Crystallization Temperatures of Komatiitic Basalts from the Vetrenyi Belt, Karelia Based on the Alumina Partition between Olivine and Chromite

IF 0.7 4区 地球科学 Q4 GEOSCIENCES, MULTIDISCIPLINARY
E. V. Asafov, A. N. Koshlyakova, A. V. Sobolev, D. P. Tobelko, N. N. Koshlyakova, S. V. Mezhelovskaya
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Abstract

The Archean–Proterozoic transition in the Earth’s history is marked by significant changes in the mantle dynamics and temperature regimes. A notable consequence is the disappearance of Al-depleted komatiites in the Late Archean and an almost complete absence of Archean-typical peridotitic komatiites since the Proterozoic. This work presents a study of the 2.41 Ga komatiitic basalts from the Vetrenyi Belt, dating back to the early Proterozoic. Unique data on the compositions of olivine and chromite, as well as on the crystallization temperatures based on Al-in-olivine geothermometry for komatiitic basalts from the Vetrenyi Belt are provided. The temperatures of the earliest stages of crystallization were approximately 1240 ± 25°C, which indicates the occurrence of water in the melt and is consistent with measured water contents of 0.4 ± 0.2 wt % H2O in the melt inclusions. However, during crystallization, the komatiitic basalt melt underwent degassing, resulting in mass crystallization of the system and a temperature rise by ~20°C due to the release of the latent heat of crystallization. The degassing of water from the melt suggests crystallization under surface conditions.

Abstract Image

基于橄榄石和铬铁矿之间的氧化铝分区的卡累利阿 Vetrenyi 地带科马蒂蒂玄武岩的结晶温度
摘要地球历史上阿新世-原生代的转变以地幔动力学和温度机制的重大变化为标志。一个显著的后果是晚阿新世贫铝岩的消失,以及自新生代以来几乎完全没有阿新世典型的橄榄岩。本研究对来自 Vetrenyi 带的 2.41 Ga 柯麦饭石玄武岩进行了研究,其年代可追溯到早新生代。该研究提供了关于橄榄石和铬铁矿成分的独特数据,以及基于 Al-in-olivine 测地热法得出的 Vetrenyi 带 komatiitic 玄武岩的结晶温度。结晶最早阶段的温度约为 1240 ± 25°C,这表明熔体中含有水,并与测得的熔体包裹体中 0.4 ± 0.2 wt % H2O 的含水量相符。然而,在结晶过程中,柯马蒂式玄武岩熔体发生了脱气,导致系统大量结晶,并由于结晶潜热的释放而使温度上升了约 20°C。熔体中水的脱气表明结晶是在地表条件下进行的。
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来源期刊
Doklady Earth Sciences
Doklady Earth Sciences 地学-地球科学综合
CiteScore
1.40
自引率
22.20%
发文量
138
审稿时长
3-6 weeks
期刊介绍: Doklady Earth Sciences is a journal that publishes new research in Earth science of great significance. Initially the journal was a forum of the Russian Academy of Science and published only best contributions from Russia. Now the journal welcomes submissions from any country in the English or Russian language. Every manuscript must be recommended by Russian or foreign members of the Russian Academy of Sciences.
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