首页> 外文期刊>GSA Bulletin >Tectonic and chronostratigraphic implications of new 40Ar/39Ar geochronology and geochemistry of the Arman and Maltan-Ola volcanic fields, Okhotsk-Chukotka volcanic belt, northeastern Russia
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Tectonic and chronostratigraphic implications of new 40Ar/39Ar geochronology and geochemistry of the Arman and Maltan-Ola volcanic fields, Okhotsk-Chukotka volcanic belt, northeastern Russia

机译:俄罗斯东北部鄂霍次克-楚科奇火山带阿尔曼和马尔他-奥拉火山田新的40Ar / 39Ar地球年代学和地球化学的构造和年代地层意义

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The Okhotsk-Chukotka volcanic belt is part of an extensive late Early to Late Cretaceous Andean-style magmatic arc that spans the entire eastern margin of the Asian continent. The belt itself stretches 3000 km from the Chukotka Peninsula to the Uda River and comprises 1.2 x 106 km3 of volcanic rock over a 500,000 km2 area. Despite its size and regional tectonic significance, the time span of magmatic activity is poorly constrained and the subject of significant debate, mostly in the Russian literature. In this paper, we provide new geochronologic control on the timing of inception and cessation of magmatism for the Arman and Maltan-Ola volcanic fields. These field localities were chosen because they are well studied, relatively accessible, and contain floral assemblages that have been used to correlate volcanic sequences at the regional scale. The majority of the volcanic sequence was emplaced between 85.5 ± 1.3 Ma and 74.0 ± 1.2 Ma, as shown by 17 new 40Ar/39Ar ages. The Coniacian– Santonian to Campanian age range indicated is 15 m.y. younger than the Albian to early Cenomanian age range given by a synthesis of floral stratigraphic, K-Ar, and Rb-Sr geochronologic data. The calc- alkaline part of the volcanic section spans an apparent age range of 85.5 ± 1.3 Ma to 80.7 ± 0.8 Ma. Capping basalts were emplaced between 77.5 ± 1.1 Ma and 74.0 ± 1.2 Ma and exhibit a within-plate geochemical signature, which we attribute to a temporally and geochemically distinct, possibly extension-related, phase of magmatism. The apparent northwestward migration of the arc front from the interior (seaward) zone (Taigonos Peninsula, Magadan batholith) in Albian–Cenomanian time to the Arman and Maltan-Ola volcanic fields in Coniacian–Santonian to Campanian time may be explained by shallowing of the subducting paleo-Pacific (Kula?) oceanic plate.
机译:鄂霍次克-楚科奇火山带是 晚白垩纪安第斯山脉晚期岩浆弧的一部分,横跨整个亚洲大陆的东部边缘。地带本身 从楚科奇半岛延伸到乌达河 3000公里,包括1.2 x 10 6 km 3 50万 km 2 区域的火山岩的数量。尽管其规模和区域构造意义重大,但 的岩浆活动时间跨度却受限制较弱,因此 成为重要的辩论主题,主要是在俄罗斯文学中。 本文为Arman 和马耳他-奥拉火山田的 岩浆形成和停止的时间提供了新的地质年代学控制。选择这些田间位置是因为对其进行了充分研究,相对容易使用,并且包含了花序组合,这些花序被用来关联该地区的 火山序列,因此选择了 规模。大部分 火山序列位于85.5±1.3 Ma 和74.0±1.2 Ma之间,如17个新的 40 Ar / 39 Ar年龄。 所显示的Coniacian– Santonian至Campanian年龄范围是<15>由花地层,K-Ar和Rb-Sr 年代学数据综合而成,比阿尔比(Albian)年龄小,到塞诺曼尼亚早期年龄范围 。火山 部分的钙碱性部分的表观年龄范围为85.5±1.3 Ma 至80.7±0.8 Ma。封盖玄武岩放置在 77.5±1.1 Ma和74.0±1.2 Ma之间,并显示出 板内地球化学特征,我们将其暂时归因于 和地球化学上不同的,可能与伸展有关的岩浆作用的 相。弧前锋从内(海)带(塔戈诺斯半岛, Magadan岩基)向西北方向迁移到阿尔曼 科尼西亚-桑顿期到坎帕尼亚时代的马耳他-奥拉火山田可能是由俯冲古太平洋板块的浅水层解释的。 < / sup>

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  • 来源
    《GSA Bulletin》 |2004年第6期|637-654|共18页
  • 作者单位

    Department of Geological and Environmental Sciences, Stanford University, Stanford, California 94305, USA;

    North East Interdisciplinary Scientific Research Institute, Far East Branch, Russian Academy of Sciences, Magadan, Portovaya Ulitsa, 16, 685000, Russia;

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