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Item is a 0.06g crusted fragment of the recent witnessed martian meteorite fall in July 2010 near Foumzgit in the Tata region of Morocco. Specimens of this fall were first recovered a little more than a month ago. This meteorite has been analyzed and submitted for classification to the Meteoritical Society Nomenclature Committee, and should be approved for its official designation soon (the name "Tata" is nickname and will not be the formal name). This meteorite has been determined to originate from planet Mars, and is the first witnessed fall of a Martian meteorite in 49 years. And although Zagami was witnessed to fall in 1962 and is also a Shergottite SNC like Tata, it cannot compare in beauty with this incredible meteorite! Glossy flowlined fusion crust blanketing a matrix with olivine inclusions and glassy maskelynite and shock veins.

Writeup from MB 99:

Tissint        29°28.917’N, 7°36.674’W

Tata, Morocco

Fell: 18 July 2011

Classification: Martian meteorite (Shergottite)

History: (H. Chennaoui Aoudjehane, FSAC, and A. Aaronson) At about 2 am local time on July 18, 2011, a bright fireball was observed by several people in the region of the Oued Drâa valley, east of Tata, Morocco. One eyewitness, Mr Aznid Lhou, reported that it was at first yellow in color, and then turned green illuminating all the area before it appeared to split into two parts. Two sonic booms were heard over the valley. In October 2011, nomads began to find very fresh, fusion-crusted stones in a remote area of the Oued Drâa intermittent watershed, centered about 50 km ESE of Tata and 48 km SSW of Tissint village, in the vicinity of the Oued El Gsaïb drainage and also near El Ga’ïdat plateau known as Hmadat Boû Rba’ ine. The largest stones were recovered in the El Ga’ïdat plateau, whereas the smallest one (a few grams) closer to the El Aglâb Mountains. One 47 g crusted stone was documented as being found at 29°28.917’ N, 7°36.674’ W.

Physical characteristics: Several fusion-crusted stones have been collected ranging from 1 to 987 g, with a total weight of around 7 kg. The stones are almost completely coated by glistening black fusion crust, characterized by thicker layers on exterior ridges as well as much glossier regions (above interior olivine macrocrysts). Some stones have thinner secondary fusion crust on some surfaces. The crust on some stones has been broken in places to reveal the interior, which appears overall pale gray in color with larger, very pale yellow olivine macrocrysts, and sporadic small pockets and some very thin veinlets of black glass. No terrestrial weathering is evident.

Petrography: (A. Irving and S. Kuehner, UWS): Olivine macrocrysts (to 1.5 mm) and microphenocrysts (to 0.4 mm) are set in a finer groundmass of patchily zoned pyroxene, plagioclase (maskelynite), Ti-poor chromite, ilmenite, pyrrhotite and minor merrillite. Both the larger olivine macrocrysts and smaller olivine microphenocrysts exhibit thin ferroan rims against the groundmass, and contain tiny chromite inclusions. Narrow ferroan zones also occur within the interior of some olivine macrocrysts.

Geochemistry: Olivine (cores of large macrocrysts Fa19.4-20.2, Fe/Mn=42-44; rims Fa43.2-60.4, Fe/Mn=50-55), cores of microphenocrysts Fa29.1-30.2, Fe/Mn=45-46; rims up to Fa53.3, Fe/Mn=53), orthopyroxene cores (Fs24.0-24.4Wo4.1-4.6, Fe/Mn=30-32), pigeonite (Fs26.1-51.6Wo11.9-16.9, Fe/Mn=31-35), subcalcic augite (Fs21.7-23.3Wo25.0-24.2, Fe/Mn=26-28), plagioclase (An61.1-64.3Or0.5-0.4). Oxygen isotopes (R. Tanaka, OkaU): analyses of acid-washed subsamples by laser fluorination gave, respectively δ17O = 2.849, 2.892; δ18O = 4.844, 4.943; Δ17O = 0.299, 0.290 per mil. Bulk composition (G. Chen and C. Herd, UAb) ICPMS analysis of powdered interior material gave Sm/Nd=0.646, indicating that this specimen has affinities with the depleted compositional group of shergottites.

Classification: Achondrite (Martian, olivine-phyric shergottite).

Specimens: A total of 30.3 g of type material and one polished thin section are on deposit at UWS. Other known institutional specimens include 370 g (ASU), 58 g (UAb), and 108 g (UNM). The remaining material is held by anonymous dealers and collectors.

Date: 18 July 2011
Latitude: 29°28.917’N
Longitude: 7°36.674’W
Mass (g): >7000
Pieces: many
Class: Martian (shergottite)
Shock stage: moderate
Weathering grade: very low
Fayalite (mol%): 19.4-60.4
Ferrosilite (mol%): 24.0-51.6; 21.7-23.3
Wollastonite (mol%): 4.1-16.9; 25.0-24.2
Classifier: A. Irving, S. Kuehner, H. Chennaoui Aoudjehane
Type spec mass (g): 30.3
Type spec location: UWS
Main mass: Anonymous
Comments: Submitted by A. Irving

人民网1月18日电 加拿大研究人员17日最终证实,去年夏天在摩洛哥坠落的陨石系来自火星的“碎片”。这是时隔50年后,火星陨石再度坠落地表。此前,1815年的法国、1865年的印度、1911年的埃及和1962年的尼日利亚曾先后迎来这些火星不速之客,并成为各地大学、研究机构和博物馆高价收购的宠儿。

  尽管去年7月就有人看见了从天而降的“火流星”,但直到去年12月底,人们才在摩洛哥境内发现了这些火星陨石的残骸,总重量大约6.8公斤左右,其中最大一块重约1公斤。阿尔伯塔大学科学家称,当务之急是将这些陨石身上的“地球污染物”清理干净。

  据悉,科学家通过分析陨石的化学成分来判断其“出生地”。由于这些物质中含有构成火星大气层的主要成分,因此其身份得以确定。另外,深黑色的火星陨石一般年龄较小,只有数百万年左右,远远比来自月球和其他星球的陨石“年轻”。

  那么,火星陨石是怎么产生的呢?科学家推测,几百万年前,一颗巨大的小行星与火星表面猛烈相撞,大量火星碎片腾空而起,进入围绕太阳运行的轨道飞行。随着时间推移,一部分陨石闯入了地球大气层。由于极其稀少,火星陨石非常贵重,每盎司售价1-2万加元,大约是目前黄金价格的10倍以上。

23600元台幣

下圖為0.04克

18000元台幣

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12000元台幣(sold)

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12000元台幣(sold)

下圖為0.43克

43700元台幣

下圖為0.03克

11800元台幣

下圖為0.08克

31000元台幣

下圖為0.09克

33000元台幣



 
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品名 :Tissint辉熔长无球粒火星陨石2.1克90%全熔壳
編號 :Tissint-2.1
價格 :NTD 54600
    RMB: 11,143

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