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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 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.
1648 H. C. Connolly, Jr., et al.
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.
The Meteoritical Bulletin, No. 92 1649
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).
1650 H. C. Connolly, Jr., et al.
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.
The Meteoritical Bulletin, No. 92 1651
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
1652 H. C. Connolly, Jr., et al.
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
The Meteoritical Bulletin, No. 92 1661
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.
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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
3Ö
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
.Ö
ster
plan
a 00
6Ö
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
8Ö
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
.Ö
ster
plan
a 00
9Ö
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
.Ö
ster
plan
a 01
1Ö
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
2Ö
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
7Ö
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
.Ö
ster
plan
a 02
2Ö
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
3Ö
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
0Ö
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
.Ö
ster
plan
a 03
4Ö
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
6Ö
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
9Ö
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
1Ö
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
3Ö
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
6Ö
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
7Ö
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