日本地球惑星科学連合2018年大会

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[EE] 口頭発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG54] ハードロック掘削 オマーンから海洋リソスフェア,島弧形成+

2018年5月21日(月) 13:45 〜 15:15 A09 (東京ベイ幕張ホール)

コンビーナ:高澤 栄一(新潟大学理学部地質科学科)、道林 克禎(名古屋大学大学院環境学研究科地球環境科学専攻地質・地球生物学講座岩石鉱物学研究室)、Peter B Kelemen (共同)、Damon A H Teagle (Ocean & Earth Science, National Oceanography Centre Southampton, University of Southampton, SO14-3ZH, Southampton, UK)、座長:Kelemen Peter(Columbia University)、森下 知晃(金沢大学)

14:45 〜 15:00

[SCG54-10] Initial studies of the petrophysics in the dike and upper gabbro from ICDP Hole GT3A, the Oman Drilling Project Phase I

*阿部 なつ江1畠山 航平2岡崎 啓史3Leong James4立石 大和5Ildefonse Benoit6Harris Michelle7道林 克禎8de Obeso Juan Carlos9ティーグル デーモン10高澤 栄一11ケレメン ピーター12The Oman Drilling Project Phase I Science Party13 (1.国立研究開発法人海洋研究開発機構海洋掘削科学研究開発センター、2.広島大学、3.国立研究開発法人海洋研究開発機構高知コア研究所、4.Arizona State University、5.岡山大学、6.Université de Montpellier、7.Plymouth University、8.静岡大学、9.Lamont -Doherty Earth ObservatoryColumbia University、10.University of Southampton, Ocean & Earth Science, National Oceanography Centre Southampton、11.新潟大学、12.Columbia University、13.University of Southampton, Oman Drilling Project Office)

キーワード:ICDP オマーン掘削、海洋地殻、岩石物性、緑簾石、地球深部探査船「ちきゅう」

We report results on the physical property measurements of the core samples from Oman Drilling Project Hole GT3A (23.11409 N, 58.21172 E) in the Samail Ophiolite, Sultanate of Oman. Cores are mainly composed of basalt and diabase, followed by gabbros (gabbro, olivine gabbro and oxide gabbro), with minor felsic, trondhjemite and tonalite, dikes intruded into the mafic rocks. Shipboard measurements of physical properties were undertaken to characterize recovered core material. During Leg 2 of ChikyuOman expedition (Aug-Sept 2017), whole-round X-ray CT images, natural gamma radiation (NGR), magnetic susceptibility (MS), P-wave velocity (Vp) and electrical resistivity, and half-round point magnetic susceptibility and color spectroscopy were measured for all sections of cores on board. P-wave velocity, bulk/grain density and porosity of discrete cube samples and thermal conductivity on pieces from the working halves of the split core sections were also measured.
Mafic rocks from the Hole GT3A are altered in the various extensions[DAT1] . Compared to the gabbros from the Hole GT1A and GT2A of the Oman Drilling Project, which were described and measured during Leg 1 of ChikyuOman2017 expedition, GT3A cores show much wider range of physical properties. For example, P-wave velocity of the samples from GT3A show a range from 2.2 to 7.1 km/s. There is a clear negative correlation between P-wave velocity and porosity[DAT2] . It is noteworthy that there is a positive correlation between the densities [DAT3] and porosity in more than 1/4 of the samples. Highly altered samples from the GT3A cores show high porosity (up to 12%) and high both bulk and grain densities (up to 3.2 and 3.4 g/cm^3, respectively). It is probably because that the larger volume of epidote with high density (3.39 – 3.48 g/cm^3) in the more altered samples. The color spectrums, especially yellowness of the core samples, clearly have correlations with the rock physics of the GT3A samples (Fig.1). The yellowness of the mafic rocks in the GT3A imply their degree of alteration reflected the mode of epidote. In other words, the epidote precipitation during the hydrothermal alteration reduces the volume of a part of oceanic crust and probably causes the higher porosity as previously proposed on a qualitative basis (Harper et al JGR 1988; Bettison-Varga et al. Geology 1992; Harper GSA Spec Papers 1995; Cann et al., Geofuid 2015).