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Hassi Messaoud 001 | |||||||||||||||||||||||||||||||||||||
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Basic information | Name: Hassi Messaoud 001 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2020 Country: Algeria Mass: ![]() | ||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 26 approved meteorites classified as Martian (nakhlite). [show all] Search for other: Martian meteorites | ||||||||||||||||||||||||||||||||||||
Comments: |
Approved 21 Feb 2021 Revised 4 Apr 2021: Fixed misspelled name | ||||||||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from MB 110:
Hassi Messaoud 001 31°51.11’N, 6°58.59’E Ouargla, Algeria Find: 2020 Mar 11 Classification: Martian meteorite (Nakhlite) History: Found on March 11, 2020, near the town of El Borma. Later acquired in 2021 by Matthew Stream from Aziz Zad. Physical characteristics: Specimen is grayish-brown and displays a slightly weathered, minor fusion crust. Petrography: (D. Sheikh, FSU) Specimen displays a cumulate texture (~1.1 mm grainsize) consisting primarily of compositionally zoned, prismatic or blocky (sometimes twinned) augite (displaying Fs-rich rims), ferroan olivine, and plagioclase; modal abundances: 75% augite, 15% plagioclase, 5% olivine. Accessory phases (modal abundance: 5%) are primarily found either in the mesostasis or within melt inclusions in augite or olivine grains; these phases include ferropigeonite, low-ca pyroxene, titanomagnetite, Si-Al-Na-Fe-K-rich glass, and fluorapatite. Geochemistry: Olivine (Fa73.3±1.0, range Fa72.6-74.5, Fe/Mn = 50±1, n=3), Augite (Fs30.1±4.7Wo38.4±1.4, range Fs22.8-37.9Wo34.9-40.3, Fe/Mn = 32±4, n=47), Pigeonite (Fs58.6±4.9 Wo9.9±3.8, range Fs53.3-62.9 Wo6.6-14.0, Fe/Mn = 31±2, n=5), Low-Ca Pyroxene (Fs64.5±4.1Wo3.1±0.9, range Fs61.1-70.2Wo3.0-5.3, Fe/Mn = 35±2, n=8), Plagioclase (An37.2±1.3Or2.9±0.5, range An35.3-39.4Or2.0-4.0, n=27). Classification: Martian (nakhlite). Sample is a martian meteorite due to the Fe/Mn ratios of olivine and pyroxene, and due to the plagioclase composition. Sample is a nakhlite due to the high modal abundance of augite and cumulate texture observed. Specimens: 15.2 g at UCLA, main mass with Matthew Stream. | ||||||||||||||||||||||||||||||||||||
Data from: MB110 Table 0 Line 0: |
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Institutions and collections |
UCLA: Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, United States (institutional address; updated 17 Oct 2011) FSU: Department of Geological Sciences, Florida State University, Tallahassee FL 32306-4100, United States (institutional address; updated 16 Dec 2010) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 110, in preparation (2021)
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Geography:![]() |
Statistics: This is 1 of 30 approved meteorites from Ouargla, Algeria This is 1 of 1088 approved meteorites from Algeria (plus 26 unapproved names) (plus 4 impact craters) | ||||||||||||||||||||||||||||||||||||
Proximity search: | |||||||||||||||||||||||||||||||||||||
Synonyms![]() |
Hassi Messauod (Original misspelled name) |