Northwest Africa 7034

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Northwest Africa 7034
MarsMeteorite-NWA7034-716969main black beauty full.jpg
Northwest Africa 7034, nicknamed "Black Beauty"
Type Achondrite
Clan Martian meteorite
Grouplet Martian (basaltic breccia) [1]
Composition Plagioclase and pyroxene phenocrysts in a fine groundmass. [2]
Weathering grade Minimal [1]
Country Western Sahara, Morocco
Coordinates 24°5.311′N14°46.671′W / 24.088517°N 14.777850°W / 24.088517; -14.777850 [3]
(purchased from dealer) [1]
Observed fall No
Found date2011
TKW 320 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.

Contents

Discovery and naming

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

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

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

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

Related Research Articles

<span class="mw-page-title-main">Martian meteorite</span> Meteorite made of rock originating from Mars

A Martian meteorite is a rock that formed on Mars, was ejected from the planet by an impact event, and traversed interplanetary space before landing on Earth as a meteorite. As of September 2020, 277 meteorites had been classified as Martian, less than half a percent of the 72,000 meteorites that have been classified. The largest complete, uncut Martian meteorite, Taoudenni 002, was recovered in Mali in early 2021. It weighs 14.5 kilograms and is on display at the Maine Mineral and Gem Museum.

<span class="mw-page-title-main">Allan Hills 84001</span> Martian meteorite discovered in Antarctica in 1984

Allan Hills 84001 (ALH84001) is a fragment of a Martian meteorite that was found in the Allan Hills in Antarctica on December 27, 1984, by a team of American meteorite hunters from the ANSMET project. Like other members of the shergottite–nakhlite–chassignite (SNC) group of meteorites, ALH84001 is thought to have originated on Mars. However, it does not fit into any of the previously discovered SNC groups. Its mass upon discovery was 1.93 kilograms (4.3 lb).

<span class="mw-page-title-main">Achondrite</span> Stony meteorite that does not contain chondrules

An achondrite is a stony meteorite that does not contain chondrules. It consists of material similar to terrestrial basalts or plutonic rocks and has been differentiated and reprocessed to a lesser or greater degree due to melting and recrystallization on or within meteorite parent bodies. As a result, achondrites have distinct textures and mineralogies indicative of igneous processes.

<span class="mw-page-title-main">HED meteorite</span> Group of achondrite meteorites

HED meteorites are a clan (subgroup) of achondrite meteorites. HED stands for "howardite–eucrite–diogenite". These achondrites came from a differentiated parent body and experienced extensive igneous processing not much different from the magmatic rocks found on Earth and for this reason they closely resemble terrestrial igneous rocks.

<span class="mw-page-title-main">Tooting (crater)</span> Volcanic crater on Mars

Tooting is an impact crater with volcanic features at 23.1°N, 207.1°E, in Amazonis Planitia, due west of the volcano Olympus Mons, on Mars. It was identified by planetary geologist Peter Mouginis-Mark in September 2004. Scientists estimate that its age is on the order of hundreds of thousands of years, which is relatively young for a Martian crater. A later study confirms this order of magnitude estimate. A preliminary paper describing the geology and geometry of Tooting was published in 2007 by the journal Meteoritics and Planetary Science, vol. 42, pages 1615–1625. Further papers have been published, including a 2010 analysis of flows on the walls of Tooting crater by A. R. Morris et al., and a 2012 review paper by P.J. Mouginis-Mark and J.M. Boyce in Chemie der Erde Geochemistry, vol. 72, p. 1–23. A geologic map has also been submitted in 2012 to the U.S. Geological Survey for consideration and future publication.

<span class="mw-page-title-main">Angrite</span> Rare group of achondrite meteorites

Angrites are a rare group of achondrites consisting mostly of Al-Ti bearing diopside, hedenbergite, olivine, anorthite and troilite with minor traces of phosphate and metals. The group is named for the Angra dos Reis meteorite. They are the oldest igneous rocks, with crystallization ages of around 4.56 billion years. Angrites are subdivided into two main groups, the quenched and plutonic angrites. The quenched angrites cooled rapidly upon the surface of the angrite parent body (APB), whereas the plutonic angrites cooled slower, deeper in the crust. The APB is thought to have been a similar size to the asteroid 4 Vesta.

<span class="mw-page-title-main">Nakhlite</span> Group of Martian meteorites

Nakhlites are a group of Martian meteorites, named after the first one, Nakhla meteorite.

<span class="mw-page-title-main">Tissint meteorite</span> Meteorite that fell in Tata, Guelmim-Es-Semara, Morocco in 2011

The Tissint meteorite is a Martian meteorite that fell in Tata Province in the Guelmim-Es Semara region of Morocco on July 18, 2011. Tissint is the fifth Martian meteorite that people have witnessed falling to Earth, and the first since 1962. Pieces of the meteorite are on display at several museums, including the Museum of Natural History of Vienna and the Natural History Museum in London.

Winonaites are a group of primitive achondrite meteorites. Like all primitive achondrites, winonaites share similarities with chondrites and achondrites. They show signs of metamorphism, partial melting, brecciation and relic chondrules. Their chemical and mineralogical composition lies between H and E chondrites.

This is a glossary of terms used in meteoritics, the science of meteorites.

Zachary D. Sharp is an American stable isotope geochemist. He is credited with the development of laser-based technology for measuring oxygen isotopes in silicates and oxides. His contributions include laser analyses of meteorites, paleoclimate reconstruction by oxygen and hydrogen isotope ratios, and analysis of isotopic composition of volcanoes, fossils, and forensic samples.

<span class="mw-page-title-main">Northwest Africa 7325</span>

Northwest Africa 7325, also known as NWA 7325, is a unique igneous meteorite which crystallized as a basalt on a large asteroid or planetesimal approximately 4.56 billion years ago. It is classified as an ungrouped achondrite, and is notable for its green fusion crust and high-magnesium/low-iron composition. It was purchased from anonymous finders in a marketplace in Erfoud, Morocco in April 2012. The original find was composed of 35 fragments with a combined weight of approximately 345 grams (12.2 oz), however many additional fragments with a total weight of over 1,100 grams (39 oz) were subsequently recovered.

<span class="mw-page-title-main">Elephant Moraine 79001</span> Meteorite found in Antarctica

Elephant Moraine 79001, also known as EETA 79001, is a Martian meteorite. It was found in Elephant Moraine, in the Antarctic during the 1979–1980 collecting season.

<span class="mw-page-title-main">Yamato 000593</span> Meteorite found in Antarctica

Yamato 000593 is the second largest meteorite from Mars found on Earth. Studies suggest the Martian meteorite was formed about 1.3 billion years ago from a lava flow on Mars. An impact occurred on Mars about 11 million years ago and ejected the meteorite from the Martian surface into space. The meteorite landed on Earth in Antarctica about 50,000 years ago. The mass of the meteorite is 13.7 kg (30 lb) and has been found to contain evidence of past water alteration.

Caroline Smith is the Head of Earth Sciences Collections and Principal Curator of Meteorites at the Natural History Museum in London, UK. She specializes in geochemistry, meteorites, microscopy, mineralogy, and public outreach.

<span class="mw-page-title-main">Karratha (crater)</span> Impact crater on Mars

Karratha is an impact crater in the Memnonia quadrangle of Mars. It was named after the town of Karratha, Western Australia, in 2021.

<span class="mw-page-title-main">Dampier (crater)</span> Impact crater on Mars

Dampier is an impact crater in the Memnonia quadrangle of Mars. It was named after the town of Dampier, Western Australia, in 2021.

<span class="mw-page-title-main">Khujirt (crater)</span> Impact crater on Mars

Khujirt is an impact crater in the Memnonia quadrangle of Mars. It was named after the district of Khujirt, central Mongolia, in 2021.

References

  1. 1 2 3 4 5 6 7 8 "NWA 7034". Meteoritical Society. Retrieved 4 January 2013.
  2. 1 2 3 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. 1 2 "Northwest Africa 7034/7533 and pairings". Meteorite Studies.
  4. 1 2 Associated Press (January 4, 2013). Mars meteorite 'Black Beauty' contains most water of any found on Earth, say scientists. The Guardian
  5. 1 2 James Woodford (Nov 22, 2024). "Meteorite crystals show evidence of hot water on ancient Mars". New Scientist.
  6. 1 2 3 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. 1 2 3 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.

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