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Junction City | |||||||||||||||||||||||||||||||||||
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Basic information | Name: Junction City This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: Yes, confirmed fall Year fell: 2022 Country: United States Mass: 1951 g | ||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 8974 approved meteorites (plus 5 unapproved names) classified as L5. [show all] Search for other: L chondrites, L chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7) | ||||||||||||||||||||||||||||||||||
Comments: | Approved 5 Sep 2024 | ||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 113:
Junction City 32°38.2482’ N, 84°24.9576’ W Georgia, United States Confirmed fall: 2022 Sept 26 Classification: Ordinary chondrite (L5) History: (P. Branch, M. Hankey) At 00.04 local time on 26 September 2022 (0404 UTC), a bright fireball traveling from the S to N detonated above southern Georgia between Atlanta and Columbus. This fireball was widely seen across the southeastern US with 66 reports to the American Meteor Society (event #6491-2022). Two cameras from the AMS ALLSKY7 Network operated by Ed Albin captured the fireball. ALLSKY7 Network camera operator Pat Branch placed the fall around Buckner Crossroads 4 km NE of Junction City, Talbot County, Georgia. Mr. Branch, Mr. Albin, and fellow hunter Carl Dietrich headed to the fall zone. Mr. Branch found the first stone 29 hours after the fall in the middle of Charles Buckner Rd, ~5.5 km NE of Junction City. A 91 g fusion-crusted fragment was sitting in an indentation in the road and surrounded by 79 g of fragments. Over the next few days, Ed Albin, Carl Dietrich, Ari Machiz, Illiana Machiz, Lance Schrumpf, Dave Lacco, Roberto Vargas, Mark Lyon, Sean Keeton, Rob Keeton, Matthew Stream, Michael Kelly, Ray Borges, Mike Buckner, and Derik Bowers found 582.8 g of fragments associated with the first find, for a total of 752.8 g in and around the same area. Eight more stones were subsequently found (see Geography section). All were found on or near the roads. The stones defined an ~7 × 1.4 km strewnfield trending SE to NW. Physical characteristics: The stones are blocky with broad regmaglypts. Fusion crust is matte to glossy. Interior of the stones are bright white, lacking shock veins, and crumbly. Petrography: (L. Garvie, ASU) A 2.4 g fragment was taken from the 159 g stone and prepared as a 1" round polished mount. Optical and scanning electron microscopy show an abundance of chondrules, chondrule fragments, and mineral grains interspersed with metals and troilite. Many chondrules show sharp boundaries with the surrounding minerals. Chondrules up to 1.2 mm, dominated by PO and BO with a mean diameter of 550 microns (n=18). One BO chondrule is mantled by a thick igneous rim of polycrystalline olivine. Feldspar outside of the chondrules shows a range of sizes, some grains to 70 μm though the majority <25 μm. Kamacite to 500 μm, anhedral, some with holly-leaf-shaped margins. The kamacite is dominantly single crystal with curvy to linear Neumann bands that often exhibit a pinched profile. Taenite/tetrataenite to 350 µm and tends to be more equant than the kamacite. Etched taenite/tetrataenite commonly exhibit dark plessitic cores. Troilite is anhedral, to 400 µm, single crystal and lacking shock lamellae. Elemental copper is rare occurring as ~20-µm-sized grains associated with troilite/taenite. Accessory minerals include chromite to 300 μm and abundant scattered Ca-Cl and Ca-Na-Mg phosphates to 0.5 mm. Geochemistry: (L. Garvie, ASU) Olivine Fa24.88±0.39, range Fa24.05-25.75, mean Cr2O3=0.03 wt%, FeO/MnO=48.07±2.44, n=19. Low Ca-pyroxene Fs21.04±0.13Wo1.61±0.29, mean Cr2O3=0.10 wt%, TiO2=0.15 wt%, and Al2O3=0.13 wt%, FeO/MnO=28.59±1.66, n=14. High Ca-pyroxene (one grain) Fa8.25Wo44.34, Cr2O3=0.76 wt%, TiO2=0.43 wt%, and Al2O3=0.149 wt%, FeO/MnO=32.82. Classification: Ordinary chondrite, L5, S2, W0. Specimens: 20.8 g at ASU | ||||||||||||||||||||||||||||||||||
Data from: MB113 Table 0 Line 0: |
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Institutions and collections |
ASU: Center for Meteorite Studies, Arizona State University, Tempe, Arizona 85287-1404, United States; Website (institutional address; updated 14 Jan 2012) AMS: Australian Museum, 6 College Street, Sydney, NSW 2010, Australia (institutional address; updated 18 Oct 2011) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 113, in preparation (2024)
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Photos: |
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Geography: |
Strewnfield: Click here to view 24 members Statistics: This is 1 of 27 approved meteorites from Georgia, United States This is 1 of 1934 approved meteorites from United States (plus 866 unapproved names) (plus 28 impact craters) | ||||||||||||||||||||||||||||||||||
Proximity search: |