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53Mn–53Cr and 26Al–26Mg ages of a feldspathic lithology in polymict ureilites
- Source :
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Earth & Planetary Science Letters . Jul2010, Vol. 295 Issue 3/4, p531-540. 10p. - Publication Year :
- 2010
-
Abstract
- Abstract: We report 53Mn–53Cr and 26Al–26Mg isotopic data, obtained by in-situ SIMS analysis, for feldspathic clasts in polymict ureilites DaG 319 and DaG 165. The analyzed clasts belong to the “albitic lithology,” the most abundant population of indigenous feldspathic materials in polymict ureilites, and are highly fractionated igneous assemblages of albitic plagioclase, Fe-rich pyroxenes, phosphates, ilmenite, silica, and Fe(Mn, K, P, Ti)-enriched glass. Glass in DaG 165 clast 19 has extremely high and variable 55Mn/52Cr ratios (500–58,000) and shows correlated 53Cr excesses up to ∼1500‰, clearly indicating the presence of live 53Mn at the time of formation. The slope of the well-correlated isochron defined by glass and pyroxenes from this clast corresponds to (53Mn/55Mn)=(2.84±0.10)×10−6 (2σ). Data for less 55Mn/52Cr-enriched glasses from DaG 319 clast B1, as well as phosphates from several other clasts, are consistent with this isochron. The 53Mn/55Mn ratio obtained from the isochron implies that these clasts are 0.70±0.18Ma younger than the D''Orbigny angrite, corresponding to the absolute age of 4563.72±0.22Ma. Plagioclase in DaG 319 clast B1 has a fairly constant 27Al/24Mg ratio of ∼900 and shows resolvable 26Mg excesses of ∼2‰. The slope of the isochron defined by pyroxene and plagioclase in this clast is (3.0±1.1)×10−7 (2σ), corresponding to a time difference of 5.4 (−0.3/+0.5)Ma after CAI (assuming the canonical initial 26Al/27Al ratio of 5×10−5) and an age 0.5 (−0.3/+0.5)Ma younger than D''Orbigny. Its absolute age (relative to D''Orbigny) is 4563.9 (+0.4/−0.5)Ma, in agreement with the 53Mn–53Cr age from clast 19. These data provide the first high-precision age date, ∼5.4Ma after CAI, for ureilites, giving a minimum estimate for the age of differentiation of their parent asteroid. Interpretation of this age for the thermal and physical history of that asteroid depends on a number of currently unknown or model-dependent parameters, including its size, bulk composition, and oxidation state, and the petrologic relationship between the feldspathic clasts and main group ureilites. [Copyright &y& Elsevier]
Details
- Language :
- English
- ISSN :
- 0012821X
- Volume :
- 295
- Issue :
- 3/4
- Database :
- Academic Search Index
- Journal :
- Earth & Planetary Science Letters
- Publication Type :
- Academic Journal
- Accession number :
- 51437247
- Full Text :
- https://doi.org/10.1016/j.epsl.2010.04.036