|
Sierra Gorda 012 | |||||||||||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Basic information | Name: Sierra Gorda 012 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2018 Country: Chile Mass: 1100 g | ||||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 6493 approved meteorites (plus 2 unapproved names) classified as H4. [show all] Search for other: H chondrites, H chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7) | ||||||||||||||||||||||||||||||||||||||
Comments: | Approved 15 May 2019 | ||||||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 108:
Sierra Gorda 012 22°30.198’S, 69°08.703’W Antofagasta, Chile Find: 2018 Apr 6 Classification: Ordinary chondrite (H4) History: The meteorite was found on 6 April 2018 by Ilya Chaplygin during an expedition organized by Timur Kryachko. Physical characteristics: The meteorite is covered by a thin film of weathered material. Fusion crust has been totally sand-blasted. The interior of the meteorite is gray to dark brown whereas the surface is dark brown. Petrography: (Pavel Yu. Plechov, FMMR) Petrographic observation of a polished section shows chondrules with clear borders. Chondrules size up to 1200 µm. Porphyric olivine and olivine-pyroxene chondrules as well as nonporphyric pyroxene and barred olivine chondrules are present. POP chondrules consist of large homogeneous Ol crystals whereas Low-Ca Px occupies peripheral parts. Low-Ca Px often has clear zoning from very high-Mg relict parts (Fs1.8) to more ferrous rims (Fs14.8) in these chondrules. Matrix consists of tiny olivine and low-Ca pyroxene grains (near 1 µm) with Fe-Ni metal and troilite. Metal consists of kamacite and taenite (with 23-34 wt% Ni). Very rare Plagioclase grains (An1.9-3.5) are about 1 µm and only few are up to 3-5 µm. These features indicate a petrological type of 4 for the meteorite. Olivine shows no undulatory extinction. No shock veins or melt were found. Weathering products (goethite, "hydrogoethite") occur as veins and in situ alteration of FeNi metal. Geochemistry: Mineral composition and Geochemistry: EDS-WDS analyses (Pavel Yu. Plechov, FMMR). Olivine Fa15.8±1.2 (N=48), orthopyroxene Fs11.2±3.1Wo0.8±0.6 (N=24), plagioclase Ab91.7An2.6Or5.1 (N=5), Cr-bearing clinopyroxene En49.9Fs15.4Wo34.2 (N=5), chromite Crt76.8Spl5.5 (N=6). Phosphates are both Cl-apatite and merrillite. Composition of kamacite (in wt%, N=5): Fe 92.4, Ni 7.1, Co 0.56 (measured by WDS). Taenite (N=3): 27.1 wt% Ni, 0.26 wt% Co. Troilite is close to ideal FeS. Classification: Ordinary chondrite (H4). Specimens: Ilya Chaplygin holds main mass. 61 g and thin section, FMMR. | ||||||||||||||||||||||||||||||||||||||
Data from: MB108 Table 0 Line 0: |
|
||||||||||||||||||||||||||||||||||||||
Institutions and collections |
FMMR: Fersman Mineralogical Museum, Leninskiy prospekt 18 korpus 2, Moscow, Russia, 119071, Russia; Website (institutional address; updated 24 Feb 2018) |
||||||||||||||||||||||||||||||||||||||
Catalogs: |
| ||||||||||||||||||||||||||||||||||||||
References: | Published in Meteoritical Bulletin, no. 108 (2020) Meteorit. Planet. Sci. 55, 1146-1150
| ||||||||||||||||||||||||||||||||||||||
Photos: |
| ||||||||||||||||||||||||||||||||||||||
Geography: |
Statistics: This is 1 of 3442 approved meteorites from Antofagasta, Chile (plus 12 unapproved names) (plus 1 impact crater) This is 1 of 3471 approved meteorites from Chile (plus 13 unapproved names) (plus 1 impact crater) | ||||||||||||||||||||||||||||||||||||||
Proximity search: | |||||||||||||||||||||||||||||||||||||||
Also see: |
This lists the most popular meteorites among people who looked up this meteorite.
| ||||||||||||||||||||||||||||||||||||||
Revision history: |
This lists important revisions made to data for this record.
|