H Ordinary Chondrites


Dashoguz (41°59'4" N, 59°41'6" E)

Turkmenistan
Fell 1998 September 5
Ordinary chondrite (H5)

A meteor trail was witnessed near the city of Dashoguz, Turkmenistan. After a search of several weeks, a very small crater (depression) with ~7 kg of meteorite fragments was found. Kakabay Annaniyazov recovered fresh, grey fragments from the rim of the crater and weathered, brown fragments from within the water-fill crater. Classification and mineralogy (T. Bunch and J. Wittke, NAU): olivine Fa17.5; pyroxene Fs15.3; plagioclase An14. Shock stage S3; weathering grade, W0/1 for the grey fragments, W4 for the brown fragments. Specimens: type specimen, 21.2 g and one thin section, NAU; main mass with anonymous purchaser.


New Orleans (29°56.8305' N, 90°6.5855' W)

New Orleans, Louisiana USA
Fell 2003 September 23. approx. 16:05 hrs (CST)
Ordinary chondrite (H5)

On the afternoon of September 23rd 2003, a meteorite tore through the two-storey home of Ray and Judy Fausset, who were not at home at the time. Neighbors said that they heard a "terrific noise." Two observations of a fireball were recorded. The main mass of the meteorite was found in the crawl space under the house. Powdery meteorite debris and fragments were found along the penetration path throughout the house. A total mass of 19,256 g was recovered from the Fausset house, the three largest fragments weighing 2966 g, 1292 g and 1001 g. Some additional material (~100 g) was also recovered in the surrounding neighborhood. Description and classification (S. Nelson, Tulane University; R. Jones and A. Brearley, UNM; T. Bunch and J. Wittke, NAU): The meteorite is light grey with a black fusion crust, and very friable. Abundant metal and troilite are visible on broken surfaces, as well as some thin (mm-thick) impact melt veins. Classification and mineralogy: The meteorite is very fragmented on a sub-mm scale. Mean compositions of olivine, Fa17.6; orthopyroxene, Fs15.4Wo1.4; clinopyroxene, Fs10.4Wo24.8; plagioclase, An12.8Or5.6; metal, Ni = 6.7 wt %, Co = 0.83 %. Minor chromite and phosphate are present. The meteorite broke a pipe and many fragments sat in water for several days. Because of this and the humid climate in New Orleans, light oxidation of interior metal within small fragments (<100 g) was evident within a week of the fall. Shock level, S1. Specimens: 82 g, UNM; 63 g, NAU; main mass with owner.

New Orleans H5. Arrow points to hole in roof. Image source: http://www.marmet-meteorites.com/sitebuildercontent/sitebuilderpictures/.pond/new.orleans.2.jpg.w560h420.jpg


Northwest Africa 2058

Morocco
2001
Ordinary chondrite (H melt rock)

Five fresh, fully crusted stones with unusually smooth fusion crust (total weight of 80.1 g) were purchased in Zagora, Morocco in 2001. Classification and mineralogy (T. Bunch and J. Wittke, NAU): melt mass of >90 vol. % that consists mostly of euhedral olivine crystals (<0.01 mm) with minor orthopyroxene and micron- to submicron-size metal spherules set in feldspathic glass. Within this mass are mm size elongated metal–sulfide nodules of eutectic texture. These nodules together with connecting metal veins form a network subparallel to the flow direction of the melt mass. No apparent vesiculation. Relict olivine (Fa17.1-18.4) and orthopyroxene (Fs15.8-16.5) chondrule fragments (<0.05 mm in diameter) are randomly distributed throughout the melt mass. Nodule metal: Ni, 7.8 wt %; Co, 0.75 %; Cr, 0.37 % and P, 0.57 %. Shock level, S6; weathering grade, W2/3. Specimens: type specimen, 17.1 g, NAU; main mass, Hupé.


Northwest Africa 2390

Northwest Africa
Purchased July 2004
Ordinary Chondrite (melt breccia, recrystallized)

A 231 g stone was purchased in Erfoud, Morocco. Description and classification (J. Wittke and T. Bunch, NAU): lightly shocked, brecciated L4 host with massive, recrystallized shock melt. Large, isolated metal-sulfide blebs display typical melt-eutectic texture. Recrystallized silicates are fine-grained (<0.02 mm) and show only localized flow fabric. Host olivine, Fa25.3; orthopyroxene, Fs21.1. Recrystallized olivine and pyroxene are moderately equilibrated and more consistent with an H composition than with L composition, Fa15.4–18.9; orthopyroxene, Fs11.0-15.3. Either reduction of silicate FeO occurred during melt/recrystallization or the impactor/target chondrite types were dissimilar. Shock level, S2-6; weathering grade is W2. Specimens: type sample, 22.3 g, NAU; main mass, Burkhard.


Other H Ordinary Chondrites

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ID Location Country Date Class. Mass (g) State Fa Fs Comments
Dho 96419°7.56" N, 54°51.38" EOman2004H41592S2, W418.516.6
Dho 96819°13'26.6" N, 54°56'0.96" EOman2004H479S1, W218.416.5-
Dho 97219°23.11' N, 54°50.02' EOman2004H58.1S2, W318.516.0-
Dho 97719°13'16.3" N, 54°57'34.6" EOman2004H31,728S1, W216.9-18.514.2-17.7 -
Dho 98319°10.27' N, 54°54.36' EOman2004H682.6S3, W517.916.1-
Dho 98419°11.84' N, 54°55.03' EOman2004H433.0S2, W417.515.6-
Dho 113019°13'23.9" N, 54°56'8.8" EOman13-1-05H43420S2, W217.716-
Dho 113619°16'29.2" N, 54°40'22.7" EOman13-1-05H529.1S2, W218.816.5-
Dho 115619°45'5.9" N, 54°21'8.5" EOman15-1-05H4108S2, W516.814.8-
Dho 118118°44'44.5" N, 54°16'1.8" EOman18-1-05H51812S3, W417.715.8-
Dho 123218°53'44.4" N, 54°20'36.8" EOman28-2-05H41088S2, W317.515.7-
JaH 07519°14.78' N ,55°2.39' E-2004H5107.6S2, W418.516.3-
NWA 1692SafsafMorocco10/2002H5857S1, W117.817-
NWA 1693SafsafMorocco10/2002H583S1, W2-319.117.5-
NWA 1792SafsafMorocco10/2002H539S1, W218.916.8-
NWA 1837ErfoudMorocco2003H445S2, W117.916.1-
NWA 1931RissaniMorocco6/2003H5267S1, W119.116.5-
NWA 1936GolmimaMorocco5/2003H42146S1, W118.616.9-
NWA 1944ZagoraMorocco6/2001H4632S1, W2-317.916.5-
NWA 2055ZagoraMorocco2001H4148S2-3, W118.0-18.416.6-17.0-
NWA 2057ErfoudMorocco2003H4958S2, W218.416.3-
NWA 2070ErfoudMorocco2002H490S5, W118.616.5shock darkened
NWA 2071ErfoudMorocco2002H4816S1, W117.916.2-
NWA 2073ErfoudMorocco2002H443.9S2, W118.116.0-
NWA 2077ErfoudMorocco2002H41077S2, W218.316.5-
NWA 2078ErfoudMorocco2003H534.8S2, W118.516.7oriented, disk-shaped
NWA 2087RissaniMorocco11/2003H535.1S2, W118.816.6Wo2.1
NWA 2108ErfoudMorocco2003H6384.7S4, W117.615.3shock darkened
NWA 2117ErfoudMorocco2003H5196.5S4, W219.316.3shock darkened
NWA 2123ErfoudMorocco2003H4351S2, W218.416.3-
NWA 2134ErfoudMorocco2004H6916S2, W318.416.3-
NWA 2143ErfoudMorocco2003H4700S2, W118.716.6few unusually large chondrules for an H (up to 3 mm)
NWA 2144ErfoudMorocco2003H4275S2, W217.715.4polymict breccia
NWA 2354ErfoudMorocco2002H5727S3, W219.617-
NWA 2361ErfoudMorocco2002H442S4, W118.715.9shock darkened
NWA 2371ErfoudMorocco2003H42,950S2, W219.517.0-
NWA 2378ErfoudMorocco2004H3.53,141S2, W24.2-22.6-Cr2O3 in olivine = 0.05-0.34 wt. %
NWA 2619-Morocco2004H4220S2, W318.216.4-
NWA 2620-Morocco2004H41,304S2, W218.516.9-
NWA 2630ErfoudMorocco2004H46,400S2, W218.716.4-
NWA 2638ErfoudMorocco2004H456S2, W317.115.8-
NWA 2648ErfoudMorocco2004H4304S1, W118.616.5-
NWA 2649ErfoudMorocco2004H4265S2, W118.816.9-
NWA 2660ErfoudMorocco2004H4215S2, W317.015.6-
NWA 2661ErfoudMorocco2004H6112S2, W318.716.8-
NWA 2662ErfoudMorocco2004H4145S1, W217.215.8-
NWA 2689ErfoudMorocco2004H4321S2-6, W318.916.7partial melt breccia
NWA 2692ErfoudMorocco2004H589S2, W217.816.2-
NWA 2694ErfoudMorocco2004H5214S2, W218.116.4-
NWA 2695ErfoudMorocco2004H4165S2, W219.017.0-
NWA 3101RissaniMorocco2003H6151.74S2, W118.816.7-
NWA 3107RissaniMorocco2003H666.85S2, W218.917.0-
NWA 3113ErfoudMorocco2003H3236S2, W216.2-18.814.8-15.4-
NWA 3115ZagoraMorocco2003H434.7S2, W218.216.3(photograph below)

Photographs of H Chondrites

NWA 3115. Image © T.E. Bunch 2005