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Northwest Africa 7034

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Northwest Africa 7034
Northwest Africa 7034, nicknamed "Black Beauty"
TypeAchondrite
ClanMartian meteorite
GroupletMartian (basaltic breccia)[1]
CompositionPlagioclase and pyroxene phenocrysts in a fine groundmass.[2]
Weathering gradeMinimal[1]
CountryWestern Sahara, Morocco
Coordinates24°5.311′N 14°46.671′W / 24.088517°N 14.777850°W / 24.088517; -14.777850[3]
(purchased from dealer)[1]
Observed fallNo
Found date2011
TKW320 grams (11 oz)[1]

Northwest Africa 7034 is a Martian meteorite.[4] It contains portions[5] estimated to be 4.43 billion years old and contains the most water of any Martian meteorite found on Earth.[6] Although it is from Mars it does not fit into any of the three SNC meteorite categories, and forms a new Martian meteorite group named "Martian (basaltic breccia)".[1] Nicknamed "Black Beauty", it was purchased in Morocco and a slice of it was donated to the University of New Mexico by its American owner.[1] The image (shown on the right) of the original NWA 7034 was photographed in 2012 by Carl Agee, University of New Mexico.

Discovery and naming

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The meteorite was found by nomads in Rabt Sbayta, Ghredad Sabti region, Western Sahara,[3] in the Sahara Desert in 2011,[7] and was purchased in Morocco by a meteorite dealer who sold it to a collector in the United States,[1] as Morocco does not have meteorite export control laws. Like all meteorites that are found in large numbers or sold at markets the name stands for the geographic region (Northwest Africa) and a number, which is given out consecutively.[8] NWA 7034 carries the nickname "Black Beauty".[4][9]

Description

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NWA 7034 consists of hundreds of fragments stuck together, containing both very old and very young rocks.[5] It was originally described as a volcanic breccia that has a porphyritic appearance, consisting of plagioclase (andesine) and pyroxene (pigeonite and augite) phenocrysts that are up to 5 mm in diameter set in a fine grained groundmass. Accessory minerals include chlorapatite, chromite, goethite, ilmenite, magnetite, maghemite, alkali feldspar and pyrite.[6] There are even some clasts present that are made of quenched magma. The groundmass is made from fine grained plagioclase, pyroxene, different oxide minerals, and traces of iron sulfides.[1] The whole rock chemistry revealed that NWA 7034 has the highest water content ever measured in a Martian meteorite.[7] The water might be derived from oceans that used to exist on Mars, but were still present when the volcanic rock, that would eventually become the meteorite, was erupted.[10]

The meteorite contains components as old as 4.42 ± 0.07 Ga (billion years),[11] and was heated during the Amazonian period of Mars.[12] It is the second oldest Martian meteorite known.[6][7][13] However, a team of Japanese researchers who studied the meteorite concluded that water on Mars originated around 4.4 billion years ago.[14]

Classification

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NWA 7034 is the first Martian meteorite that is a breccia and does not fall in any of the known Martian meteorite groups (shergottite, nakhlite, chassignite and ALH 84001).[2] NWA 7034 was classified as an ungrouped planetary achondrite until the Meteoritical Society approved the new designation "Martian (basaltic breccia)" in January 2013. The iron/manganese ratio is consistent with that of other Martian meteorites, but the oxygen isotopes do not correlate with a Martian origin. The change in oxygen isotope ratios could be explained by removal or addition of heavier or lighter isotopes, or by mixing with a mass with a different isotopic ratio. This could happen during aqueous alteration of the Martian crust. Another explanation would be an isotopic contamination of the Martian crust during impact brecciation.[2]

In 2018 the Nomenclature Committee of the Meteoritical Society accepted a petition to reclassify the NWA 7034 pairing group as "Martian (polymict breccia)". The older term, "basaltic breccia," was held to be unsuitable because the stones contain a variety of clast types, including impact melts, sedimentary rocks, and a wide variety of other lithologies.

Origin

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A 2022 study concluded that meteorite NWA 7034 was ejected from Mars by the impact that formed the crater Karratha about 5-10 million years ago in the Terra Cimmeria-Terra Sirenum region of the southern highlands. The authors proposed that before its ejection, this meteorite was part of the ejecta deposits from an earlier impact that formed the nearby Khujirt crater approximately 1.5 billion years ago.[15]

See also

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References

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  1. ^ a b c d e f g h "NWA 7034". Meteoritical Society. Retrieved 4 January 2013.
  2. ^ a b c Agee, C. B.; N.V. Wilson; F.M. McCubbin; Z.D. Sharp; et al. (2012). "Basaltic Breccia NWA 7034: New ungrouped planetary Achondrite" (PDF). 43rd Lunar and Planetary Science Conference (1659): 2690. Bibcode:2012LPI....43.2690A. Retrieved 4 January 2013.
  3. ^ a b "Northwest Africa 7034/7533 and pairings". Meteorite Studies.
  4. ^ a b Associated Press (January 4, 2013). Mars meteorite 'Black Beauty' contains most water of any found on Earth, say scientists. The Guardian
  5. ^ a b James Woodford (Nov 22, 2024). "Meteorite crystals show evidence of hot water on ancient Mars". New Scientist.
  6. ^ a b c Lagain, A.; Bouley, S.; Zanda, B.; Miljković, K.; Rajšić, A.; Baratoux, D.; Payré, V.; Doucet, L. S.; Timms, N. E.; Hewins, R.; Benedix, G. K.; Malarewic, V.; Servis, K.; Bland, P. A. (2022-07-12). "Early crustal processes revealed by the ejection site of the oldest martian meteorite". Nature Communications. 13 (1): 3782. doi:10.1038/s41467-022-31444-8. ISSN 2041-1723. PMC 9276826.
  7. ^ a b c Staff (January 3, 2013). "Researchers Identify Water Rich Meteorite Linked To Mars Crust". NASA. Retrieved January 3, 2013.
  8. ^ "Guidelines for meteorite nomenclature". Meteoritical Society. p. Section 3.4)c) and Section 3.5. Retrieved 4 January 2013.
  9. ^ Tills 2013, p. 111.
  10. ^ "Mars Meteorite May Be Missing Link to Red Planet's Past". Space.com. 3 January 2013. Retrieved 5 January 2013.
  11. ^ Nyquist, Laurence E.; Shih, Chi-Yu; McCubbin, Francis M.; Santos, Alison R.; Shearer, Charles K.; Peng, Zhan X.; Burger, Paul V.; Agee, Carl B. (2016-02-17). "Rb-Sr and Sm-Nd isotopic and REE studies of igneous components in the bulk matrix domain of Martian breccia Northwest Africa 7034". Meteoritics & Planetary Science. 51 (3): 483–498. Bibcode:2016M&PS...51..483N. doi:10.1111/maps.12606. ISSN 1086-9379. S2CID 131565237.
  12. ^ Cassata, William S.; Cohen, Benjamin E.; Mark, Darren F.; Trappitsch, Reto; Crow, Carolyn A.; Wimpenny, Joshua; Lee, Martin R.; Smith, Caroline L. (2018-05-01). "Chronology of martian breccia NWA 7034 and the formation of the martian crustal dichotomy". Science Advances. 4 (5): eaap8306. Bibcode:2018SciA....4.8306C. doi:10.1126/sciadv.aap8306. ISSN 2375-2548. PMC 5966191. PMID 29806017.
  13. ^ Williams, Rob (4 January 2013). "'Black Beauty' rock is a 2 billion year old unique 'meteorite' from Mars, say scientists". London: Independent. Archived from the original on 2022-06-21. Retrieved 5 January 2013.
  14. ^ "Water was formed 4.4 billion years ago on Mars: Study". Telangana Today. 1 November 2020.
  15. ^ Lagain, A.; Bouley, S.; Zanda, B.; Miljković, K.; Rajšić, A.; Baratoux, D.; Payré, V.; Doucet, L. S.; Timms, N. E.; Hewins, R.; Benedix, G. K. (2022-07-12). "Early crustal processes revealed by the ejection site of the oldest martian meteorite". Nature Communications. 13 (1): 3782. Bibcode:2022NatCo..13.3782L. doi:10.1038/s41467-022-31444-8. ISSN 2041-1723. PMC 9276826. PMID 35821210.

Book sources

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