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Cosmic ray exposure and pre‐atmospheric size of the Gebel Kamil iron meteorite
Author(s) -
Ott U.,
Merchel S.,
Herrmann S.,
Pavetich S.,
Rugel G.,
Faestermann T.,
Fimiani L.,
GomezGuzman J. M.,
Hain K.,
Korschinek G.,
Ludwig P.,
D'Orazio M.,
Folco L.
Publication year - 2014
Publication title -
meteoritics and planetary science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.09
H-Index - 100
eISSN - 1945-5100
pISSN - 1086-9379
DOI - 10.1111/maps.12334
Subject(s) - meteorite , impact crater , meteoroid , accelerator mass spectrometry , radionuclide , atmosphere (unit) , cosmogenic nuclide , iron meteorite , cosmic ray , geology , radius , noble gas , astrobiology , radiocarbon dating , astronomy , physics , meteorology , nuclear physics , paleontology , computer security , computer science , quantum mechanics
Abstract Cosmogenic He, Ne, and Ar as well as the radionuclides 10 Be, 26 Al, 36 Cl, 41 Ca, 53 Mn, and 60 Fe have been determined on samples from the Gebel Kamil ungrouped Ni‐rich iron meteorite by noble gas mass spectrometry and accelerator mass spectrometry ( AMS ), respectively. The meteorite is associated with the Kamil crater in southern Egypt, which is about 45 m in diameter. Samples originate from an individual large fragment (“Individual”) as well as from shrapnel. Concentrations of all cosmogenic nuclides—stable and radioactive—are lower by a factor 3–4 in the shrapnel samples than in the Individual. Assuming negligible 36 Cl decay during terrestrial residence (indicated by the young crater age <5000 years; Folco et al. [Folco L., 2011]), data are consistent with a simple exposure history and a 36 Cl‐ 36 Ar cosmic ray exposure age ( CRE ) of approximately (366 ± 18) Ma (systematic errors not included). Both noble gases and radionuclides point to a pre‐atmospheric radius >85 cm, i.e., a pre‐atmospheric mass >20 tons, with a preferred radius of 115–120 cm (50–60 tons). The analyzed samples came from a depth of approximately 20 cm (Individual) and approximately 50–80 cm (shrapnel). The size of the Gebel Kamil meteoroid determined in this work is close to estimates based on impact cratering models combined with expectations for ablation during passage through the atmosphere (Folco et al. [Folco L., 2010], [Folco L., 2011]).