Morishita Tomoaki

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Morishita
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Tomoaki
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Dynamic accretion beneath a slow-spreading ridge segment: IODP hole 1473A and the Atlantis Bank oceanic core complex

2019-11-07 , Dick, Henry J. B. , MacLeod, Christopher J. , Blum, Peter , Abe, Natsue , Blackman, Donna K. , Bowles, Julie A. , Cheadle, Michael J. , Cho, K. , Ciazela, Jakub , Deans, Jeremy , Edgcomb, Virginia P. , Ferrando, Carlotta , France, Lydéric , Ghosh, Biswajit , Ildefonse, Benoit , John, Barbara E. , Kendrick, Mark A. , Koepke, Juergen , Leong, James , Liu, Chuanzhou , Ma, Qiang , Morishita, Tomoaki , Morris, Antony , Natland, James H. , Nozaka, Toshio , Pluemper, Oliver , Sanfilippo, Alessio , Sylvan, Jason B. , Tivey, Maurice A. , Tribuzio, Riccardo , Viegas, G.

809 deep IODP Hole U1473A at Atlantis Bank, SWIR, is 2.2 km from 1,508‐m Hole 735B and 1.4 from 158‐m Hole 1105A. With mapping, it provides the first 3‐D view of the upper levels of a 660‐km2 lower crustal batholith. It is laterally and vertically zoned, representing a complex interplay of cyclic intrusion, and ongoing deformation, with kilometer‐scale upward and lateral migration of interstial melt. Transform wall dives over the gabbro‐peridotite contact found only evolved gabbro intruded directly into the mantle near the transform. There was no high‐level melt lens, rather the gabbros crystallized at depth, and then emplaced into the zone of diking by diapiric rise of a crystal mush followed by crystal‐plastic deformation and faulting. The residues to mass balance the crust to a parent melt composition lie at depth below the center of the massif—likely near the crust‐mantle boundary. Thus, basalts erupted to the seafloor from >1,550 mbsf. By contrast, the Mid‐Atlantic Ridge lower crust drilled at 23°N and at Atlantis Massif experienced little high‐temperature deformation and limited late‐stage melt transport. They contain primitive cumulates and represent direct intrusion, storage, and crystallization of parental MORB in thinner crust below the dike‐gabbro transition. The strong asymmetric spreading of the SWIR to the south was due to fault capture, with the northern rift valley wall faults cutoff by a detachment fault that extended across most of the zone of intrusion. This caused rapid migration of the plate boundary to the north, while the large majority of the lower crust to spread south unroofing Atlantis Bank and uplifting it into the rift mountains.

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Occurrence of felsic rocks in oceanic gabbros from IODP hole U1473A: Implications for evolved melt migration in the lower oceanic crust.

2018-12-20 , Nguyen, Du Khac , Morishita, Tomoaki , Soda, Yusuke , Tamura, Akihiro , Ghosh, Biswajit , Harigane, Yumiko , France, Lydéric , Liu, Chuanzhou , Natland, James H. , Sanfilippo, Alessio , MacLeod, Christopher J. , Blum, Peter , Dick, Henry J. B.

Felsic rocks are minor in abundance but occur ubiquitously in International Ocean Discovery Program Hole U1473A, Southwest Indian Ridge. The trace element abundances of high-Ti brown amphibole, plagioclase, and zircon in veins, as well as the presence of myrmekitic texture in the studied felsic rocks support crystallization origin from highly-evolved melts, probably controlled by fractional crystallization. Based on geochemical criteria and texture of the mineral assemblage in felsic rocks and their relationship with host gabbros, they can be divided into three types: (1) Felsic rock with sharp boundaries is formed when felsic melt intrudes into fractures of host gabbros, resulting in minimal interaction between the melt and the wall minerals. (2) Replacive felsic rock, which is characterized by a pseudomorphic replacement of minerals in the host gabbro. This vein type is caused by the replacement of the host mineralogy by minerals in equilibrium with the felsic melts. (3) Felsic rock with diffused boundaries is formed either by infiltration of felsic melt into the solidifying gabbro body or crystallization of interstitial melts. Infiltration modes of felsic melts are likely controlled by the temperature condition of the cooling host gabbros.