Understanding the Spreading and Formation of Oceanic Plates by Drilling in the Upper Crust off Hawaii

IF 0.2 Q4 GEOGRAPHY, PHYSICAL
S. Umino, Y. Kusano
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引用次数: 2

Abstract

The style of crustal extension is governed by M, which is the ratio of magma consumed to relax the crustal strain caused by plate spreading. Bathymetric profiles across ridges are repro-duced well by changing M . However, what determines the value of M has not been explained. Fast-spread oceanic crust comprises dense sheet flows underlain by thin dense sheeted dikes compared to magmas. This density structure increases the magma extruded, allowing the crust to be extended solely by magmatic accretion; whereas, the intermediate-spread crust consists of less dense pillow lavas, yielding an apparent level of neutral buoyancy that traps magma to develop the sheeted dikes below. Consequently, the crust extends through dike intrusions in the lower levels and faults at shallow levels. Thus, the density structure of the oceanic crust determines the style of plate spreading, or the value of M . Because the spreading rate or the strain rate does not vary within the same ridge segment, intrasegment variations in crustal structure depend directly on the supply rate of magma, or the value of M , which decreases with the thin-ning of extrusive layers and the thickening of sheeted dikes along the Galapagos Spreading Center and the East Pacific Rise. This tendency is supported by the crustal architecture observed in holes 504B and 1256D, the Hess Deep and the Oman Ophiolite. The density structure of the upper crust can be discerned by the proportion of sheet flows among extrusive rocks on the ridge axis, which is drastically reduced with spreading rates from 10 cm/a to 7 cm/a. This spreading rate interval coincides with the change in axial magma chamber depth. Throughout this rate interval, the key observation is whether the style of crustal extension from magmatic accre-tion-dominant details ) . Sediments and lavas emplaced off ridge ( uppermost basement 100 m in Hole 1256D ( Umino et al ., 2008a ) and 50 m in Hole 504B ( Ayadi et al ., 1998 ) , respectively ) are excluded from density estimates. The 1256D crust on the East Pacific Rise spread at an ultrafast rate of 22 cm/a comprises high-density sheet flows, yielding almost the same lithostatic and magmastatic pressures. The 504B crust on the Costa Rica Rift spread at an intermedi-ate rate of 6.6 cm/a has an apparent level of neutral buoyancy ( LNB ) , where lithostatic pressure is lower than magmastatic pressure. Magma uprising from the axial magma chamber ( AMC ) is preferentially trapped in the LNB and forms the
通过在夏威夷外的上地壳钻探了解大洋板块的扩展和形成
地壳伸展的类型受M的支配,M是由板块扩张引起的地壳应变松弛所消耗的岩浆比例。通过改变M值,可以很好地再现脊上的水深剖面。然而,是什么决定了M的值还没有解释。与岩浆相比,快速扩张的海洋地壳由密集的片状流组成,下面是薄而密集的片状岩脉。这种密度结构增加了岩浆的挤压,使得地壳仅通过岩浆吸积而扩张;然而,中间伸展的地壳由密度较低的枕状熔岩组成,产生明显的中性浮力,使岩浆被困住,形成下面的片状岩脉。因此,地壳在较低层次上通过岩脉侵入,在较浅层次上通过断层伸展。因此,洋壳的密度结构决定了板块扩张的方式,即M值。由于在同一脊段内扩张速率或应变速率不变化,因此地壳结构的分段内变化直接取决于岩浆的供应速率或M值,M值随着沿加拉帕戈斯扩张中心和东太平洋隆起的挤压层变薄和片状岩脉变厚而减小。504B和1256D孔、赫斯深和阿曼蛇绿岩观测到的地壳结构支持了这一趋势。上地壳的密度结构可以通过在脊轴上的挤压岩石间的片流比例来识别,随着扩展速率从10 cm/a急剧减少到7 cm/a。这一扩张速率区间与岩浆库轴向深度变化一致。在整个速率区间内,关键的观察是地壳伸展的样式是否来自岩浆增生(以细节为主)。在密度估算中不包括山脊外的沉积物和熔岩(1256D洞最上层基底100 m (Umino et al ., 2008a)和504B洞50 m (Ayadi et al ., 1998))。东太平洋隆起1256D地壳以22 cm/a的超快速度扩张,包括高密度的片流,产生几乎相同的静岩和岩浆压力。哥斯达黎加裂谷504B地壳以6.6 cm/a的中等速率扩张,具有明显的中性浮力(LNB)水平,其中静岩压力低于岩浆压力。从轴向岩浆房(AMC)升起的岩浆优先被困在LNB中,并形成了地幔
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来源期刊
CiteScore
1.50
自引率
33.30%
发文量
28
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