When a Plateau Suppresses a Plume: Disappearance of the Samoan Plume Under the Ontong Java Plateau

IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY
AGU Advances Pub Date : 2024-06-26 DOI:10.1029/2023AV001079
M. G. Jackson, V. A. Finlayson, Bernhard Steinberger, Kevin Konrad
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Abstract

The Samoan hotspot generated an age-progressive volcanic track that can be traced back to 24 Ma at Alexa Bank, but the trace of the older portion (>24 Ma) of the hotspot track is unclear. We show that six seamounts located in and around the Magellan Seamount chain—north of the Ontong-Java Plateau (OJP)—have ages (87–106 Ma), geochemistry, and locations consistent with absolute plate motion model reconstructions of the Samoan hotspot track in the late Cretaceous, and three additional seamounts have geochemistry and locations consistent with a Samoan origin. However, a large segment of the Samoan hotspot (24–87 Ma) remains unidentified. Absolute plate motion models show that, from ∼60 to 30 Ma, the OJP passed over the Samoan plume. The exceptional thickness of the OJP lithosphere may have largely suppressed Samoan plume melting because the inferred volcanic trace of the Samoan hotspot wanes, and then disappears, on the OJP. Fortunately, 44 Ma volcanism at Malaita Island, located on the southern margin of the OJP, has a location, age, and geochemistry consistent with a Samoan plume origin, and provides a “missing link” bridging the younger and older segments of the Samoan hotspot. Our synthesis of geochemical, geochronological, and plate motion model evidence reveals that Samoa exhibits a clear hotspot age progression for over 100 Myr. Passage of ancient plateaus over young plumes—here called “plume-plateau” interaction—may be relatively common: the OJP also passed over the putative Rarotonga hotspot, and the Society and Pitcairn hotspots were overtopped by the Manihiki Plateau.

Abstract Image

当高原抑制烟羽时:翁通爪哇海台下萨摩亚烟羽的消失
萨摩亚热点产生了一条年龄递增的火山轨迹,可以追溯到亚历山大岸的 24 Ma,但热点轨迹的较早部分(24 Ma)的踪迹尚不清楚。我们的研究表明,位于麦哲伦海山链(翁通-爪哇高原(OJP)以北)及其周围的六座海山的年龄(87-106 Ma)、地球化学特征和位置与晚白垩世萨摩亚热点轨道的绝对板块运动模型重建结果一致,另外三座海山的地球化学特征和位置与萨摩亚起源一致。然而,萨摩亚热点的很大一部分(24-87 Ma)仍未确定。绝对板块运动模型显示,从 60 至 30 Ma,OJP 穿过萨摩亚羽流。OJP岩石圈的特殊厚度可能在很大程度上抑制了萨摩亚羽流的熔化,因为推断的萨摩亚热点火山痕迹在OJP上减弱,然后消失。幸运的是,位于奥杰帕南缘的马莱塔岛(Malaita Island)的 44 Ma 火山活动在位置、年龄和地球化学方面都与萨摩亚羽流的起源相吻合,并提供了连接萨摩亚热点较年轻部分和较古老部分的 "缺失环节"。我们对地球化学、地质年代和板块运动模型证据的综合分析表明,萨摩亚在 100 多亿年的时间里呈现出明显的热点年龄递增现象。古老的高原经过年轻的羽块--这里称为 "羽块-高原 "相互作用--可能比较常见:OJP 也经过假定的拉罗汤加热点,而社会和皮特凯恩热点被马尼希基高原覆盖。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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CiteScore
2.90
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