TY - JOUR
T1 - Melt–fluid infiltration along detachment shear zones in oceanic core complexes
T2 - Insights from amphiboles in gabbro mylonites from the Godzilla Megamullion, Parece Vela Basin, the Philippine Sea
AU - Harigane, Yumiko
AU - Okamoto, Atsushi
AU - Morishita, Tomoaki
AU - Snow, Jonathan E.
AU - Tamura, Akihiro
AU - Yamashita, Hiroyuki
AU - Michibayashi, Katsuyoshi
AU - Ohara, Yasuhiko
AU - Arai, S.
N1 - Funding Information:
We thank the captain and crew of the R/V Hakuho-maru, the science teams during cruise KH07-02, and Kyoko Okino and Teruaki Ishii for their support and cooperation during this study. We also thank Yongjun Gao for technical assistance with LA–ICP–MS analyses at the University of Houston, and Genji Saito and Nobuo Geshi for technical advice on F and Cl measurements by JXA-8900 EPMA at GSJ-Lab, AIST. We are grateful to Laurence Coogan, Othmar Müntener, Ricard Tribuzio and an anonymous reviewer who provided thoughtful comments on this paper. We thank Aaron Stallard of Stallard Scientific Editing and Christopher Conway for improving the manuscript. This study was supported by research grants awarded to YH (24740344), KM (19340148 and 16340151), and SA (20244085) by the Japan Society for the Promotion of Science, to JES (OCE 1030950) by the National Science Foundation, and to TM as a Grant-in-Aid for Scientific Research on Innovative Areas (The Ministry of Education, Culture, Sports, Science and Technology) for Geofluids (led by E. Takahashi). Bathymetric data that has been used at Fig. 1 is confidential. All data of major and trace element analyses in our article are shown in Supplemental material (Tables S1-S6).
Funding Information:
We thank the captain and crew of the R/V Hakuho-maru, the science teams during cruise KH07-02, and Kyoko Okino and Teruaki Ishii for their support and cooperation during this study. We also thank Yongjun Gao for technical assistance with LA–ICP–MS analyses at the University of Houston, and Genji Saito and Nobuo Geshi for technical advice on F and Cl measurements by JXA-8900 EPMA at GSJ-Lab, AIST. We are grateful to Laurence Coogan, Othmar Müntener, Ricard Tribuzio and an anonymous reviewer who provided thoughtful comments on this paper. We thank Aaron Stallard of Stallard Scientific Editing and Christopher Conway for improving the manuscript. This study was supported by research grants awarded to YH (24740344), KM ( 19340148 and 16340151 ), and SA ( 20244085 ) by the Japan Society for the Promotion of Science , to JES ( OCE 1030950 ) by the National Science Foundation , and to TM as a Grant-in-Aid for Scientific Research on Innovative Areas (The Ministry of Education, Culture, Sports, Science and Technology) for Geofluids (led by E. Takahashi).
Publisher Copyright:
© 2019 Elsevier B.V.
PY - 2019/11/1
Y1 - 2019/11/1
N2 - Multiple generations of amphibole may form in the lower crust due to magmatism and metamorphism during the development of oceanic core complexes. We investigated the occurrence and chemical compositions of amphibole in gabbro mylonites from the medial area of the Godzilla Megamullion along the Parece Vela Rift in the Philippine Sea. The samples contain brown and green amphiboles with a variety of different textures that may have different origins. The brown amphibole occurs mainly as blebs in clinopyroxene porphyroclasts (Bleb amphibole), the rims around clinopyroxene porphyroclasts (Coronitic amphibole), and as porphyroclasts and fine-grained amphibole within the matrix (Matrix amphibole). The trace element and Cl contents of the bleb and green amphiboles indicate magmatic and metamoprhic origins, respectively. The bleb amphibole is interpreted to have crystallized from a hydrous silicate melt derived from an oxide gabbro-forming melt prior to retrograde metamorphism. In contrast, the compositions of the coronitic amphibole and matrix amphibole vary between those of typical magmatic and metamorphic amphiboles, suggesting that the amphibole-forming reactions were continuously retrogressive. Retrograde metamorphism is generally interpreted to have involved seawater-derived fluids, but the trace element contents of the coronitic and matrix amphiboles do not differ significantly from those of the original minerals (i.e., clinopyroxene and plagioclase). One sample of gabbro mylonite (KH07–02-D18–1) contains amphiboles with high concentrations of light rare earth elements, indicating a large influx of externally derived LREE-enriched fluids. These fluids are interpreted to have formed from an interaction between hydrous silicate melt with LREE-enriched composition and seawater-derived fluid. Our results suggest that multiple phases of melt–fluid infiltration occurred during the development of the detachment fault at the Godzilla Megamullion.
AB - Multiple generations of amphibole may form in the lower crust due to magmatism and metamorphism during the development of oceanic core complexes. We investigated the occurrence and chemical compositions of amphibole in gabbro mylonites from the medial area of the Godzilla Megamullion along the Parece Vela Rift in the Philippine Sea. The samples contain brown and green amphiboles with a variety of different textures that may have different origins. The brown amphibole occurs mainly as blebs in clinopyroxene porphyroclasts (Bleb amphibole), the rims around clinopyroxene porphyroclasts (Coronitic amphibole), and as porphyroclasts and fine-grained amphibole within the matrix (Matrix amphibole). The trace element and Cl contents of the bleb and green amphiboles indicate magmatic and metamoprhic origins, respectively. The bleb amphibole is interpreted to have crystallized from a hydrous silicate melt derived from an oxide gabbro-forming melt prior to retrograde metamorphism. In contrast, the compositions of the coronitic amphibole and matrix amphibole vary between those of typical magmatic and metamorphic amphiboles, suggesting that the amphibole-forming reactions were continuously retrogressive. Retrograde metamorphism is generally interpreted to have involved seawater-derived fluids, but the trace element contents of the coronitic and matrix amphiboles do not differ significantly from those of the original minerals (i.e., clinopyroxene and plagioclase). One sample of gabbro mylonite (KH07–02-D18–1) contains amphiboles with high concentrations of light rare earth elements, indicating a large influx of externally derived LREE-enriched fluids. These fluids are interpreted to have formed from an interaction between hydrous silicate melt with LREE-enriched composition and seawater-derived fluid. Our results suggest that multiple phases of melt–fluid infiltration occurred during the development of the detachment fault at the Godzilla Megamullion.
KW - Amphibole
KW - Detachment fault
KW - Gabbro mylonite
KW - Godzilla Megamullion
KW - Oceanic core complex
KW - Trace elements
UR - http://www.scopus.com/inward/record.url?scp=85068431533&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85068431533&partnerID=8YFLogxK
U2 - 10.1016/j.lithos.2019.06.019
DO - 10.1016/j.lithos.2019.06.019
M3 - Article
AN - SCOPUS:85068431533
SN - 0024-4937
VL - 344-345
SP - 217
EP - 231
JO - Lithos
JF - Lithos
ER -