EVIDENCE for LATE FORMATION and YOUNG METAMORPHISM in the ACHONDRITE NAKHLA

被引:33
作者
Papanastassiou, D. A. [1 ]
Wasserburc, G. J. [1 ]
机构
[1] CALTECH, Div Geol & Planetary Sci, Lunatic Asylum Charles Arms Lab, Pasadena, CA 91109 USA
基金
美国国家科学基金会;
关键词
URANIUM;
D O I
10.1029/GL001i001p00023
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We have determined an age T=1.37 AE for Nakhla and an initial Sr-87/Sr-86, I = 0.7023. A rather thorough Sr equilibration took place at this time between all the phases of this meteorite, but there is clear evidence of somewhat incomplete isotopic equilibrium during the 1.37 AE event, which is not consistent with the derivation of Nakhla from a magma at this time. Nakhla has a young model age of 3.6-2.9 AE which requires that gross differentiation processes for its parent body occur between 3.6 and 1.37 AE, significantly later than 4.6 AE. The most reasonable model is that Nakhla formed as an igneous rock at similar to 3 AE and was metamorphosed at 1.37 AE. Several similarities exist between the Nakhla parent planet and the Earth and indicate the existence of other objects with close terrestrial chemical affinities.
引用
收藏
页码:23 / 26
页数:4
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