冲击灾变与大灭绝的回顾、透视与展望:迈向新生代撞击事件地层学

IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Earth-Science Reviews Pub Date : 2024-08-31 DOI:10.1016/j.earscirev.2024.104904
Grzegorz Racki , Christian Koeberl
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引用次数: 0

摘要

尽管陨石撞击研究有几个有时是著名的传播者,但在 20 世纪 80 年代之前,陨石撞击研究长期处于边缘地位。从那时起,由于阿尔瓦雷斯(Alvarez)关于中生代末期奇克苏鲁伯(Chicxulub)发生灾难性撞击的假说被迅速接受,人们开始大力寻找撞击-灭绝对。然而,在声称同时发生的大规模灭绝中,未完全确定和/或间接确定年代的撞击坑出现了重大错误。例如,仅以地球物理研究为依据的假定巨型陨石坑,如那些据称由撞击驱动的二叠纪末和奥陶纪晚期灭绝的证据,并没有得到邻近地区任何真实撞击证据(如灾难性沉积)的支持。该方法首先是(1)确定撞击坑和喷出物,然后是(2)对其进行精确的辐射或生物地层测年,最后是(3)评估撞击的 "杀伤 "潜力。根据全球数据库中最新的撞击坑信息和更新的地层边界年龄,撞击对广泛定义的大规模灭绝的贡献已被证伪。在新生代,发生了两种截然不同的撞击现象:奇克苏鲁伯小行星特大撞击和中奥陶纪至晚奥陶纪来自碎裂的软玉体的长时间小行星雨。因此,有人提出将稳定的背景条件(撞击单独发生,很少成群发生)和扰动(轰击)时间段区分开来。对于其他四次 "五大灭绝",目前有关撞击触发的证据已经得到详细审查,但尚未得到证实。研究还考虑了由小行星雨引发的晚始新世至渐新世早期的长期撞击强化危机的可能性,以及伴随其他重大陨石坑事件发生的生物变化:北欧中期的马尼库阿甘和侏罗纪末的莫罗翁结构。特别是对于波皮盖小行星群(由成对的 100 公里大小的陨石坑暗示)和莫洛克汶-莫约尼尔可能的巧合,撞击特征与可能的逐步生物事件之间的关系远非定论。即使在直径为 40 千米的陨石坑中记录到的中型陨石撞击可能引发了近乎全球性的气候灾害,但由于大灾难严重程度控制的多样性,其杀伤效应也是不可预测的。此外,奥陶纪宇宙轰击也没有对生物大多样化产生任何负面影响。然而,小行星群可能(由于太阳系内部异常的尘埃)最终分别引发或加速了奥陶纪晚期和渐新世的冰期。总之,这意味着生物圈对地外刺激的反应具有连续性。此外,还首次尝试解释预测的其他奇克苏鲁伯类特大事件的隐藏记录。根据之前提出的巨型日震和地震记录,对中奥陶纪、晚泥盆纪和晚三叠纪 "消失的 "海洋撞击进行了追踪。弗拉斯年-法门年过渡时期似乎最有可能发生这种隐秘的大灾难,表现为全球性的 "顶部-弗拉斯年再加工事件"。总之,在 18 次灭绝中,有 1 次已证实是撞击引起的大灭绝,3-4 次可能是撞击增强的生物危机,现在可以从地外强迫的角度加以考虑。这一初步结论与近期文献中关于四次 "大灭绝 "与四次最大撞击有关的简单断言只是表面上一致,因为还需要很多实质性证据。事实上,有据可查的火山大灾难目前已成为新灾难地质学的主流。许多关于地外因素与生物圈更替之间周期性因果关系的建议(大多由非地质学家提出)再次被证明是完全不确定的。在这种情况下,现实主义撞击灾变论和阿尔瓦雷斯的 "天体理论 "的未来仍有许多引人入胜的话题。相比之下,"非螺栓理论 "的灾难性概念,如星系间暗物质的触发作用,在化石记录中无法为这些 "看不见的 "现象提供真正的证据,这一点太值得怀疑了。
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Impact catastrophism versus mass extinctions in retrospective, perspective and prospective: Toward a Phanerozoic impact event stratigraphy
Despite several, sometimes prominent propagators, meteorite impact research had a long period of peripheral status until the 1980s. Since then, there has been an intense search for impact-extinction pairs, driven by the rapid acceptance of Alvarez's hypothesis of a catastrophic Chicxulub impact at the end of the Mesozoic era. However, substantial errors have occurred for incompletely identified and/or indirectly dated impact craters in the context of purportedly coeval mass extinctions. For example, supposed giant craters based only on geophysical studies, such as those alleged as evidence of impact-driven end-Permian and Late Ordovician extinctions, are not supported by any real impact evidence (e.g., catastrophic sedimentation) in adjacent areas.
The updated three-step methodology presents an accurate approach to cause-effect inference in impact catastrophism. It begins with (1) conclusive recognition of impact craters and ejecta, followed by (2) their precise radiometric or biostratigraphic dating, and concludes with (3) assessing the impact's “kill” potential. The impact contribution to widely defined mass extinctions has been falsified based on the latest crater information from the global database and the updated ages of stratigraphic boundaries. In the Phanerozoic, two contrasting collision phenomena occurred: the Chicxulub asteroid mega-impact and a prolonged asteroid shower from a shattered chondritic body in the Middle to Late Ordovician. Accordingly, a distinction has been proposed between steady background conditions (impacts occurring singly and rarely in clusters) and perturbation (bombardment) intervals. Current evidence for an impact trigger has been reviewed in detail for the other four Big Five mass extinctions, but no confirmation has been found. The probability of a prolonged impact-enhanced Late Eocene to Early Oligocene crisis, caused by an asteroid shower, is considered, as well as biotic changes accompanying other major cratering events: the mid-Norian Manicouagan and the end-Jurassic Morokweng structures. In particular, for the Popigai asteroid swarm, implied from paired 100-km-sized craters, and the possible Morokweng-Mjølnir coincidence, the relationships between impact signatures and likely stepwise biotic events are far from conclusive. Even if medium-sized bolide impacts, recorded in ∼40-km-diameter craters, may have initiated near-global climatic hazards, the killing effect is unpredictable due to the diversity of cataclysm severity controls. Also the Ordovician cosmic bombardment did not have any negative influence on the great biodiversification. However, the asteroid swarms may have (by unusual dustiness of the inner Solar System) ultimately triggered or accelerated ice ages in the Late Ordovician and Oligocene, respectively. Overall, this implies a continuum in the biosphere's response to extraterrestrial stimuli.
Furthermore, a first attempt was made to explain the hidden record of predicted additional Chicxulub-type mega-events. ‘Lost’ oceanic impacts in the Middle Ordovician, Late Devonian, and Late Triassic were traced in the context of previously suggested records of mega-tsunamis and seismicity. The Frasnian-Famennian transition seems to be the most likely case of such a cryptic cataclysm, manifested in the worldwide “top-Frasnian reworking event.” In summary, of the 18 extinctions, one confirmed impact-induced mass extinction and 3–4 possible impact-enhanced biotic crises can now be considered in terms of extraterrestrial forcing. This tentative conclusion is only superficially consistent with the simplistic assertion in recent literature of four ‘mass extinctions’ associated with the four largest impacts, as much substantial evidence is still needed. In fact, well-documented volcanic cataclysms currently shape the mainstream neocatastrophic geology.
Many proposals, mostly by non-geologists, of periodic causal connections between extraterrestrial factors and biosphere turnovers are shown once more to be totally inconclusive. In this context, the future of actualistic impact catastrophism and Alvarez's ‘bolide theory’ remains open to many fascinating topics. In contrast, ‘non-bolide’ catastrophic concepts, such as the triggering role of intergalactic dark matter, are too questionable to provide real evidence in the fossil record for these ‘invisible’ phenomena.
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来源期刊
Earth-Science Reviews
Earth-Science Reviews 地学-地球科学综合
CiteScore
21.70
自引率
5.80%
发文量
294
审稿时长
15.1 weeks
期刊介绍: Covering a much wider field than the usual specialist journals, Earth Science Reviews publishes review articles dealing with all aspects of Earth Sciences, and is an important vehicle for allowing readers to see their particular interest related to the Earth Sciences as a whole.
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