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Balambala | |||||||||||||||||||||||||||||
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Basic information | Name: Balambala This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2018 Country: Kenya Mass: 60.5 kg | ||||||||||||||||||||||||||||
Classification history: |
This is 1 of 8 approved meteorites classified as Iron, IIF. [show all] Search for other: IIF irons, Iron meteorites, and Metal-rich meteorites | ||||||||||||||||||||||||||||
Comments: | Approved 2 Aug 2020 | ||||||||||||||||||||||||||||
Writeup |
Writeup from MB 109:
Balambala 0°3.555’N, 39°6.45’E North-Eastern, Kenya Find: 2018 Jan Classification: Iron meteorite (IIF) History: Dhagax Bir is the name attributed to the meteorite by the region’s goat herders; the name means metal stone in the local spoken Somali dialect. According to the local residents the meteorite was in this location for as long as anyone could remember, including a woman 60 years of age who regularly herded goats past this stone since she was 10 years old. In January 2018, a nomad identified the stone as an iron meteorite, and then brought it to a local broker in the nearest city of Garissa. The broker began circulating photos and it was subsequently purchased by Mahamed Nur Ogle and John Higgins. Physical characteristics: The single, approximately shield-shaped mass is about 33 × 41 cm in width and 10-15 cm thick. It is covered in large (~5 cm-wide) regmaglypts; a few cm-sized spherical holes are also present on one side. Some rust is present on the top surface, but otherwise, there is little evidence of oxidation. Petrography: (C. Herd and L. Tunney, UAb) Optical investigation of a 4.5 × 6 cm polished and etched end slice reveals cm-scale rounded troilite inclusions, and lath-like (~1 × 8 mm) schreibersite inclusions, both swathed in kamacite. The bulk of the meteorite consists of kamacite spindles in a matrix of taenite. The spindles occur evenly throughout, except for adjacent to inclusions, where ~500 μm-wide spindle-poor regions are surrounded by ~200 μm-wide spindle-rich rings that broadly parallel the outlines of the inclusions. SEM investigation reveals that larger kamacite spindles or groupings of spindles are often cored by 50-100 μm subequant schreibersite crystals. The average kamacite bandwidth is 53±17 μm (n=36). Taenite is zoned to higher Ni adjacent to kamacite spindles. No alteration was observed. Geochemistry: (C. Herd, L. Tunney, and G. Chen, UAb) ICP-MS data, using sample of North Chile (Filomena) as standard: Ni = 13.0, Co = 0.67 (both wt%); Ir = 5.2, Ge = 223, Ga = 8.1, As = 20.6, W = 0.76, Re = 0.45, Pt = 14.9, Cu = 208, Au = 2.6 (all µg/g). Classification: Iron, IIF, based on the high Ge/Ga ratio, high Co content, and fit with regression parameters established by Kracher et al. (1980). Specimens: Type specimen of 261 g at UAb. Main mass with Mahamed Nur Ogle and J. Higgins. | ||||||||||||||||||||||||||||
Data from: MB109 Table 0 Line 0: |
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Institutions and collections |
UAb: 1-26 Earth Sciences Building, University of Alberta, Edmonton, AB, T6G 2E3, Canada, Canada; Website (institutional address; updated 17 Oct 2011) |
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Catalogs: |
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References: | Published in Gattacceca J., McCubbin F. M., Grossman J., Bouvier A., Bullock E., Chennaoui Aoudjehane H., Debaille V., D’Orazio M., Komatsu M., Miao B. and Schrader D. L. (2021) The Meteoritical Bulletin, No. 109. Meteoritics & Planetary Science 56, 1626–1630.
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Geography: |
Statistics: This is 1 of 5 approved meteorites from North-Eastern, Kenya This is 1 of 14 approved meteorites from Kenya (plus 1 unapproved name) | ||||||||||||||||||||||||||||
Proximity search: |