2017
DOI: 10.1111/maps.12842
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Petrology, mineralogy, porosity, and cosmic‐ray exposure history of Huaxi ordinary chondrite

Abstract: A meteorite fall was heard and collected on July 13, 2010 at about 18:00 (local time) in the Shibanjing village of the Huaxi district of Guiyang, Guizhou province, China. The total mass of the fall is estimated to be at least 1.6 kg; some fragments are missing. The meteorite consists mainly of olivine, low-Ca pyroxene, high-Ca pyroxene, plagioclase, kamacite, taenite, and troilite. Minor phases include chromite and apatite. Various textural types of chondrules exist in this meteorite: most chondrule textures c… Show more

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Cited by 8 publications
(31 citation statements)
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“…1. We found no systematic influence on the density results from the variable numbers of scans needed to acquire the complete volumes when analyzing sample masses of 30-360 g. The measured densities of fragments from the Tamdakht and Huaxi meteorites are consistent with previous density measurements on smaller fragments, performed by El Abassi et al 2013and Li et al (2017), respectively, which suggest that the bulk density data presented here are accurate. (Consolmagno et al 2008) are outlined next to the legend.…”
Section: Bulk Densitiessupporting
confidence: 88%
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“…1. We found no systematic influence on the density results from the variable numbers of scans needed to acquire the complete volumes when analyzing sample masses of 30-360 g. The measured densities of fragments from the Tamdakht and Huaxi meteorites are consistent with previous density measurements on smaller fragments, performed by El Abassi et al 2013and Li et al (2017), respectively, which suggest that the bulk density data presented here are accurate. (Consolmagno et al 2008) are outlined next to the legend.…”
Section: Bulk Densitiessupporting
confidence: 88%
“…The radionuclide data from Tamdakht are consistent with our measurements and shielding-dependent variations of 60 Co and 26 Al production rates. Huaxi and Kamargaon came from considerably smaller meteoroids according to calculations based on the noble gas contents in Huaxi giving a radius of~11 cm (Li et al 2017) and radionuclide activities in Kamargaon giving r ≤ 10 cm according to Ray et al (2017). While our data are consistent with the estimates for Huaxi, the considerably higher activity of 26 Al in Kamargaon measured by us contradicts the previous size estimate.…”
Section: Pre-atmospheric Sizessupporting
confidence: 63%
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