Locality type: | Meteorite Fall Location |
Classification |
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Species: | Chromite |
Formula: | Fe2+Cr23+O4 |
Confirmation |
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Validity: | Believed Valid |
Data |
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Mineral Data: | Click here to view Chromite data |
Locality Data: | Click here to view Tamdakht meteorite, Ghassate Caïdat, Ouarzazate Cercle, Ouarzazate Province, Drâa-Tafilalet Region, Morocco |
Data Identifiers |
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Mindat Occurrence Record ID: | 951993 |
Long-form Identifier: | 1:3:951993:0 |
GUID (UUID V4): | eafbe425-b250-40af-8b16-b081e7f3b9bc |
Nearest other occurrences of Chromite |
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71.2km (44.2 miles) | ⓘTaghouni Mine (Tarouni Mine), Ouisselsate Caïdat, Amerzgane Cercle, Ouarzazate Province, Drâa-Tafilalet Region, Morocco |
72.2km (44.9 miles) | ⓘBou Azzer Vein No. 2, Tansifte Caïdat, Agdz Cercle, Zagora Province, Drâa-Tafilalet Region, Morocco |
72.5km (45.0 miles) | ⓘVein No. 7, Bou Azzer Mine, Ouisselsate Caïdat, Amerzgane Cercle, Ouarzazate Province, Drâa-Tafilalet Region, Morocco |
73.3km (45.6 miles) | ⓘAghbar, Tansifte Caïdat, Agdz Cercle, Zagora Province, Drâa-Tafilalet Region, Morocco |
81.0km (50.3 miles) | ⓘInguijem, Tansifte Caïdat, Agdz Cercle, Zagora Province, Drâa-Tafilalet Region, Morocco |
81.9km (50.9 miles) | ⓘAgoudal Mines, Tansifte Caïdat, Agdz Cercle, Zagora Province, Drâa-Tafilalet Region, Morocco |
82.6km (51.3 miles) | ⓘAgoudal East Mine, Agoudal Mines, Tansifte Caïdat, Agdz Cercle, Zagora Province, Drâa-Tafilalet Region, Morocco |
86.8km (53.9 miles) | ⓘAït Ahmane, Tansifte Caïdat, Agdz Cercle, Zagora Province, Drâa-Tafilalet Region, Morocco |
References |
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Reference Search (possible matching items) |
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| Alexeev, V. A., Gorin, V. D., Ivliev, A. I., Kashkarov, L. L., Ott, U., Sadilenko, D. A., Ustinova, G. K. (2012) Integrated study of the thermoluminescence, noble gases, tracks, and radionuclides in the fresh-fallen Ash Creek L6 and Tamdakht H5 chondrites. Geochemistry International, 50 (2) 105-124 doi:10.1134/s0016702912020024 | Journal (article/letter/editorial) | Radionuclides in the FreshFallen Ash Creek L6 and Tamdakht H5 Chondrites V. A. Alexeev a, V. D. Gorina, A...examined in the freshfallen Ash Creek (L6) and Tamdakht (H5) chon drites. The experimental information...and more and more accurately evaluate them. The Tamdakht H5 and Ash Creek L6 meteorites dis cussed herein...for approximately 70% of the total number of meteorite falls. Material accretion and the origin of the...are most probable within this densely populated region, even more so in the presence of a number of parent | | | Journal (article/letter/editorial) | alteration features and a 11-month record of in situ meteorite and soil temperatures, are used to evaluate the...Kr€ahenb€ uhl 1993) and the efflorescence of salts on meteorite surfaces (e.g., Jull et al. 1988; Velbel 1988;...concentration of 15 samples from the JaH 091 meteorite shower (Gnos et al. 2006) and of 16 individual...the hot desert of Oman during the Omani-Swiss meteorite search project. This study was initiated after...i.e., the hygroscopic behavior of freshly cut meteorite surfaces (Fig. 1). In a relatively humid environment | | | Journal (article/letter/editorial) | FIB sections retrieved from the matrix of each meteorite using a Talos F200X. All observations were conducted... [14] Schrader & Davidson (submitted) GCA. METEORITE MATERIAL MODEL FOR STRUCTURAL PROPERTIES Parul...needed to achieve this objective. At present, the meteorite material found on earth are the only objects from...properties for the entire family of asteroids, meteorite unit models are developed to determine the effective...turn deduce the properties of asteroids. The meteorite unit is a representative volume that accounts | | | Journal (article/letter/editorial) | University, Sapporo, 001-0021, Japan, 3Antarctic Meteorite Research Center, National Institute of Polar Research...to one of the most primitive meteorites. This meteorite contains highly abundance of presolar grains [1]...anticipated [6]. [6] observed that Fe,Ni metal in this meteorite was invariably and extensively altered to form...increasing metamorphism, reaching ~12,000‰ in one meteorite. This enrichment is almost 4 times that in the...orbit of the 3628 Boznemcova asteroid lies in the region affected by two resonances, the Kirkwood gap 3:1 |
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