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在完整的大洋地壳中钻探辉长岩。

Drilling to gabbro in intact ocean crust.

作者信息

Wilson Douglas S, Teagle Damon A H, Alt Jeffrey C, Banerjee Neil R, Umino Susumu, Miyashita Sumio, Acton Gary D, Anma Ryo, Barr Samantha R, Belghoul Akram, Carlut Julie, Christie David M, Coggon Rosalind M, Cooper Kari M, Cordier Carole, Crispini Laura, Durand Sedelia Rodriguez, Einaudi Florence, Galli Laura, Gao Yongjun, Geldmacher Jörg, Gilbert Lisa A, Hayman Nicholas W, Herrero-Bervera Emilio, Hirano Nobuo, Holter Sara, Ingle Stephanie, Jiang Shijun, Kalberkamp Ulrich, Kerneklian Marcie, Koepke Jürgen, Laverne Christine, Vasquez Haroldo L Lledo, Maclennan John, Morgan Sally, Neo Natsuki, Nichols Holly J, Park Sung-Hyun, Reichow Marc K, Sakuyama Tetsuya, Sano Takashi, Sandwell Rachel, Scheibner Birgit, Smith-Duque Chris E, Swift Stephen A, Tartarotti Paola, Tikku Anahita A, Tominaga Masako, Veloso Eugenio A, Yamasaki Toru, Yamazaki Shusaku, Ziegler Christa

机构信息

Department of Earth Science and Marine Science Institute, University of California, Santa Barbara, CA 93106, USA.

出版信息

Science. 2006 May 19;312(5776):1016-20. doi: 10.1126/science.1126090. Epub 2006 Apr 20.

Abstract

Sampling an intact sequence of oceanic crust through lavas, dikes, and gabbros is necessary to advance the understanding of the formation and evolution of crust formed at mid-ocean ridges, but it has been an elusive goal of scientific ocean drilling for decades. Recent drilling in the eastern Pacific Ocean in Hole 1256D reached gabbro within seismic layer 2, 1157 meters into crust formed at a superfast spreading rate. The gabbros are the crystallized melt lenses that formed beneath a mid-ocean ridge. The depth at which gabbro was reached confirms predictions extrapolated from seismic experiments at modern mid-ocean ridges: Melt lenses occur at shallower depths at faster spreading rates. The gabbros intrude metamorphosed sheeted dikes and have compositions similar to the overlying lavas, precluding formation of the cumulate lower oceanic crust from melt lenses so far penetrated by Hole 1256D.

摘要

通过熔岩、岩脉和辉长岩对完整的大洋地壳序列进行采样,对于推进对在大洋中脊形成的地壳的形成和演化的理解是必要的,但几十年来,这一直是科学大洋钻探难以实现的目标。最近在东太平洋1256D钻孔的钻探在地震层2内达到了辉长岩,该层位于以超快扩张速率形成的地壳中1157米深处。这些辉长岩是在大洋中脊下方形成的结晶熔体透镜体。达到辉长岩的深度证实了从现代大洋中脊的地震实验推断出的预测:熔体透镜体在扩张速率较快时出现在较浅的深度。这些辉长岩侵入了变质的席状岩脉,并且其成分与上覆熔岩相似,这排除了1256D钻孔迄今穿透的熔体透镜体形成堆积型下洋壳的可能性。

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