朱佳豪, 裴彦良, 支鹏遥, 等, xxxx. 东印度洋东经90°海岭的地球物理特征和成因探讨[J]. 海洋科学进展, x(x): xx-xx. doi: 10.12362/j.issn.1671-6647.20230404001.
引用本文: 朱佳豪, 裴彦良, 支鹏遥, 等, xxxx. 东印度洋东经90°海岭的地球物理特征和成因探讨[J]. 海洋科学进展, x(x): xx-xx. doi: 10.12362/j.issn.1671-6647.20230404001.
ZHU J H, PEI Y L, ZHI P Y, et al, xxxx. Geophysical characteristics and genesis of the Ninetyeast Ridge in the Eastern Indian Ocean[J]. Advances in Marine Science, x(x): xx-xx. DOI: 10.12362/j.issn.1671-6647.20230404001
Citation: ZHU J H, PEI Y L, ZHI P Y, et al, xxxx. Geophysical characteristics and genesis of the Ninetyeast Ridge in the Eastern Indian Ocean[J]. Advances in Marine Science, x(x): xx-xx. DOI: 10.12362/j.issn.1671-6647.20230404001

东印度洋东经90°海岭的地球物理特征和成因探讨

Geophysical characteristics and genesis of the Ninetyeast Ridge in the Eastern Indian Ocean

  • 摘要: 东经90°海岭发育于东印度洋,自孟加拉沉积扇向南穿越赤道直至印度洋南部布罗肯脊,是世界上最长的线性构造。海岭的形成机制与东印度洋晚白垩世至新生代的多阶段演化有关,由于其跨越赤道、长度大于5000 km,南北不同区域的构造背景较为复杂,因此,其不同分段的地球物理特征也各具特色。通过分析海岭不同分段的形貌、浅层结构、重磁、地壳厚度及洋底年龄等地质地球物理数据,结合东印度洋海底扩张演化史,探讨了海岭的不同分段的成因机制。结果表明,90°E海岭的形成与板内热点活动、地幔柱-洋中脊相互作用、板块扩张与扩张中心跃迁、以及转换断层等诸多因素有关,是多种地质作用和地质过程综合作用的结果。2°N以北的海岭可能形成于远离扩张中心的印度板块内部,与板内火山作用有关联;18°S以南的部分形成于印度板块与南极洲板块边界转换断层附近;而2°N~18°S之间的中部区域则最为复杂,推测中段的形成受到了凯尔盖朗热点与沃顿扩张脊的相互作用,以及海岭下方的多次洋脊跳跃等因素的影响。分析认为,海岭中段是深入认识海岭成因机制、解决海岭构造演化和动力学机制以及脊-柱相互作用等重大科学问题的关键区域。未来在海岭中段开展地球物理测量及钻探工作,丰富海岭中段的地球物理综合数据,揭示中段不同位置岩石的物质组成与形成年代,是解决上述重大科学问题的必由之路。

     

    Abstract: The 90°E Ridge is the longest Lineament in the world, which is developed in the Eastern Indian Ocean and crosses the equator southward from the Bengal sedimentary fan to the Brocken Ridge in the south of the Indian Ocean. The formation mechanism of seamounts is related to the multi-stage evolution of the East Indian Ocean from Late Cretaceous to Cenozoic. Because its length across the equator is more than 5 000 kilometers, and the tectonic background of different regions in the north and south is more complex, the geophysical characteristics of different segments are also different. The paper analyzes geological and geophysical data such as the morphology, shallow structure, gravity and magnetism, crustal thickness, and ocean floor age of different sections of the ridge, and combines them with the evolution history of seafloor expansion in the Eastern Indian Ocean to explore the genetic mechanisms of different sections of the ridge. The results show that the formation of the 90°E Ridge is related to many factors, such as intraplate hot spot activity, mantle plume mid ocean ridge interaction, plate expansion and the transition of the expansion center, as well as transform faults, and is the result of multiple geological processes and geological processes. The ridge to the north of 2°N may be formed in the interior of Indian Plate far away from the expansion center, which is related to intraplate volcanism; The part to the south of 18°S was formed near the boundary transform fault between Indian Plate and Antarctica Plate; The central region between 2°N and 18°S is the most complex, and it is speculated that the formation of the middle section is influenced by factors such as the interaction between the Kerguelen hotspot and the Wharton spreading ridge, as well as multiple ridge jumps below the ridge. Analysis suggests that the middle section of the ridge is a key area for in-depth understanding of the genetic mechanism of the ridge, solving major scientific problems such as structural evolution and dynamic mechanisms of the ridge, and interactions between ridge and mantle plume. In the future, the only way to solve the above major scientific problems is to carry out geophysical survey and drilling work in the middle of the ridge, enrich the comprehensive geophysical data in the middle of the ridge, and reveal the material composition and formation age of rocks at different locations in the middle of the ridge.

     

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