NWA 11562: A Unique Ureilite with Extreme Mg-rich Constituents

Abstract A comprehensive study of an ungrouped achondrite meteorite, North West Africa (NWA) 11562, was conducted, involving petrology, mineralogy, and mass-independent chromium isotopic composition. NWA 11562 comprises 34.9 vol% olivine, 56.1 vol% pyroxenes, 6.7 vol% Fe–Ni metal and oxides, 2.2 vol% carbon, and 0.2 vol% anhydrite. The oxygen isotopic composition ( δ 18 O = 6.24‰ ± 0.13‰ and Δ 17 O = −1.81‰ ± 0.03‰; Meteoritical Bulletin Database) and chromium isotopic compositions ( ε 54 Cr = −0.82 ± 0.10, 2SE) are consistent with NWA 11562 being a ureilite, and petrographic observations show features similar to those of the common ureilite group meteorites. Olivine (core: Fo 99.0 ± 0.1; rim: Fo 98.9 ± 0.1 ) and pyroxene (orthopyroxene: Mg# 99.0 ± 0.2; clinopyroxene: Mg# 99.1 ± 0.7) core compositions are more magnesian than in any previously known ureilite and lack the characteristic reduction rims of ureilites. Rounded small olivine grains within NWA 11562 indicate that the meteorite experienced impact and associated melting. Combined with the characteristic Fe/Mn ratio (3.84 ± 0.16) and Mg# (99.0 ± 0.1) of olivine cores, we suggest that NWA 11562 represents a more Mg-rich ureilite than any previously reported. NWA 11562 has a high 55 Mn/ 52 Cr ratio, and when combined with literature data, it plots on a well-defined 53 Mn– 53 Cr isochron, providing a more accurate age, i.e., 4566.7 ± 0.8 Ma, overlapping previous work. This age may represent the result of early partial melting of the ureilite parent body.

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Publication Details

Journal
The Planetary Science Journal
Published
2024-08-01
DOI
https://doi.org/10.3847/psj/ad6154
Citations
1
Primary Topic
High-pressure geophysics and materials
Type
article
Field-Weighted Citation Impact
0.53

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article

NWA 11562: A Unique Ureilite with Extreme Mg-rich Constituents

Mingbao Li, Yan Fan, P. M. Ranjith, Chao Wang et al.
1 citations
The Planetary Science Journal
High-pressure geophysics and materials
0.53
article

NWA 11562: A Unique Ureilite with Extreme Mg-rich Constituents

Mingbao Li, Yan Fan, P. M. Ranjith, Chao Wang, Shijie Li, Ke Zhu, Wen Yu
article en
1 citations

Abstract

Abstract A comprehensive study of an ungrouped achondrite meteorite, North West Africa (NWA) 11562, was conducted, involving petrology, mineralogy, and mass-independent chromium isotopic composition. NWA 11562 comprises 34.9 vol% olivine, 56.1 vol% pyroxenes, 6.7 vol% Fe–Ni metal and oxides, 2.2 vol% carbon, and 0.2 vol% anhydrite. The oxygen isotopic composition ( δ 18 O = 6.24‰ ± 0.13‰ and Δ 17 O = −1.81‰ ± 0.03‰; Meteoritical Bulletin Database) and chromium isotopic compositions ( ε 54 Cr = −0.82 ± 0.10, 2SE) are consistent with NWA 11562 being a ureilite, and petrographic observations show features similar to those of the common ureilite group meteorites. Olivine (core: Fo 99.0 ± 0.1; rim: Fo 98.9 ± 0.1 ) and pyroxene (orthopyroxene: Mg# 99.0 ± 0.2; clinopyroxene: Mg# 99.1 ± 0.7) core compositions are more magnesian than in any previously known ureilite and lack the characteristic reduction rims of ureilites. Rounded small olivine grains within NWA 11562 indicate that the meteorite experienced impact and associated melting. Combined with the characteristic Fe/Mn ratio (3.84 ± 0.16) and Mg# (99.0 ± 0.1) of olivine cores, we suggest that NWA 11562 represents a more Mg-rich ureilite than any previously reported. NWA 11562 has a high 55 Mn/ 52 Cr ratio, and when combined with literature data, it plots on a well-defined 53 Mn– 53 Cr isochron, providing a more accurate age, i.e., 4566.7 ± 0.8 Ma, overlapping previous work. This age may represent the result of early partial melting of the ureilite parent body.

The Planetary Science JournalVol. 5(8)
Japan Society for the Promotion of Science London, National Natural Science Foundation of China
Life below water
Openalex Percentile: Top 35%
High-pressure geophysics and materials
0.53
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NWA 11562: A Unique Ureilite with Extreme Mg-rich Constituents — Mingbao Li, Yan Fan, et al. · The Planetary Science Journal (2024) | TGRS Research Map | TGRS