Shervais John W, Reagan Mark, Haugen Emily, Almeev Renat R, Pearce Julian A, Prytulak Julie, Ryan Jeffrey G, Whattam Scott A, Godard Marguerite, Chapman Timothy, Li Hongyan, Kurz Walter, Nelson Wendy R, Heaton Daniel, Kirchenbaur Maria, Shimizu Kenji, Sakuyama Tetsuya, Li Yibing, Vetter Scott K
Department of Geology Utah State University Logan UT USA.
Department of Earth and Environmental Science University of Iowa Iowa City IA USA.
Geochem Geophys Geosyst. 2019 Jan;20(1):314-338. doi: 10.1029/2018GC007731. Epub 2019 Jan 16.
The Izu-Bonin-Mariana (IBM) fore arc preserves igneous rock assemblages that formed during subduction initiation circa 52 Ma. International Ocean Discovery Program (IODP) Expedition 352 cored four sites in the fore arc near the Ogasawara Plateau in order to document the magmatic response to subduction initiation and the physical, petrologic, and chemical stratigraphy of a nascent subduction zone. Two of these sites (U1440 and U1441) are underlain by fore-arc basalt (FAB). FABs have mid-ocean ridge basalt (MORB)-like compositions, however, FAB are consistently lower in the high-field strength elements (TiO, PO, Zr) and Ni compared to MORB, with NaO at the low end of the MORB field and FeO* at the high end. Almost all FABs are light rare earth element depleted, with low total REE, and have low ratios of highly incompatible to less incompatible elements (Ti/V, Zr/Y, Ce/Yb, and Zr/Sm) relative to MORB. Chemostratigraphic trends in Hole U1440B are consistent with the uppermost lavas forming off axis, whereas the lower lavas formed beneath a spreading center axis. Axial magma of U1440B becomes more fractionated upsection; overlying off-axis magmas return to more primitive compositions. Melt models require a two-stage process, with early garnet field melts extracted prior to later spinel field melts, with up to 23% melting to form the most depleted compositions. Mantle equilibration temperatures are higher than normal MORB (1,400 °C-1,480 °C) at relatively low pressures (1-2 GPa), which may reflect an influence of the Manus plume during subduction initiation. Our data support previous models of FAB origin by decompression melting but imply a source more depleted than normal MORB source mantle.
伊豆-小笠原-马里亚纳(IBM)弧前区保存了约5200万年前俯冲作用开始时形成的火成岩组合。国际大洋发现计划(IODP)352航次在小笠原高原附近的弧前区钻取了四个站位的岩芯,以记录对俯冲作用开始的岩浆响应以及新生俯冲带的物理、岩石学和化学地层。其中两个站位(U1440和U1441)的基底为弧前玄武岩(FAB)。FAB具有类似大洋中脊玄武岩(MORB)的成分,然而,与MORB相比,FAB的高场强元素(TiO、PO、Zr)和Ni含量始终较低,NaO处于MORB范围的低端,FeO*处于高端。几乎所有FAB都亏损轻稀土元素,稀土总量较低,并且相对于MORB,其高不相容元素与低不相容元素的比值(Ti/V、Zr/Y、Ce/Yb和Zr/Sm)较低。U1440B孔的化学地层趋势与最上部熔岩在轴外形成一致,而下部熔岩在扩张中心轴下方形成。U1440B的轴部岩浆向上部变得更加分异;上覆的轴外岩浆恢复到更原始的成分。熔体模型需要一个两阶段过程,早期石榴石相熔体在后期尖晶石相熔体之前被提取出来,最高可达23%的熔融形成最亏损的成分。在相对较低的压力(1-2GPa)下,地幔平衡温度高于正常MORB(1400℃-1480℃),这可能反映了俯冲作用开始期间马努斯地幔柱的影响。我们的数据支持先前关于FAB起源于减压熔融的模型,但意味着其源区比正常MORB源区地幔更亏损。