基于方解石同位素比值的日本西南四国岛满杂岩发震增生体流体来源

Natsuki Uchida, M. Murayama, Y. Matsubara, A. Sakaguchi
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引用次数: 0

摘要

四国岛东增生杂岩是在发震深度出土的,含有大量方解石脉。研究这些脉可以更好地了解俯冲带深部各种流体的来源。例如,流体来源可以从方解石的同位素比例和沉积温度的比较中推断出来。本文对横河杂岩及其围岩74个方解石脉样品进行了δδ 18 O VPDB和δδ 13 C VPDB测量,这些方解石脉的峰值温度为140℃~ 250℃,与南开俯冲带的发震热条件相当。研究结果表明,方解石的同位素比值与寄主岩石的古温度有关。方解石的最低δδ 13 C VPDB值与寄主岩石的古温度有关。古温度值越高,方解石样品的δδ 13 C VPDB值越低。这表明裂缝封闭脉体在不同阶段起着流体流动的管道作用,且区域内δδ 13c VPDB值最低的方解石样品沉积在温度峰值阶段。方解石的流体来源可由δδ 18o SMOW值和沉积温度推断。方解石脉可能是由变质流体沉积而成。这意味着原位流体在吸积棱镜的主体内流动,不受来自板块边界断层浅部或深部的外来流体的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Fluid source of seismogenic accretionary body based on calcite isotope ratio, Shimanto complex, Shikoku, southwest Japan
The Shimanto accretionary complex in Shikoku, which was ex-humed from seismogenic depths, contains many calcite veins. These veins may be studied to better understand the origin of various fluids in the deep sections of a subduction zone. For example, fluid sources may be inferred from comparison of the isotopic ratio of the calcite and its depositional temperature. This study obtained δδ 18 O VPDB and δδ 13 C VPDB measurements from 74 samples of calcite veins in the Yokonami Melange and surrounding rocks, which had been exposed to peak temperatures of 140 ° C to 250 ° C, comparable to seismogenic thermal conditions in the Nankai subduction zone. The study results show that the isotopic ratio of calcite is related to the paleo-temperature of the host rock. The lowest δδ 13 C VPDB value for calcite from several measurements obtained for a single location is dependent on the paleo-temperature of the host rock. In addition, the calcite samples from the higher paleo-temperature areas have the lowest δδ 13 C VPDB values. This suggests that crack-seal veins acted as conduits for fluid flow at various stages, and calcite samples with the lowest δδ 13 C VPDB values in an area were deposited during the peak tem-perature stage. The fluid source of calcite may be inferred from δδ 18 O SMOW values and depositional temperature. It is revealed that the calcite veins might be deposited from metamorphic fluid. This im-plies that in-situ fluid flows within the main body of the accretionary prism, free of exotic fluid from shallow or deep sections along the plate boundary fault.
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