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Baja California | |||||||||||||||||||||||||||||||
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Basic information | Name: Baja California This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: unknown Country: Mexico Mass: ![]() | ||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 338 approved meteorites classified as Iron, IIIAB. [show all] Search for other: IIIAB irons, Iron meteorites, and Metal-rich meteorites | ||||||||||||||||||||||||||||||
Comments: | Approved 4 Jul 2020 | ||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from MB 109:
Baja California 28°N, 113°W Baja California, Mexico Find: before July 2017 Classification: Iron meteorite (IIIAB) History: (D. Hill, UAz) One meteorite specimen was found by Mr. Aguilar (date unknown) near a ranch 70 km east of Guerrero Negro, Baja California, Mexico, on a rocky mountain (probably near Rancho). Friends of the finder brought an endcut of the meteorite to the U. of Arizona for examination. It was eventually sold to a group of meteorite dealers in 2019. Physical characteristics: Total mass of a single specimen is approximately 10 kg. Dimensions are 30.5 × 16 × 5 cm and tapers on one end. It is irregularly shaped and flat on one side. The meteorite’s unusual shape is defined by a 10 cm cavity where an inclusion melted and ablated away during atmospheric passage. The specimen exhibits an oxidized brown to black-brown, weathered fusion crust with pits up to 7 mm in diameter over the entire surface. There are some whitish and bluish paint spots on the exterior. The meteorite has deep regmaglypts and large rounded regions ranging from a few cm across to 11 cm diameter and 4 cm deep where inclusions probably melted and softened during entry through the atmosphere. Petrography: (D. Hill, UAz) Widmansatten pattern exhibits kamacite with average bandwith of 1.48±0.48 mm; largest bands are 3 mm wide. Kamacite bands are stubby in length; up to 10 mm. Taenite is zoned with plessite interiors, most commonly comb plessite. Schreibersite tends to occur near pinched ends of taenite and as ribbons adjacent to taenite. Sulfides are present as 2 mm grains and complex, fine grained, spider-like regions containing kamacite, pentlandite, and schreibersite with nickel-bearing troilite as 10 μm raisin-like inclusions. Geochemistry: Mineral compositions and geochemistry: (D. Hill, UAz): EMP data, kamacite: Fe = 92.47, Ni = 6.63; taenite: Fe = 63.77 Ni = 35.33 (all in %). Average composition: (N. Chabot, JHUAPL and R. Ash, UMD), LA-ICP-MS data (four laser tracks), Co = 4980±180, Cu = 180±30, Ga = 16.6±0.4, Ge = 37±1, As = 6.4±0.9, Ir = 0.238±0.028, Au = 0.72±0.03 (all in ppm). Distance, physical characteristics, and composition preclude pairing with Loreto (IIIAB), Mexico. Classification: Iron, IIIAB. Coarse octahedrite. Specimens: Type specimen: 311 g UAz | ||||||||||||||||||||||||||||||
Data from: MB109 Table 0 Line 0: |
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Institutions and collections |
UAz: Lunar and Planetary Laboratory, University of Arizona, 1629 E. University Blvd., Tucson, AZ 85721, United States (institutional address; updated 14 Jan 2012) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 109, in preparation (2020)
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Geography:![]() |
Statistics: This is 1 of 4 approved meteorites from Baja California, Mexico This is 1 of 113 approved meteorites from Mexico (plus 4 unapproved names) (plus 1 impact crater) | ||||||||||||||||||||||||||||||
Proximity search: |