

052

16L5

14

5.5

A/B

A/B

MC

Y 0

5217

L5

198.

7B

/CA

MC

Y 0

5218

H3

214.

5B

/CA

/B1–

212–

9M

CY

052

19C

V3

145

BA

/B0–

4M

CY

052

20L5

96

.6B

A/B

MC

Y 0

5221

L5

81C

BM

CY

052

22LL

5 81

.3A

/BA

MC

Y 0

5223

H5

69C

AM

CY

052

24LL

5 40

.5B

AM

CY

052

25LL

6 67

.6A

AM

CY

052

26L5

65

.5C

A/B

MC

Y 0

5227

LL6

6.3

A/B

BM

CY

052

28L6

29

.9C

B/C

MC

Y 0

5229

CM

2 9.

7B

B1–

28M

CY

052

30C

M2

60.1

BA

1–32

MC

Y 0

5231

CM

1-2

6.2

BA

/B0–

331–

40M

CY

052

32C

K4

2.1

BB

33M

CY

052

33L5

8.

7C

A/B

MC

Y 0

5234

CM

1-2

0.8

BA

/B0–

2M

CY

052

35L6

1.

3B

/CB

MC

Y 0

5236

L6

2.1

CA

/BM

CY

052

37L5

9.

7B

A/B

MC

Y 0

5238

L5

1.4

CA

/BM

CY

052

39M

es19

.3C

B34

–39

27–3

6M

CY

052

40LL

5 1.

2B

/CA

/BM

CY

052

41L5

2.

5B

/CA

/BM

CY

052

42C

M2

2B

B1–

256

MC

Y 0

5243

L6

11.1

B/C

BM

CY

052

44LL

5 3.

1B

A/B

MC

Y 0

5245

CM

2 1.

3B

B0–

403

MC

Y 0

5246

L6

1.2

B/C

BM

CY

052

47LL

5 9.

2B

A/B

MC

Y 0

5248

L5

0.8

B/C

BM

CY

052

49LL

5 4.

7B

BM

CY

052

50L6

34

.9B

/CB

MC

Y 0

5251

CM

2 25

.3B

B1–

381

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1683

MC

Y 0

5252

LL6

41.5

A/B

A/B

MC

Y 0

5253

H6

18.2

B/C

BM

CY

052

54LL

6 8.

8A

/BA

/BM

CY

052

55L5

1

B/C

BM

CY

052

56H

6 1.

3B

/CB

MC

Y 0

5257

L6

0.5

B/C

BM

CY

052

58L6

0.

6B

/CB

MC

Y 0

5259

L6

0.8

B/C

BM

CY

052

60L5

4.

2B

/CB

MC

Y 0

5261

LL5

0.2

BA

/BM

CY

052

62LL

6 0.

8B

A/B

MC

Y 0

5263

LL6

0.9

BA

/BM

CY

052

64L6

0.

8B

/CB

Mill

er R

ange

(MIL

)M

IL 0

3331

H6

1550

CC

MIL

033

32L5

23

95A

/BA

MIL

033

33L5

19

22A

/BB

/CM

IL 0

3334

H6

4025

.9B

/CE

AM

IL 0

3335

L5

2283

.3B

/CE

A/B

MIL

033

36L5

96

9.8

BE

A/B

tM

IL 0

3337

LL5

1564

.7A

/BE

At

MIL

033

38L5

15

97.3

A/B

EA

/Bt

MIL

033

39LL

5 90

3.7

A/B

A/B

tM

IL 0

3340

LL5

911.

5A

/BB

/Ct

MIL

033

41LL

5 71

7.2

A/B

A/B

tM

IL 0

3342

H5

658

BA

/Bt

MIL

033

43H

5 76

5B

/CB

/Ct

MIL

033

44H

5 53

6.5

B/C

B/C

tM

IL 0

3345

L6

603.

1B

/CB

/CE

tM

IL 0

3347

LL6

548.

2A

/BB

/Ct

MIL

033

48LL

6 39

5B

A/B

tM

IL 0

3349

H5

274.

6B

/CA

tM

IL 0

3350

LL5

309.

3A

/BA

/Bt

MIL

033

51LL

6 36

8.6

B/C

Bt

MIL

033

52H

5 25

8.7

CB

/Ct

MIL

033

53L5

26

2.9

B/C

At

MIL

033

54L5

15

9.8

B/C

At

MIL

033

55L6

20

2.6

BA

tM

IL 0

3357

H5

501.

2C

Bt

MIL

033

58H

5 32

3.2

CB

tM

IL 0

3359

L5

502.

7B

BE

tM

IL 0

3365

L5

1114

.8A

/BA

/Bt

MIL

033

66L5

81

5.9

B/C

A/B

tM

IL 0

3367

H6

372.

9B

/CB

/Ct

MIL

033

70H

5 16

9.8

CB

t

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

MIL

033

71L4

82

.7B

A24

19t

MIL

033

72LL

5 97

.8B

/CA

/Bt

MIL

033

73L5

10

3.9

BA

tM

IL 0

3374

L5

71.3

B/C

EA

tM

IL 0

3375

L5

125.

9C

A/B

tM

IL 0

3376

H6

212.

5C

Bt

MIL

033

77C

O3

129.

8B

A/B

1–42

tM

IL 0

3378

L5

145.

1C

Bt

MIL

033

79H

5 20

7.5

CA

/Bt

MIL

033

80L5

85

.7B

A/B

tM

IL 0

3381

H5

46B

/CA

tM

IL 0

3382

LL5

58.4

B/C

At

MIL

033

83L5

19

1A

/BA

tM

IL 0

3384

LL5

122.

5B

A/B

tM

IL 0

3385

LL6

99.3

A/B

At

MIL

033

86L5

12

7B

/CA

/Bt

MIL

033

87L5

68

.3B

At

MIL

033

88L5

15

4.3

BA

tM

IL 0

3389

LL5

146

BA

tM

IL 0

3390

H5

83.9

B/C

At

MIL

033

91L5

68

.9B

At

MIL

033

92LL

5 94

.5B

At

MIL

033

93H

5 64

.7B

/CA

tM

IL 0

3394

H6

22.3

B/C

Bt

MIL

033

95H

5 20

B/C

EA

/Bt

MIL

033

96H

5 29

.1B

/CA

tM

IL 0

3397

H5

3.9

B/C

At

MIL

033

98H

5 16

.6B

/CA

/Bt

MIL

033

99LL

5 18

.6A

/BA

tM

IL 0

3420

LL5

45.1

A/B

At

MIL

034

21H

5 2.

4B

/CA

tM

IL 0

3422

L5

29.4

BA

tM

IL 0

3423

LL5

45.4

A/B

At

MIL

034

24LL

5 4.

4A

/BA

tM

IL 0

3425

H5

18.2

B/C

A/B

tM

IL 0

3426

L5

35.2

B/C

A/B

tM

IL 0

3427

H5

54.7

B/C

A/B

tM

IL 0

3428

L5

23.5

B/C

A/B

tM

IL 0

3429

H5

27.3

B/C

EA

tM

IL 0

3430

H5

4.4

CA

/Bt

MIL

034

31H

6 5.

8C

EA

/Bt

MIL

034

33H

6 16

.5C

At

MIL

034

34L5

6.

5B

/CB

tM

IL 0

3435

H5

4.6

CA

/Bt

MIL

034

36H

6 14

.2C

A/B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1684 H. C. Connolly, Jr., et al.

MIL

034

37H

6 6.

8C

A/B

MIL

034

38H

5 37

CB

MIL

034

39H

3 1.

4B

A2–

200–

15M

IL 0

3440

H6

31.7

CA

/BM

IL 0

3441

L5

34.3

B/C

BM

IL 0

3442

CO

3 63

.8C

A/B

0–38

2M

IL 0

3443

Mes

46.3

BB

26M

IL 0

5001

L5

3055

.5B

EB

M

IL 0

5002

H5

21,4

90C

EC

tM

IL 0

5003

LL5

2181

.8A

/BA

/Bt

MIL

050

04L6

83

1.1

B/C

B/C

tM

IL 0

5005

L5

1127

.8B

EA

tM

IL 0

5006

L5

1234

.8B

EA

MIL

050

07L5

30

4.4

B/C

BM

IL 0

5008

H5

330.

9B

/CE

A/B

MIL

050

09L6

39

6.8

A/B

AM

IL 0

5010

H4

582.

4B

/CA

/B19

16M

IL 0

5011

L5

1608

.3A

/BA

/BM

IL 0

5012

L5

2409

.6A

/BA

MIL

050

13C

O3

1494

.6B

/CE

A/B

1–47

1–6

MIL

050

14L5

88

1.6

A/B

AM

IL 0

5015

L5

1025

.8B

BM

IL 0

5016

L5

1336

.2C

A/B

MIL

050

17H

5 98

7.2

B/C

B/C

EM

IL 0

5019

L5

394.

4B

/CA

/BM

IL 0

5020

L5

368.

7B

/CB

/CM

IL 0

5021

LL5

300.

5A

/BA

MIL

050

22L5

23

5.7

B/C

EA

/BM

IL 0

5023

LL4

133.

1A

/BA

/BM

IL 0

5024

CO

3 19

6.6

A/B

A0–

55M

IL 0

5025

L5

104.

3A

/BA

MIL

050

26L5

72

.5B

/CB

MIL

050

27LL

6 67

.5A

/BE

AM

IL 0

5028

LL5

77.9

A/B

A/B

MIL

050

29L

-IM

132.

7A

/BE

A/B

2521

MIL

050

30LL

5 11

2.9

BA

/BM

IL 0

5032

H6

127.

8B

/CA

/BM

IL 0

5033

H5

179.

2C

A/B

MIL

050

34L6

19

2.4

CB

MIL

050

35Lu

nar-b

asal

tM

IL 0

5036

L6

314.

1C

BM

IL 0

5037

H5

239

CA

/BM

IL 0

5038

L6

187.

4C

CM

IL 0

5039

L5

227.

6A

/BA

/BM

IL 0

5040

L5

305.

4B

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

MIL

050

41Eu

r (br

ecci

ated

)23

9.8

BB

/C60

MIL

050

42LL

5 26

2.6

A/B

A/B

MIL

050

43L6

30

8C

CM

IL 0

5044

L5

180.

2C

CM

IL 0

5045

L5

283.

4B

/CE

A/B

MIL

050

46L5

38

8.3

BA

/BM

IL 0

5047

LL5

289.

7A

/BE

AM

IL 0

5048

L5

197.

2B

/CB

MIL

050

49L5

15

2B

/CB

MIL

050

50L3

25

3.3

BA

/B6–

253–

17M

IL 0

5051

L5

368

CA

/BM

IL 0

5052

L5

257.

6C

BM

IL 0

5053

LL6

399

BB

/CM

IL 0

5054

H5

233.

6B

/CA

MIL

050

55LL

5 10

9.2

A/B

AM

IL 0

5056

LL5

113.

6B

AM

IL 0

5057

LL6

472.

2A

/BA

/BM

IL 0

5058

L6

128.

1A

/BB

/CM

IL 0

5059

L5

118.

5B

/CA

MIL

050

60LL

6 34

.7A

/BA

MIL

050

61L5

58

.8B

/CA

/BM

IL 0

5062

How

23.8

BA

29–5

4M

IL 0

5063

L5

23.3

B/C

A/B

MIL

050

64L5

82

.5A

/BA

/BM

IL 0

5065

H5

23.3

B/C

AM

IL 0

5066

H5

21.1

A/B

AM

IL 0

5067

LL5

42A

/BA

/BM

IL 0

5068

H5

36.1

A/B

A/B

MIL

050

70L6

61

.9C

BM

IL 0

5071

L6

28.4

CB

MIL

050

72L5

28

.1C

A/B

MIL

050

73LL

5 10

6.7

BA

/BM

IL 0

5074

H5

88.4

CA

/BM

IL 0

5075

L5

86.8

CB

MIL

050

76L3

59

.5B

A/B

MIL

050

77L5

32

.5C

BM

IL 0

5078

LL6

41.2

A/B

A/B

MIL

050

79L5

82

.7A

/BB

MIL

050

80LL

6 30

.2A

/BA

/BM

IL 0

5081

H6

41.2

CC

MIL

050

82C

B

12B

B1–

31–

3M

IL 0

5083

L6

35.7

B/C

BM

IL 0

5084

L6

30.9

B/C

BM

IL 0

5085

How

18.6

BB

27–6

0M

IL 0

5086

CM

2 1.

7B

EA

/B0–

250–

4

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1685

MIL

050

87LL

6 13

.1B

BM

IL 0

5088

L5

16.8

BB

MIL

050

89L6

17

.3A

/BB

MIL

050

90L6

23

.5A

/BB

MIL

050

91L5

14

.8C

A/B

MIL

050

92L5

31

.5C

A/B

MIL

050

93LL

6 6.

9A

AM

IL 0

5094

LL5

9.4

B/C

BM

IL 0

5095

LL5

28.3

BB

MIL

050

96LL

5 13

.9A

/BB

MIL

050

97LL

6 24

.6B

BM

IL 0

5098

H4

9.9

CB

MIL

050

99L5

49

.9B

A/B

MIL

051

00L6

17

.3C

CM

IL 0

5101

L5

22.2

CC

MIL

051

02L5

12

.8B

/CB

MIL

051

03L5

5.

6C

BM

IL 0

5104

CO

3 41

BA

1–28

1M

IL 0

5105

L5

33.3

A/B

AM

IL 0

5106

LL5

12A

/BA

MIL

051

07LL

6 18

.7A

/BE

AM

IL 0

5108

L6

19.5

CA

/BM

IL 0

5109

LL5

5B

/CB

MIL

051

11L5

0.

9B

/CB

MIL

051

12C

M2

2.8

1–20

MIL

051

13LL

5 0.

3B

/CB

MIL

051

14H

6 7.

8C

A/B

MIL

051

15L5

5.

9B

/CB

MIL

051

16L5

2.

2C

A/B

MIL

051

17L5

1.

3B

/CB

MIL

051

18H

4 1.

4C

EB

2017

MIL

051

19C

M2

0.9

BB

0–32

MIL

051

20L6

2.

7C

A/B

MIL

051

21LL

6 2

B/C

BM

IL 0

5122

L6

0.8

CA

/BM

IL 0

5123

L6

5.2

CA

/BM

IL 0

5124

CM

2 2.

6B

B1–

2032

MIL

051

25L5

0.

8C

A/B

MIL

051

27LL

6 3.

5B

/CB

MIL

051

28L6

1.

9C

BM

IL 0

5129

LL6

2.8

A/B

AM

IL 0

5130

L6

12.5

A/B

AM

IL 0

5131

L6

4.7

B/C

BM

IL 0

5132

L6

17.4

CB

MIL

051

33LL

5 4.

6A

A/B

2824

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

MIL

051

34L6

3.

6C

A/B

MIL

051

35L6

4.

9C

BM

IL 0

5136

L-IM

8.3

B/C

B25

21M

IL 0

5137

CM

1 2.

4B

EB

MIL

051

38LL

6 7.

5A

A/B

MIL

051

39EH

3 10

.6C

C2

0–3

MIL

051

40H

6 13

.4C

CM

IL 0

5141

L5

1.6

CC

MIL

051

42L5

11

.4C

BM

IL 0

5143

L6

4.2

CB

MIL

051

45LL

6 2.

1A

A/B

MIL

051

46L5

2.

3C

BM

IL 0

5148

L6

0.9

CB

MIL

051

49L5

2.

6B

BM

IL 0

5150

L5

42.3

CB

MIL

051

51LL

6 10

1.5

AA

/BM

IL 0

5152

CM

2 46

.6B

A/B

1–37

1–26

MIL

051

53L5

51

.2B

/CB

MIL

051

54L5

72

B/C

A/B

MIL

051

55L-

IM53

.5B

B25

21M

IL 0

5156

LL6

94.4

BB

MIL

051

57L6

95

.2A

/BB

MIL

051

58L6

73

.7C

BM

IL 0

5159

LL5

89B

BM

IL 0

5160

L5

38.4

CA

MIL

051

61H

6 24

.6C

BM

IL 0

5162

L5

33.7

CB

MIL

051

63H

6 42

.9C

BM

IL 0

5164

L6

38.8

B/C

BM

IL 0

5165

How

25.6

BB

30–6

0M

IL 0

5166

H6

39.7

CA

MIL

051

67L6

29

CA

MIL

051

68L6

75

.7B

BM

IL 0

5169

L5

48.1

B/C

BM

IL 0

5171

H6

4.3

CB

/CM

ount

Pra

tt (P

RA

)PR

A 0

4401

How

55C

EB

1–60

PRA

044

02H

ow37

.8B

B16

–60

PRA

044

03LL

6 65

5.7

BA

PRA

044

04LL

6 35

8.9

BA

PRA

044

05LL

6 13

73.5

AA

PRA

044

06H

6 11

88.6

CA

/BPR

A 0

4407

L5

508

BA

/BPR

A 0

4408

LL6

384.

7A

/BA

PRA

044

09LL

6 32

6.8

A/B

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1686 H. C. Connolly, Jr., et al.

PRA

044

10LL

5 27

8.6

BA

PRA

044

11LL

5 17

0.6

B/C

A/B

PRA

044

12L6

82

.8C

BPR

A 0

4413

L5

84.6

BA

PRA

044

15LL

6 10

6.8

BA

/BPR

A 0

4416

LL5

69.8

B/C

BPR

A 0

4417

LL5

87.5

BB

PRA

044

18L5

36

.7B

/CB

PRA

044

19LL

6 62

.9B

APR

A 0

4420

L6

21.6

CB

PRA

044

21L5

25

.7C

BPR

A 0

4422

LL6

5060

AA

Rob

erts

Mas

sif (

RB

T)

RB

T 03

520

LL6

1327

.7A

/BA

/BR

BT

0352

1LL

5 13

78A

AR

BT

0352

4H

6 18

2.6

CA

RB

T 03

525

L5

299.

7A

/BA

/BR

BT

0352

6H

5 26

9C

AR

BT

0352

7L5

14

2.3

BB

tR

BT

0352

8LL

6 78

.3B

A/B

tR

BT

0352

9H

5 12

8.5

CB

RB

T 04

100

L6

2609

CB

RB

T 04

101

L5

1918

.6C

B/C

RB

T 04

102

L5

1328

.4B

/CA

/BR

BT

0410

3H

5 18

4.9

CA

/BR

BT

0410

4LL

5 20

4.8

A/B

A/B

2924

RB

T 04

105

L5

298.

2C

BR

BT

0410

6L4

29

2.4

CC

RB

T 04

107

LL5

522.

9B

A/B

RB

T 04

108

L6

386.

1B

/CB

RB

T 04

109

LL6

198.

9B

BR

BT

0411

0LL

6 17

2.1

B/C

CR

BT

0411

1H

6 27

3.6

CA

/BR

BT

0411

2LL

5 20

4.3

BA

/BR

BT

0411

3L6

38

3.2

CC

RB

T 04

114

L3

281.

6B

/CA

/B1–

293–

18R

BT

0411

5LL

5 14

56.3

BA

/BR

BT

0411

6LL

6 11

42.9

A/B

A/B

RB

T 04

117

H5

965.

3C

A/B

RB

T 04

118

LL5

985.

5A

/BB

RB

T 04

119

H5

945.

5C

CR

BT

0412

0L5

76

6.4

CA

RB

T 04

121

L5

495.

4B

AR

BT

0412

2H

5 30

2.1

B/C

CR

BT

0412

3H

6 36

7.7

CA

/B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

RB

T 04

124

H6

297.

4C

BR

BT

0412

5LL

5 37

5.4

A/B

BR

BT

0412

6L5

13

48.2

CB

RB

T 04

128

L5

1104

.8B

/CA

/BE

RB

T 04

129

LL5

1140

BB

RB

T 04

134

L5

277.

3C

BR

BT

0413

5L6

24

5.5

CB

RB

T 04

136

LL5

217.

4B

A/B

RB

T 04

137

H4

235.

2C

BR

BT

0413

8L5

21

9.7

CB

RB

T 04

139

L5

141.

4C

BR

BT

0414

0L6

35

.3C

B/C

RB

T 04

141

H5

126

CB

RB

T 04

142

H6

101.

4C

B/C

RB

T 04

144

H6

192.

7C

A/B

RB

T 04

145

H6

47.3

CB

RB

T 04

146

H6

130.

7C

BR

BT

0414

7L6

12

6.6

CA

/BR

BT

0414

8H

6 12

4.1

CA

/BR

BT

0414

9H

6 94

.7C

EC

RB

T 04

150

H5

27.5

CB

RB

T 04

151

H6

120

CB

RB

T 04

152

H6

151.

9C

BR

BT

0415

3L5

86

.1B

/CB

RB

T 04

154

H5

103.

8C

BR

BT

0415

5H

6 10

3.6

CB

RB

T 04

156

H6

100.

2C

BR

BT

0415

7H

5 62

.6C

BR

BT

0415

8LL

6 86

.4B

/CB

RB

T 04

159

H6

61.9

CB

RB

T 04

160

H6

60C

A/B

RB

T 04

161

H5

57.1

CA

/BR

BT

0416

2Ir

on-u

ng52

.3R

BT

0416

3H

5 35

.6C

BR

BT

0416

4H

6 11

.9C

CR

BT

0416

5H

6 14

.4C

BR

BT

0416

6LL

6 11

.1C

A/B

RB

T 04

167

H5

23.5

CB

RB

T 04

168

H6

11.3

CA

/BR

BT

0416

9H

6 9.

1C

A/B

RB

T 04

170

LL5

71.3

BA

/BR

BT

0417

1H

5 17

0.3

CA

/BR

BT

0417

2H

5 14

1.6

B/C

A/B

RB

T 04

173

L5

99.6

B/C

A/B

RB

T 04

174

L5

110.

5C

A/B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1687

RB

T 04

175

L5

61.2

B/C

A/B

RB

T 04

176

L5

22.1

B/C

A/B

RB

T 04

177

L6

42.6

BB

RB

T 04

178

H6

27.4

CA

/BR

BT

0417

9L5

19

.8C

A/B

RB

T 04

180

H6

19.7

CB

RB

T 04

181

LL5

3.1

BB

RB

T 04

182

H6

20C

BR

BT

0418

3H

6 12

CB

RB

T 04

184

H5

11.5

CB

RB

T 04

185

LL5

7.7

BA

/BR

BT

0418

6Ir

on-I

IE (?

)4.

618

–20

16–1

9R

BT

0418

7L5

5.

1C

A/B

RB

T 04

188

LL6

10.3

BB

RB

T 04

189

H5

11.6

CB

RB

T 04

190

L6

191.

5B

BR

BT

0419

1L5

69

CA

/BR

BT

0419

2L5

28

.5C

B/C

RB

T 04

193

L5

85C

A/B

RB

T 04

194

L5

123.

9B

A/B

RB

T 04

195

L5

162

CA

/BR

BT

0419

6L5

93

.3A

/BA

RB

T 04

197

L5

39.9

CB

RB

T 04

198

L5

77.9

BA

/BR

BT

0419

9L5

38

.3C

BR

BT

0420

0H

6 31

.3C

A/B

RB

T 04

201

L5

12.2

CB

RB

T 04

202

H5

14.8

CC

RB

T 04

203

LL6

17.8

BC

RB

T 04

204

H6

13.3

CB

RB

T 04

205

H5

12.4

CB

RB

T 04

206

L5

12.8

CA

/BR

BT

0420

7H

5 38

.2C

A/B

RB

T 04

208

H6

1.1

CB

/CR

BT

0420

9LL

6 2.

2C

A/B

RB

T 04

210

H4

133.

5A

/BA

/B18

16R

BT

0421

1H

5 18

2.7

CA

/BR

BT

0421

2H

6 13

6.1

CC

RB

T 04

213

L5

127.

9B

AR

BT

0421

4H

5 73

.9C

CR

BT

0421

5H

5 11

1.8

CC

RB

T 04

216

L5

86.5

CB

/CR

BT

0421

7L5

18

7.3

CB

/CR

BT

0421

8L5

11

8.9

CA

/BR

BT

0421

9L5

69

.2C

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

RB

T 04

220

H5

66.8

CB

RB

T 04

221

H5

57.3

CB

RB

T 04

222

L5

64B

A/B

RB

T 04

223

L5

28.4

BB

RB

T 04

224

LL5

44.8

CB

RB

T 04

225

H6

34.1

CA

/BR

BT

0422

6H

5 29

CB

RB

T 04

227

L6

57.3

BA

/BR

BT

0422

8A

cp19

.8C

C8

10R

BT

0422

9H

5 75

.1C

BR

BT

0423

0L5

68

.9C

A/B

RB

T 04

231

LL6

11.1

BA

/BR

BT

0423

2H

5 9.

3C

A/B

RB

T 04

233

L5

20.3

CB

RB

T 04

234

H6

16.3

CB

RB

T 04

235

H6

8.5

CC

RB

T 04

236

LL5

13.8

AA

RB

T 04

237

L5

40.9

CB

RB

T 04

238

L5

10.1

CC

RB

T 04

239

Ach

on-u

ng12

CA

/B24

20R

BT

0424

1L6

86

.7B

/CA

RB

T 04

242

L5

54.6

B/C

B/C

RB

T 04

243

H5

41.4

B/C

A/B

RB

T 04

244

LL6

73.5

A/B

AR

BT

0424

5L5

34

B/C

B/C

RB

T 04

246

LL5

28.1

A/B

AR

BT

0424

7H

5 44

.2R

BT

0424

8L5

35

.6B

/CA

/BR

BT

0424

9L5

25

.2B

/CB

/CR

BT

0425

0L5

7.

9C

BR

BT

0425

2L5

32

.7B

A/B

RB

T 04

253

L5

47C

BR

BT

0425

4L5

54

.9C

BR

BT

0425

6L5

34

.7C

BR

BT

0425

7L5

34

.1C

BR

BT

0425

8L5

7.

6C

BR

BT

0425

9LL

6 4.

5B

/CB

RB

T 04

260

CM

2 86

.3C

EC

0–1

1R

BT

0426

1M

artia

n78

.8B

B39

20–2

7R

BT

0426

2M

artia

n20

4.6

BB

38–4

016

–32

RB

T 04

270

L6

370.

6C

A/B

RB

T 04

271

L5

341.

8B

/CB

/CR

BT

0427

2L5

40

0.5

B/C

BR

BT

0427

3H

5 25

7.1

CB

RB

T 04

274

L5

431.

1C

B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

1688 H. C. Connolly, Jr., et al.

RB

T 04

275

L5

712.

2B

/CB

RB

T 04

276

H6

189.

7C

BR

BT

0427

7H

5 32

6.9

B/C

BR

BT

0427

9H

5 19

5B

/CB

RB

T 04

280

L5

225.

7C

BR

BT

0428

1H

5 13

8.4

CB

RB

T 04

282

L5

144.

9C

BR

BT

0428

3LL

5 11

9.6

BB

/CR

BT

0428

4LL

5 10

2.8

B/C

BR

BT

0428

5L6

83

.2C

BR

BT

0428

6H

6 67

.8C

BR

BT

0428

7H

5 37

.8C

BR

BT

0428

8H

5 45

CB

RB

T 04

289

H5

43.1

CB

RB

T 04

290

H5

25.6

BB

RB

T 04

291

L5

54.2

CB

RB

T 04

292

L5

32.3

CB

RB

T 04

293

L5

72.2

CA

/BR

BT

0429

4L5

59

.3C

BR

BT

0429

5L5

70

.3C

A/B

RB

T 04

296

L5

52.9

B/C

A/B

RB

T 04

297

L5

77.5

CB

RB

T 04

298

LL5

44B

EB

RB

T 04

299

Iron

-ung

55.2

RB

T 04

300

L5

3.1

CB

RB

T 04

301

L5

9.1

CB

RB

T 04

302

CV

3 11

.6B

B1–

91

RB

T 04

303

L5

16.6

CB

RB

T 04

304

L5

8.5

CB

RB

T 04

305

L5

14.7

CB

/CR

BT

0430

6L6

11

.8C

BR

BT

0430

7L5

8.

1A

/BA

RB

T 04

308

L5

7.1

B/C

BR

BT

0430

9C

M2

1.3

BE

B1–

50Sa

nfor

d C

liffs

(SA

N)

SAN

034

50L5

51

68B

A/B

SAN

034

54L5

13

46.8

BA

SAN

034

57L5

78

6.9

BB

SAN

034

64L5

91

9.1

BE

A/B

SAN

034

65L5

59

6.5

BA

/BSA

N 0

3466

L5

553.

4B

EA

/BSA

N 0

3467

L5

462.

9B

A/B

SAN

034

70L5

22

4.1

B/C

EA

/BSA

N 0

3471

L5

237.

4B

EA

/B

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

SAN

034

72H

ow19

5.2

BA

/B20

–52

SAN

034

73D

io12

5.4

B/C

A22

2SA

N 0

3474

L5

224.

5B

EA

/BSA

N 0

3475

L5

179.

8B

/CA

SAN

034

76L5

14

5.6

BE

A/B

SAN

034

77L5

10

8B

/CA

/BSA

N 0

3478

LL5

107.

2B

EA

/BSA

N 0

3479

LL5

58.7

B/C

A/B

Tayl

or G

laci

er (T

YR

)TY

R 0

5180

L5

244.

2B

/CA

/Ba F

or cl

ass (

whi

ch re

fers

to cl

assi

ficat

ion)

: Acp

= ac

apul

coite

; Ang

= an

grite

; Ach

on-u

ng =

acho

ndrit

e,un

grou

ped;

Bra

= b

rach

inite

; D

io =

dio

geni

te; E

uc =

euc

rite;

FC

= fu

sion

cru

st c

hond

rite;

How

=ho

war

dite

; Ir

on-u

ng =

iro

n un

grou

ped;

IM

-Im

= i

mpa

ct m

elt;

Imr

= im

pact

-mel

t ro

ck;

Mes

=m

esos

ider

ite; P

al =

pal

lasi

te; P

rA =

prim

itive

ach

ondr

ite; U

re =

ure

ilite

. Oth

er a

bbre

viat

ions

can

be

foun

d on

the

JSC

Cur

atio

n W

eb p

age.

b WG

= w

eath

erin

g gr

ade.

t = th

awed

.

Tabl

e 3.

Con

tinue

d. A

list

of a

ll m

eteo

rites

app

rove

d fr

om th

e 20

03 to

200

5 A

NSM

ET s

easo

ns.

Nam

eC

lass

aM

ass

(g)

WG

bFr

actu

ring

Fa (mol

%)

Fs

(mol

%)

Info

The Meteoritical Bulletin, No. 92 1689

Tabl

e 4.

A li

st o

f met

eorit

es re

cove

red

by P

rogr

amm

a N

azio

nale

Ric

erch

e in

Ant

artid

e (P

NR

A),

the

Italia

n go

vern

men

t-spo

nsor

ed e

xped

ition

.

Nam

eTy

pe o

f fin

d si

teD

ate

of

reco

very

La

titud

e (S

)Lo

ngitu

de

(E)

Tota

l kn

own

mas

s (g

)N

o. of

pi

eces

Cla

ssSS

WG

Fa

(mol

%)

Fs

(mol

%)

Mag

netic

su

s (lo

g χ)

Type

sp

ecim

en

mas

s (g

)In

foC

omm

ents

Alla

n H

ills 0

6001

Blu

e ic

e15

-Oct

-200

676

°43.

017′

158°

46.1

17′

128.

11

H5

S3W

1-2

18.3

17.5

5.09

128.

1M

NA

-SI

Alla

n H

ills 0

6002

Blu

e ic

e15

-Oct

-200

676

°44.

552′

15

8°50

.583

′11

9.2

1H

~55.

0411

9.2

MN

A-S

ILi

kely

pai

red

with

ALH

060

01A

llan

Hill

s 060

03B

lue

ice

15-O

ct-2

006

76°4

2.67

7′

158°

47.5

70′

251

H~5

5.07

25M

NA

-SI

Like

ly p

aire

d w

ith A

LH 0

6001

Alla

n H

ills 0

6004

Blu

e ic

e15

-Oct

-200

676

°42.

313′

15

8°46

.703

′61

.71

H~5

5.07

61.7

MN

A-S

ILi

kely

pai

red

with

ALH

060

01A

llan

Hill

s 060

05B

lue

ice

15-O

ct-2

006

76°4

2.31

3′

158°

46.7

03′

61

H~5

5.05

6M

NA

-SI

Like

ly p

aire

d w

ith A

LH 0

6001

Alla

n H

ills 0

6006

Blu

e ic

e15

-Oct

-200

676

°42.

335′

15

8°46

.552

′28

0.9

4H

~55.

0828

0.9

MN

A-S

ILi

kely

pai

red

with

ALH

060

01A

llan

Hill

s 060

07B

lue

ice

15-O

ct-2

006

76°4

2.33

1′

158°

46.5

50′

226.

31

H5

S3W

1-2

18.7

16.9

5.20

226.

3M

NA

-SI

Like

ly p

aire

d w

ith A

LH 0

6001

Alla

n H

ills 0

6008

Blu

e ic

e15

-Oct

-200

676

°42.

331′

158°

46.4

91′

120

2H

~55.

0612

0M

NA

-SI

Like

ly p

aire

d w

ith A

LH 0

6001

Alla

n H

ills 0

6009

Blu

e ic

e15

-Oct

-200

676

°42.

729′

15

8°46

.516

′28

.61

H~5

5.08

28.6

MN

A-S

ILi

kely

pai

red

with

ALH

060

01A

llan

Hill

s 060

10B

lue

ice

15-O

ct-2

006

76°4

2.75

8′

158°

46.7

17′

1.08

1H

~55.

071.

08M

NA

-SI

Like

ly p

aire

d w

ith A

LH 0

6001

Alla

n H

ills 0

6011

Blu

e ic

e15

-Oct

-200

676

°42.

753′

15

8°46

.716

′ 24

.31

H~5

5.10

24.3

MN

A-S

ILi

kely

pai

red

with

ALH

060

01A

llan

Hill

s 060

12B

lue

ice

15-O

ct-2

006

76°4

3.04

0′

158°

46.4

39′

912

H5

S3W

1-2

18.7

17.8

5.07

91M

NA

-SI

Like

ly p

aire

d w

ith A

LH 0

6001

Tabl

e 5.

A li

st o

f met

eorit

es re

cove

red

by th

e C

hine

se A

ntar

ctic

Exp

editi

on.

Nam

eD

ate

of

reco

very

La

titud

e(N

)Lo

ngitu

de(E

)

Tota

l kn

own

mas

s(g

)N

o. o

f pi

eces

Cla

ssSS

WG

Fa

(mol

%)

Fs (mol

%)

Mag

netic

sus

(log

χ)

Type

sp

ecim

en

mas

s(g

)C

omm

ents

Gro

ve M

ount

ain

GRV

052

049

16-J

an-2

006

72°4

6′23

′′75

°20′

8′′

96.7

1L5

S6W

1Fa

24.0

± 0

.4Fs

20.6

± 0

.54.

6PR

ICSe

e se

para

te e

ntry

GRV

055

364

9-Ja

n-20

0672

°59′

36′′

75°1

3′6′

′39

6.4

1M

esPR

ICSe

e se

para

te e

ntry

For c

lass

(whi

ch re

fers

to c

lass

ifica

tion)

: Mes

= m

esos

ider

ite.

1690 H. C. Connolly, Jr., et al.

Tabl

e 6.

A li

st o

f all

appr

oved

met

eorit

es fr

om A

sia.

Nam

eLo

catio

n of

re

cove

ry

Dat

e of

re

cove

ry

or p

urch

ase

Find

/fa

llLa

titud

e(N

)Lo

ngitu

de

(E)

Tota

l kn

own

mas

s (g

)

No.

of

pi

eces

Cla

ss

Type

sp

ecim

en

mas

s (g

)SS

WG

Fa

mol

%Fs

m

ol%

Wo

mol

%

Mag

netic

su

s(lo

g χ)

Com

men

ts

Uni

ted

Ara

b E

mir

ates

Ara

bian

Pen

insu

la 0

01U

nite

d A

rab

Emira

tes

2006

Find

145

1D

io21

See

sepa

rate

ent

ry

Ara

bian

Pen

insu

la 0

02U

nite

d A

rab

Emira

tes

2006

Find

541

Euc

10.8

See

sepa

rate

ent

ry

Ara

bian

Pen

insu

la 0

03U

nite

d A

rab

Emira

tes

2006

Find

561

Dio

11.2

See

sepa

rate

ent

ry

Ara

bian

Pen

insu

la 0

04U

nite

d A

rab

Emira

tes

2006

Find

311

Dio

7Se

e se

para

te e

ntry

Ara

bian

Pen

insu

la 0

05U

nite

d A

rab

Emira

tes

2005

Find

146

1Eu

c21

See

sepa

rate

ent

ry

Ara

bian

Pen

insu

la 0

06U

nite

d A

rab

Emira

tes

2005

Find

671

Euc

13.5

See

sepa

rate

ent

ry

Chi

naW

eike

ngqu

anJi

uqua

n C

ity,

Gan

su

Prov

ince

2006

Find

40°1

6′99

°49′

665

1H

535

96

319

.4 ±

0.4

17.1

± 0

.24.

45Se

e se

para

te e

ntry

Om

anD

hofa

r 142

7D

hofa

r re

gion

17 Ja

nuar

y 20

01Fi

nd19

°6.7

71′

54°4

9.12

6′12

.92

1U

re2.

6Se

e se

para

te e

ntry

Sayh

al U

haym

ir 29

0Sa

yh a

l U

haym

ir re

gion

2004

Find

21°0

4′31

.6′′

54°4

9.12

6′17

,960

64C

H3

20.1

See

sepa

rate

ent

ry

For c

lass

(whi

ch re

fers

to c

lass

ifica

tion)

: Dio

= d

ioge

nite

; Euc

= e

ucrit

e.SS

= sh

ock

stag

e.W

G =

wea

ther

ing

grad

e.

Tabl

e 7.

A li

st o

f app

rove

d re

lict m

eteo

rites

from

Sw

eden

.

Nam

eA

bbre

viat

ion

Dat

e of

re

cove

ryLo

ngitu

de(N

)La

titud

e(E

)A

ppro

xim

ate

size

s(c

ross

sect

ions

in m

m)

Info

Com

men

ts

Öst

erpl

ana

Öst

001

1987

58°3

5′13

°26′

45 ×

30

Lund

U-1

Wea

ther

ed m

eteo

rite

cont

aine

d in

red

limes

tone

pla

te (9

8 ×

80 ×

50

mm

). Li

ght g

ray

redu

ctio

n ha

lo (t

otal

cro

ss se

ctio

n in

clud

ing

met

eorit

e: 1

35 ×

135

mm

) aro

und

dark

gra

y de

pres

sion

from

whi

ch

mos

t of t

he m

eteo

rite

has w

eath

ered

out

. Thi

s sto

ne h

as a

syno

nym

of

Öst

erpl

ana

001.

Öst

erpl

ana

002

Öst

002

10-O

ct-1

993

58°3

5′13

°26′

55

× 5

5 ×

> 13

Lund

U-1

Dar

k m

eteo

rite i

n re

d lim

esto

ne p

late

(165

× 1

30 ×

12

mm

). Th

in, l

ight

gr

ay re

duct

ion

halo

(75

× 75

mm

).Ö

ster

plan

a 00

st 0

038-

Nov

-199

358

°35′

13°2

6′45

× >

25 ×

>15

Lund

U-1

Dar

k m

eteo

rite

in re

d pe

ntag

onal

lim

esto

ne p

late

(abo

ut 1

00 ×

80

× 10

×

110

× 18

× (h

eigh

t) 17

mm

). Pl

ate

cut d

iago

nally

thro

ugh

cent

er o

f m

eteo

rite.

Cen

tral p

art o

f met

eorit

e bl

uish

-gre

enis

h, su

rrou

nded

by

rust

y re

d cm

-thic

k zo

ne. L

ight

redu

ctio

n ha

lo e

xten

ds ~

1 cm

out

from

m

eteo

rite.

Öst

erpl

ana

004

Öst

004

6-Ja

n-19

9458

°35′

13°2

6′50

× 5

2Lu

ndU

-1D

ark

met

eorit

e in

red

limes

tone

pla

te (1

27 ×

175

× 3

1 m

m).

Ligh

t re-

duct

ion

halo

(52

× 54

mm

). Tw

o pr

omin

ent w

orm

bur

row

s in

plat

e. O

ne

wor

m tr

ack

follo

ws c

lose

ly o

uter

rim

of r

educ

tion

halo

. In

the

plat

e th

ere

is a

lso

a pe

rfec

tly ro

und

whi

te c

ircle

of c

alci

te fr

om a

ver

tical

ly

posi

tione

d na

utilo

id sh

ell.

The Meteoritical Bulletin, No. 92 1691

Öst

erpl

ana

005

Öst

005

8-Fe

b-19

9058

°35′

13°2

6′ab

out 1

0 ×

10Lu

ndU

-2Sm

all s

omew

hat s

quar

e-sh

aped

met

eorit

e w

ith in

tens

e re

duct

ion

halo

ster

plan

a 00

st 0

06Id

entif

ied

5-M

ay-1

992;

re

cove

red

in

the

1960

s

58°3

5′13

°26′

50 ×

50

Lund

U-2

Stro

ngly

wea

ther

ed, s

quar

e-sh

aped

met

eorit

e with

shar

p ed

ges.

Mos

t of

met

eorit

e m

ass i

s los

t and

mai

nly

the

depr

essi

on o

f the

met

eorit

e re

mai

ns (~

Öpl

001

). Th

e m

eteo

rite

is in

fron

t of a

gar

age

entra

nce

and

has b

een

driv

en o

ver b

y ca

rs th

ousa

nds o

f tim

es.

Öst

erpl

ana

007

Öst

007

28-D

ec-1

993

58°3

5′13

°26′

95 ×

80;

95

× 80

Lund

U-1

Larg

e dar

k, v

ery

roun

d m

eteo

rite i

n tw

o la

rge p

late

s (ea

ch 4

80 ×

480

×

30 m

m).

Surr

ound

ed b

y in

ner l

ight

ora

nge

redu

ctio

n ha

lo (2

10 ×

200

m

m) a

nd a

n an

othe

r out

er d

arke

r red

hal

o. M

eteo

rite

with

hal

os lo

oks

like

an e

ye, w

here

the

met

eorit

e is

the

pupi

l.Ö

ster

plan

a 00

st 0

085-

May

-199

558

°35′

13°2

6′40

× 1

8; 2

8 ×

15Lu

ndU

-1D

ark

met

eorit

e w

ith e

llipt

ical

shap

e in

two

red

limes

tone

pla

tes s

awed

pe

rpen

dicu

larly

to th

e sea

floo

r. Pl

ate s

izes

are 1

60 ×

100

× 2

7 m

m an

d 16

0 ×

100

× 20

mm

ster

plan

a 00

st 0

0915

-Jan

-199

658

°35′

13°2

6′40

× 2

5 ×

8Lu

ndU

-1D

ark

met

eorit

e in

red

limes

tone

pla

te (9

7 ×

116

× 54

mm

). M

eteo

rite a

t ed

ge o

f pla

te an

d sa

wed

thro

ugh

both

per

pend

icul

arly

and

horiz

onta

lly

rela

tive

to th

e se

a flo

or.

Öst

erpl

ana

010

Öst

010

1995

58°3

5′13

°26′

35 ×

20

Lund

U-1

Dar

k m

eteo

rite

in v

ery

smal

l and

thin

red

limes

tone

pla

te (6

7 ×

80 ×

6

mm

). M

eteo

rite

has e

xtra

ordi

naril

y w

ell p

rese

rved

cho

ndru

le

stru

ctur

es. C

hond

rule

s are

on

aver

age

0.5

to 0

.6 m

m in

dia

met

er. S

ize

of re

duct

ion

halo

50

× 70

mm

ster

plan

a 01

st 0

1131

-Jan

-100

758

°35′

13°2

6′37

× 4

4; 3

2 ×

57Lu

ndU

-1Ve

ry d

ark,

alm

ost b

lack

met

eorit

e in

two

larg

e re

d lim

esto

ne p

late

s (e

ach

400

× 40

0 ×

25 m

m).

Ligh

t red

uctio

n ha

los (

85 ×

85

mm

). W

orm

tra

cks a

long

the

rim o

f the

redu

ctio

n ha

lo. A

par

ticul

arly

shar

p-ed

ged

met

eorit

e.Ö

ster

plan

a 01

st 0

1210

-Sep

-199

658

°35′

13°2

6′58

× 2

1Lu

ndU

-1D

istin

ctly

elo

ngat

e, “

copr

olite

-sha

ped”

gra

y, g

reen

ish

and

redd

ish

met

eorit

e in

red

limes

tone

pla

te (2

15 ×

165

× 3

0m

m).

Öst

erpl

ana

013

Öst

013

11-M

ar-1

996

58°3

5′13

°26′

23 ×

34

Lund

U-1

Smal

l tea

rdro

p sh

aped

dar

k m

eteo

rite i

n re

d lim

esto

ne p

late

(215

× 2

37

× 22

mm

) with

wor

m b

urro

ws.

Prop

ortio

nally

larg

e (1

10 ×

110

mm

), bu

t diff

use

gray

redu

ctio

n ha

lo.

Öst

erpl

ana

014

Öst

014

11-A

pr-1

996

58°3

5′13

°26′

40 ×

30

Lund

U-1

Dar

k pe

ar-s

hape

d m

eteo

rite

in re

d lim

esto

ne p

late

(245

× 1

70 ×

30

mm

). Ve

ry in

tens

e and

dis

tinct

ligh

t ora

nge-

gray

redu

ctio

n ha

lo (8

0 ×

80 m

m).

Öst

erpl

ana

015

Öst

015

1-Ju

n-19

9658

°35 ′

13°2

6′23

×15

× >

11Lu

ndU

-1G

ray

dist

inct

ly sq

uare

-sha

ped

met

eorit

e in

red

limes

tone

pla

te (1

35 ×

12

5 ×

12 m

m).

Diff

use,

but

larg

e gr

ay re

duct

ion

halo

(70

× 60

mm

).

Öst

erpl

ana

016

Öst

016

4-A

ug-1

996

58°3

5′13

°26′

22 ×

15

Lund

U-1

Dar

k m

eteo

rite

in re

d lim

esto

ne p

late

(95

× 14

5 ×

12 m

m).

Thin

, ver

y in

tens

e ora

nge-

gray

redu

ctio

n ha

lo (2

8 ×

24m

m).

Larg

e nau

tiloi

d sh

ell

in p

late

(ver

tical

cro

ss se

ctio

n of

two

cham

bers

).Ö

ster

plan

a 01

st 0

1715

-May

-199

758

°35′

13°2

6′20

× 2

7Lu

ndU

-1Ve

ry d

ark,

alm

ost b

lack

squa

red

to su

brou

nded

met

eorit

e in

larg

e re

d lim

esto

ne p

late

(400

× 2

50 ×

34

mm

) with

larg

e na

utilo

id sh

ell

span

ning

alm

ost d

iago

nally

acro

ss m

ost o

f the

pla

te. C

ham

bers

of s

hell

exce

llent

ly d

ispl

ayed

. Ver

y in

tens

e lig

ht g

ray

redu

ctio

n ha

lo (6

0 ×

60m

m) a

roun

d m

eteo

rite.

Wor

m tr

acks

alo

ng m

argi

n of

and

in

redu

ctio

n ha

lo.

Öst

erpl

ana

018

Öst

018

15-J

an-1

996

58°3

5′13

°26′

25 ×

32;

40

× 33

Lund

U-1

Very

dar

k, al

mos

t bla

ck m

eteo

rite,

som

ewha

t tria

ngul

ar-s

hape

d, in

two

red

limes

tone

pla

tes (

190

× 15

0 ×

12 an

d 19

0 ×

160

× 12

mm

). N

autil

oid

shel

l ext

endi

ng a

long

the

who

le lo

ng si

de o

f the

lim

esto

ne p

late

. Pla

te

cuts

thro

ugh

shel

l. R

educ

tion

halo

(60

× 50

mm

).

Tabl

e 7.

Con

tinue

d. A

list

of a

ppro

ved

relic

t met

eorit

es fr

om S

wed

en.

Nam

eA

bbre

viat

ion

Dat

e of

re

cove

ryLo

ngitu

de(N

)La

titud

e(E

)A

ppro

xim

ate

size

s(c

ross

sect

ions

in m

m)

Info

Com

men

ts

1692 H. C. Connolly, Jr., et al.

Öst

erpl

ana

019

Öst

019

15-A

pr-1

997

58°3

5′13

°26′

35 ×

20;

40

× 65

Lund

U-1

Larg

e da

rk m

eteo

rite

in tw

o la

rge

red

limes

tone

pla

tes (

500

× 30

0 ×

12m

m an

d 52

0 ×

300

× 13

mm

). In

one

pla

te ex

celle

ntly

pre

serv

ed lo

ng

naut

iloid

shel

l with

per

fect

ly e

xpos

ed c

ham

bers

and

siph

uncl

e cr

osse

s pl

ate

alm

ost d

iago

nally

. In

seco

nd p

late

mor

e di

ffuse

impr

int o

f the

sa

me

shel

l. W

eak

impr

ints

als

o of

oth

er sh

ells

in th

e tw

o pl

ates

. Met

e-or

ite o

ccur

s in

one

of th

e co

rner

s of t

he la

rge

plat

es.

Öst

erpl

ana

020

Öst

020

10-J

un-1

997

58°3

5′13

°26′

25 ×

17

Lund

U-1

Dar

k m

eteo

rite

with

“ru

gged

” m

argi

ns in

red

limes

tone

pla

te (2

20 ×

17

0 ×

12 m

m).

Met

eorit

e in

corn

er o

f pla

te. T

hin,

inte

nse r

educ

tion

halo

(3

5 ×

30 m

m).

Öst

erpl

ana

021

Öst

021

15-J

un-1

997

58°3

5′13

°26′

abou

t 12

× 25

Lund

U-1

Gra

y, su

brou

nded

to sq

uare

shap

ed m

eteo

rite

in re

d lim

esto

ne st

eps o

f th

e ga

rden

of G

unne

bo c

astle

. Met

eorit

e is

pre

sent

ly w

eath

erin

g at

a

fast

rate

ster

plan

a 02

st 0

2227

-Nov

-199

958

°35′

13°2

6′18

× 1

8Lu

ndU

-1D

ark

met

eorit

e w

ith fi

ve su

brou

nded

cor

ners

in re

d lim

esto

ne p

late

(~

110

× 11

0 ×

23 m

m).

One

side

of p

late

cut d

iago

nally

giv

ing

the p

late

a

som

ewha

t tria

ngul

ar a

ppea

ranc

e (b

ut st

ill fo

ur c

orne

rs).

Inte

nse,

so

lar-c

oron

a lik

e, re

duct

ion

halo

(50

× 50

mm

).Ö

ster

plan

a 02

st 0

232-

Dec

-199

958

°35′

13°2

6′40

× 3

5; 5

0 ×

30Lu

ndU

-1D

ark

met

eorit

e in

two

very

larg

e red

lim

esto

ne p

late

s (ea

ch 1

200

× 70

0 ×

24 m

m).

Man

y na

utilo

id sh

ells

on

plat

e. In

tens

e re

duct

ion

halo

s (70

×

60 m

m).

Öst

erpl

ana

024

Öst

024

2-D

ec-1

999

58°3

5′13

°26′

25 ×

15

Lund

U-1

Dar

k el

onga

te m

eteo

rite

in ro

ugh

red

limes

tone

blo

ck (n

ot sa

wed

or

polis

hed)

(130

× 9

0 m

m).

Prom

inen

t lig

ht g

ray

redu

ctio

n ha

lo (6

0 ×

50m

m).

Öst

erpl

ana

025

Öst

025

29-M

ar-2

000

58°3

5′13

°26′

11 ×

7Lu

ndU

-1Ve

ry sm

all d

ark

met

eorit

e in

pro

porti

onal

ly v

ery

larg

e re

d lim

esto

ne

plat

e (5

70 ×

740

× 3

0m

m).

Two

larg

e na

utilo

id sh

ells

in p

late

. Thi

n,

inte

nse

redu

ctio

n ha

lo (1

5 ×

11 m

m).

Öst

erpl

ana

026

Öst

026

17-M

ar-2

000

58°3

5′13

°26′

50 ×

30

Lund

U-1

Dar

k m

eteo

rite

in v

ery

larg

e re

d lim

esto

ne p

late

(111

5 ×

735

× 18

). In

tens

e re

duct

ion

halo

(50

× 60

mm

). Tw

o ve

ry la

rge

naut

iloid

shel

ls

(560

and

350

mm

) in

plat

e. O

ne o

nly

abou

t 100

mm

from

met

eorit

e.

Öst

erpl

ana

027

Öst

027

29-M

ar-2

000

58°3

5′13

°26′

60 ×

55;

50

× 70

Lund

U-1

Dar

k m

eteo

rite

with

shap

e si

mila

r to

Indi

an su

bcon

tinen

t in

two

red

limes

tone

pla

tes (

415

× 35

5 ×

30 a

nd 6

60 ×

400

× 3

0 m

m).

Plat

es w

ith

very

inte

nse

red

and

oran

ge c

olor

s, pr

omin

ent r

educ

tion

halo

(abo

ut

110

× 11

0 m

m).

Öst

erpl

ana

028

Öst

028

11-S

ep-2

000

58°3

5′13

°26′

30 ×

20

Lund

U-1

Gra

y m

eteo

rite,

shap

e som

ewha

t tria

ngul

ar, b

ut ro

unde

d co

rner

s, in

red

limes

tone

pla

te (3

85 ×

200

× 2

2 m

m).

Com

para

tivel

y la

rge,

but

diff

use

redu

ctio

n ha

lo (9

0 ×

90m

m).

Hal

o ch

ange

s col

or fr

om g

ray

to re

ddis

h gr

ay. W

orm

bur

row

s in

redu

ctio

n ha

lo.

Öst

erpl

ana

029

Öst

029

2-O

ct-1

998

58°3

5′13

°26′

80 ×

50

× 20

; 80

× 50

; 80

× 5

0Lu

ndU

-1Lo

ose m

eteo

rite a

nd tw

o bl

ocks

with

the e

nclo

sing

red

limes

tone

. In

the

bloc

ks th

ere

are

impr

ints

mad

e by

the

met

eorit

e. S

ome

met

eorit

ic

mat

eria

l is l

eft i

n th

ese

depr

essi

ons.

The

loos

e m

eteo

rite

has a

co

mpr

esse

d ap

pear

ance

; it i

s dar

k gr

eeni

sh g

ray.

In th

e tw

o bl

ocks

(e

ach

230

× 26

0 ×

30 m

m) w

ith d

ark

gray

to b

lack

impr

ints

of t

he

met

eorit

es th

ere

are

also

larg

e gr

ay re

duct

ion

halo

s.Ö

ster

plan

a 03

st 0

308-

Apr

-199

458

°35′

13°2

6′80

× 1

24; 8

0 ×

124

Lund

U-1

Larg

e bl

ack

roun

ded

(som

ewha

t bea

n- o

r kid

ney-

shap

ed) m

eteo

rite

in

two

gray

lim

esto

ne p

late

s (ea

ch 3

15 ×

315

× 3

0m

m).

Tabl

e 7.

Con

tinue

d. A

list

of a

ppro

ved

relic

t met

eorit

es fr

om S

wed

en.

Nam

eA

bbre

viat

ion

Dat

e of

re

cove

ryLo

ngitu

de(N

)La

titud

e(E

)A

ppro

xim

ate

size

s(c

ross

sect

ions

in m

m)

Info

Com

men

ts

The Meteoritical Bulletin, No. 92 1693

Öst

erpl

ana

031

Öst

031

15-S

ep-1

998

58°3

5′13

°26′

50 ×

50;

65

× 45

Lund

U-1

Bla

ck m

eteo

rite

(look

s alm

ost l

ike

opal

) in

two

gray

lim

esto

ne p

late

s (1

60 ×

80

× 60

and

160

× 90

× 5

0 m

m).

The l

arge

r met

eorit

e par

t on

one

plat

e has

thre

e ver

y sh

arp

corn

ers,

like a

tria

ngle

, but

the “

hypo

tenu

se”

is c

urve

d. T

he o

ther

smal

ler p

art o

n a

sepa

rate

pla

te re

pres

ents

a c

ut

thro

ugh

the m

argi

n of

the m

eteo

rite.

The

shap

e of t

his m

eteo

rite p

art i

s en

tirel

y di

ffere

nt fr

om th

e la

rger

par

t: tw

o ar

eas,

one

roun

d, o

ne tr

ian-

gula

r con

nect

ed b

y a

thin

brid

ge.

Öst

erpl

ana

032

Öst

032

11-S

ep-2

000

58°3

5′13

°26′

210

× 65

× 4

1;

210

× 65

× 5

0Lu

ndU

-1La

rges

t met

eorit

e fo

und

by 2

006.

Occ

urs i

n tw

o gr

ay li

mes

tone

blo

cks

(eac

h 73

0 ×

180

× 65

mm

). Th

e saw

has

cut t

he b

lock

s and

the m

eteo

rite

perp

endi

cula

rly re

lativ

e to

the

sea

floor

. Met

eorit

e ha

s fis

h-lik

e sh

ape.

W

ell d

ispl

ayed

har

dgro

unds

in b

lock

s. O

ne p

rom

inen

t har

dgro

und

a fe

w c

entim

eter

s bel

ow m

eteo

rite.

Met

eorit

e its

elf n

ot o

n ha

rdgr

ound

bu

t has

sunk

into

the

orig

inal

ly so

ft se

dim

ent.

Öst

erpl

ana

033

Öst

033

12-O

ct-2

000

58°3

5′13

°26′

50 ×

25;

65

× 35

Lund

U-1

Dar

k el

liptic

al, r

ound

ed m

eteo

rite

in tw

o gr

ay li

mes

tone

pla

tes (

300

× 29

0 ×

40 a

nd 4

00 ×

400

× 3

0 m

m).

Prom

inen

t fre

sh c

rack

s thr

ough

the

met

eorit

e pa

rt on

the

smal

ler p

late

ster

plan

a 03

st 0

342-

Nov

-199

858

°35′

13°2

6′20

× 2

5; 1

6 ×

26Lu

ndU

-1D

ark

gray

to b

lack

, vag

uely

squa

re-s

hape

d m

eteo

rite

in tw

o lim

esto

ne

plat

es (e

ach

165

× 14

5 ×

30 m

m) w

ith th

e ch

arac

teris

tic re

ddis

h gr

ay

colo

r of t

he F

lora

bed

.

Öst

erpl

ana

035

Öst

035

20-M

ar-1

996

58°3

5′13

°26′

80 ×

60

× 15

; 85

× 7

0 ×

30;

42 ×

40

×31

Lund

U-1

Perh

aps t

he m

ost b

eaut

iful a

nd p

erfe

ct fo

ssil

met

eorit

e fo

und

by 2

006.

A

larg

e ro

unde

d m

eteo

rite,

with

per

fect

ly p

rese

rved

cho

ndru

le

stru

ctur

es a

lmos

t thr

ough

out t

he e

ntire

exp

osed

met

eorit

e su

rfac

e.

Stru

ctur

e of

an

extra

neou

s cla

st in

orig

inal

met

eorit

e al

so p

rese

rved

. M

eteo

rite

occu

rs in

thre

e pl

ates

of r

ed li

mes

tone

(195

× 2

90 ×

31;

195

×

300

× 30

and

195

× 3

00 ×

30

mm

). O

ne p

late

con

tain

s a n

ot-s

o-ni

ce

cut t

hrou

gh th

e m

argi

n of

the

met

eorit

e. T

he tw

o ot

her p

late

s con

tain

th

e ex

celle

nt c

uts a

nd te

xtur

ally

pre

serv

ed su

rfac

es th

roug

h th

e m

eteo

rite.

The

upp

er a

nd lo

wer

par

t of a

nau

tiloi

d sh

ell i

s exp

osed

on

each

of t

hese

two

plat

es. P

rom

inen

t wor

m tr

acks

aro

und

met

eorit

e.

Out

er p

arts

of m

eteo

rite

have

flak

y ap

pear

ance

. Ö

ster

plan

a 03

st 0

3624

-Oct

-199

658

°35′

13°2

6′65

× 4

4; 6

5 ×

44Lu

ndU

-1D

ark

wea

ther

ed, “

ugly

” met

eorit

e at c

rack

surf

ace i

n tw

o re

d lim

esto

ne

bloc

ks/p

late

s (30

0 ×

110

× 31

mm

and

320

× 11

0 ×

31 m

m).

Onl

y a p

art

of th

e m

eteo

rite

is p

rese

rved

and

it o

ccur

s at t

he m

argi

n of

the

two

bloc

ks.

Öst

erpl

ana

037

Öst

037

2-O

ct-1

998

58°3

5′13

°26′

60 ×

45;

60

× 50

Lund

U-1

Stro

ngly

wea

ther

ed, b

row

nish

met

eorit

e in

two

red

limes

tone

blo

cks

(460

× 2

20 ×

50

and

470

× 22

0 ×

50 m

m).

Very

larg

e gr

ay re

duct

ion

halo

(230

× 1

60 m

m).

From

the

low

est p

art o

f the

Sex

tum

men

bed

, the

s.k

. Måc

ka b

ed.

Öst

erpl

ana

038

Öst

038

15-J

un-1

999

58°3

5′13

°26′

40 ×

20

× 18

Lund

U-1

Dar

k, ru

st b

row

n m

eteo

rite i

n re

d lim

esto

ne p

late

(150

× 1

30 ×

25

mm

). M

eteo

rite

at m

argi

n of

pla

te a

nd sa

wed

thro

ugh

both

the

verti

cal a

nd

horiz

onta

l dire

ctio

ns. L

arge

diff

use

redu

ctio

n ha

lo (1

10 ×

110

mm

).Ö

ster

plan

a 03

st 0

3911

-Sep

-200

058

°35′

13°2

6′35

× 3

2Lu

ndU

-1St

rong

ly w

eath

ered

bro

wn

met

eorit

e in

lim

esto

ne b

lock

(300

× 2

80 ×

28

0 m

m).

Gra

y re

duct

ion

halo

(120

× 1

20m

m).

Öst

erpl

ana

040

Öst

040

10-J

un-2

000

58°3

5′13

°26′

30 ×

14

Lund

U-1

Smal

l lip

-sha

ped

met

eorit

e in

red

limes

tone

pla

te (2

05 ×

230

×

100

mm

).Ö

ster

plan

a 04

st 0

4119

9658

°35′

13°2

6′20

× 1

5Lu

ndU

-1D

ark

met

eorit

e in

red

limes

tone

blo

ck (1

15 ×

135

× 6

5m

m).

Met

eorit

e-ex

posi

ng si

de o

f blo

ck is

a ra

w (i

.e.,

not s

awed

) roc

k su

rfac

e, o

ther

side

s sa

wed

. Pro

min

ent g

ray

redu

ctio

n ha

lo (8

0 ×

80 m

m).

Tabl

e 7.

Con

tinue

d. A

list

of a

ppro

ved

relic

t met

eorit

es fr

om S

wed

en.

Nam

eA

bbre

viat

ion

Dat

e of

re

cove

ryLo

ngitu

de(N

)La

titud

e(E

)A

ppro

xim

ate

size

s(c

ross

sect

ions

in m

m)

Info

Com

men

ts

1694 H. C. Connolly, Jr., et al.

Öst

erpl

ana

042

Öst

042

11-S

ep-2

000

58°3

5′13

°26′

35 ×

30

Lund

U-1

Stro

ngly

bro

wn-

wea

ther

ed ro

und

met

eorit

e in

dark

red

limes

tone

blo

ck

(280

× 3

00 ×

80

mm

). Th

e m

eteo

rite

is n

ot sa

wed

, but

exp

osed

on

a ro

ugh

rock

surf

ace.

Pro

min

ent g

ray

redu

ctio

n ha

lo (1

20 ×

130

mm

).Ö

ster

plan

a 04

st 0

4317

-Feb

-200

258

°35′

13°2

6′15

× 1

5Lu

ndU

-1Sm

all d

ark

met

eorit

e in

red

limes

tone

pla

te (2

30 ×

200

× 2

8m

m).

Öst

erpl

ana

044

Öst

044

17-M

ar-2

002

58°3

5′13

°26′

50 ×

40

Lund

U-1

Med

ium

-siz

ed m

eteo

rite

with

ver

y ru

sty

appe

aran

ce in

red

limes

tone

bl

ock

(115

× 8

5 ×

55 m

m).

Som

e si

des o

f blo

ck sa

wed

, oth

ers r

ough

ro

ck su

rfac

es. M

eteo

rite

saw

ed th

roug

h bo

th in

ver

tical

and

hor

izon

tal

dire

ctio

ns.

Öst

erpl

ana

045

Öst

045

7-M

ay-2

002

58°3

5′13

°26′

35 ×

20

Lund

U-1

Dar

k m

eteo

rite i

n re

d lim

esto

ne b

lock

(170

× 1

30 ×

48

mm

). M

eteo

rite-

expo

sed

surf

ace

not s

awed

, but

side

s of b

lock

are

saw

ed. P

rom

inen

t gr

ay re

duct

ion

halo

(90

× 70

mm

).Ö

ster

plan

a 04

st 0

465-

May

-200

258

°35′

13°2

6′20

× 1

3Lu

ndU

-1D

ark

met

eorit

e in

red

limes

tone

pla

te (9

1 ×

60 ×

11

mm

). In

tens

e lig

ht

redu

ctio

n ha

lo (4

0 ×

34 m

m).

Met

eorit

e ha

s som

ewha

t rec

tang

ular

ap

pear

ance

, with

two

shar

p co

rner

s on

one

of th

e sh

ort s

ides

, but

op

posi

ng si

de h

as ro

unde

d co

rner

s.Ö

ster

plan

a 04

st 0

4721

-Nov

-200

258

°35′

13°2

6′37

× 2

7; 3

1 ×

20Lu

ndU

-1D

ark

met

eorit

e in

two

gray

lim

esto

ne p

late

s (10

6 ×

136

× 29

and

106

× 13

6 ×

54 m

m).

Met

eorit

e sa

wed

in p

erpe

ndic

ular

dire

ctio

n re

lativ

e to

se

a flo

or. O

rthoc

erat

ite sh

ell (

verti

cal c

ut) a

t the

side

abo

ve m

eteo

rite.

G

ullh

ögen

001

Gul

001

14-J

un-2

000

58°2

3′13

°48′

12 m

mLu

ndU

-3A

lmos

t rou

nd g

ray

stru

ctur

e in

two

red

Orth

ocer

atite

lim

esto

ne b

lock

s. Su

rrou

nded

by

5 cm

redu

ctio

n ha

lo.

Tabl

e 7.

Con

tinue

d. A

list

of a

ppro

ved

relic

t met

eorit

es fr

om S

wed

en.

Nam

eA

bbre

viat

ion

Dat

e of

re

cove

ryLo

ngitu

de(N

)La

titud

e(E

)A

ppro

xim

ate

size

s(c

ross

sect

ions

in m

m)

Info

Com

men

ts