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下寒武统黑色页岩金属富集机理与小行星撞击
引用本文:丁卫平,代晓光,邓宇飞,王富强.下寒武统黑色页岩金属富集机理与小行星撞击[J].科学技术与工程,2023,23(21):8945-8958.
作者姓名:丁卫平  代晓光  邓宇飞  王富强
作者单位:中化地质矿山总局地质研究院
基金项目:中化地质矿山总局地质研究院2021年研究项目(DYKJ202101)
摘    要:扬子地台寒武系下统存在富含V、Ni、Mo和铂族元素(platinum group element, PGE)等的黑色页岩,局部地区有U或者Ba、Hg、As等的富集,研究这些元素富集机理有利于寻找相关矿产或者探究地质事件。6 500万年前的小行星撞击地球产生了高PGE含量的地层或者化石,依据这一事实和陨石的特征及其他地质地球化学证据,推断下寒武统黑色页岩中Ni-Mo-PGE富集是陨石撞击结果,PGE中的Ir、Os富集最明显是因为二者最抗淋滤。U在康滇地轴东侧黑色页岩中最高可达480×10-6,因康滇地轴本身就存在混合型铀矿,推测黑色页岩中U来自它的风化。据V和Ba-Hg-As等的地化特性,认为V富集是受生物活动影响,但因V易于在热泉水中富集,故寒武纪早期泛非运动的构造-热事件可导致V富集成矿,Ba、Hg、As也因该事件产生构造裂隙后,它们优先随热液沿裂隙上升富集,并在海底局部成矿。此外,5.65亿年前的埃迪卡拉动物群发生地基本上就是5.8亿年前小行星撞击地点,提出此次行星撞击可能与埃迪卡拉生物群出现存在因果关系。由于在中国存在寒武纪澄江生物群大爆发事件,推测该次生物...

关 键 词:小行星  撞击  下寒武统  黑色页岩  金属富集  康滇地轴  铀矿
收稿时间:2022/10/20 0:00:00
修稿时间:2023/7/14 0:00:00

Black shale metal enrichment of the lower Cambrian and asteroid impact
Ding Wei Ping,Dai Xiaoguang,Deng Yufei,Wang Fuqiang.Black shale metal enrichment of the lower Cambrian and asteroid impact[J].Science Technology and Engineering,2023,23(21):8945-8958.
Authors:Ding Wei Ping  Dai Xiaoguang  Deng Yufei  Wang Fuqiang
Institution:Geological Institute of China Chemical Geology and Mine Bureau, Beijing
Abstract:There is black shale rich in V, Ni, Mo and PGE at the Lower Cambrian Formation in Yangtze platform,and local U or Ba, Hg and As are enriched. Studying the enrichment mechanism of these elements is conducive to finding relevant minerals or probing geological events,The asteroid impact 65 million years ago on Earth produced strata or fossils with high PGE content. Based on this fact and the characteristics of the meteorite and other geological and geochemical properties, it is inferred that Ni-Mo-PGE enrichment in the lower Cambrian black shale is the result of meteorite impact, and Ir and Os enrichment is most obvious because they are most resistant to eluviation. U reaches up to 480×10-6 in the black shale on the east side of Kangdian axis, there are some migmatite uranium deposit in Kangdian axis. U in the shale comes from the weathering of this deposit. Based on the geochemical characteristics of V and Ba-Sb-Hg-As, V enrichment is affected by biological activities, but V is easy to enrich in hot spring water, the tectonic-thermal events (Pan-African movement) in the early Cambrian can lead to V enrichment and mineralization. Because of this event, the geological structure broke through the seabed formation, Ba, Hg, As appear in geochemical front halo ,and local mineralized in the seabed. In addition, 565 million years ago Ediacaran biota basically appears in the place where asteroid impacted earth 580 million years ago, so we think that this asteroid impact may be related to biological extinction in Ediacara,due to the Cambrian Chengjiang Fossil Site outbreak in China, speculated that the Cambrian black shale also exist meteorite impact traces, The fine sandstone with debris and black shale and even conglomerate in the Lower Cambrian reflects the black shale deposition mutation deposition environment, and other geochemical characteristics also support the asteroid impact theory.
Keywords:Asteroid  Impact  Lower Cambrian  Black shale  Metal enrichment  Kangdian axis  Uranium mine  
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