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1.
Yukio Isozaki Shinji Yamamoto Shuhei Sakata Hideyuki Obayashi Takafumi Hirata Ken-ichi Obori Toshinori Maebayashi Satoshi Takeshima Toshikazu Ebisuzaki Shigenori Maruyama 《地学前缘(英文版)》2018,9(4):1073-1083
Despite the recent development in radiometric dating of numerous zircons by LA-ICPMS, mineral separation still remains a major obstacle, particularly in the search for the oldest material on Earth. To improve the efficiency in zircon separation by an order of magnitude, we have designed/developed a new machine-an automatic zircon separator(AZS). This is designed particularly for automatic pick-up of100 μm-sized zircon grains out of a heavy mineral fraction after conventional separation procedures. The AZS operates in three modes:(1) image processing to choose targeted individual zircon grains out of all heavy minerals spread on a tray,(2) automatic capturing of the individual zircon grains with microtweezers, and(3) placing them one-by-one in a coordinated alignment on a receiving tray. The automatic capturing was designed/created for continuous mineral selecting without human presence for many hours. This software also enables the registration of each separated zircon grain for dating, by recording digital photo-image, optical(color) indices, and coordinates on a receiving tray. We developed two new approaches for the dating; i.e.(1) direct dating of zircons selected by LA-ICPMS without conventional resin-mounting/polishing,(2) high speed U-Pb dating, combined with conventional sample preparation procedures using the new equipment with multiple-ion counting detectors(LA-MIC-ICPMS).With the first approach, Pb-Pb ages obtained from the surface of a mineral were crosschecked with the interior of the same grain after resin-mounting/polishing. With the second approach, the amount of time required for dating one zircon grain is ca. 20 s, and a sample throughput of 150 grains per hour can be achieved with sufficient precision(ca. 0.5%).We tested the practical efficiency of the AZS, by analyzing an Archean Jack Hills conglomerate in Western Australia with the known oldest(4.3 Ga) zircon on Earth. Preliminary results are positive; we were able to obtain more than 194 zircons that are over 4.0 Ga out of ca. 3800 checked grains, and 9 grains were over 4300 Ma with the oldest at 4371 ± 7 Ma. This separation system by AZS, combined with the new approaches, guarantees much higher yield in the hunt for old zircons. 相似文献
2.
鉴于保护地调查评价历史与目标,国家公园地质考察评价基准是地质学关于地球的“时间、空间、演化”知识的发现路径,既识别国家公园候选地的国家符合性地质事件,又识别国家公园自然性、独特性、优美性、多样性、整体性的地质机制,提供国家公园最重要的自然生态系统与自然景观保育管理的地质学支撑。浙江丽水百山祖国家公园符合性的地质事件是公园发现的4.0~4.2 Ga冥古宙陆核物质的锆石晶体、中生代岛弧陆盆火山酸性火山岩系列和从流纹岩山岭到花岗岩—变质岩谷底的“峰—岭—丘—谷（盆）”的亚热带滨海山地地貌结构,地貌结构发育演化是百山祖公园最重要的自然生态系统、区域性流域水源地、独特山水景观的形成基础。保护百祖山公园地貌结构和过程的完整性与真实性是确保其重要自然生态系统自然演化和生态服务产品持续供给的基础。 相似文献
3.
扬子西缘东川落雪地区元古宙地层中3890 Ma锆石的发现 总被引：1，自引：0，他引：1
利用LA-ICP-MS U-Pb同位素测定技术,在扬子西缘滇中东川地区古元古界阿不都组流纹质玻屑熔结凝灰岩中发现了1颗冥古宙锆石,锆石具有明显的核-幔-边结构,其核部的207 Pb/206 Pb年龄为3890±47 Ma,此年龄被解释为岩浆结晶,Th/U比值为0.34;变质边的207 Pb/206 Pb年龄为3561±45～3616±55 Ma,Th/U比值为0.07～0.19.锆石的原位Hf同位素测定给出了176 Hf/177 Hf=0.280317～0.280451,εHf(t)=-4.6～0.6(平均值为-2.5),TDM1=3861～3980 Ma,TDM2=4036～4106 Ma(平均值为4059 Ma).这颗锆石为扬子陆块目前发现的最老锆石,其Hf同位素及微量元素特征说明扬子陆块存在4.0 Ga的地壳增生作用及古老陆壳的再循环;结合前人同位素研究资料,说明扬子西缘东川落雪地区元古宙时同华北陆块可能具有亲缘性;本次的发现,为扬子陆块寻找冥古宙和始太古代物质实体提供重要依据,也为认识地球早期大陆演化过程提供了重要新信息. 相似文献
4.
Balz Samuel Kamber Martin J. Whitehouse Stephen Moorbath 《Earth and Planetary Science Letters》2005,240(2):276-290
The oldest known bona fide succession of clastic metasediments occurs in the Isua Greenstone Belt, SW Greenland and consists of a variety of mica schists and rare metaconglomerates. The metasediments are in direct contact with a felsic metavolcanic lithology that has previously been dated to 3.71 Ga. Based on trace element geochemical data for > 30 metasediments, we selected the six samples with highest Zr concentrations for zircon extraction. These samples all yielded very few or no zircon. Those extracted from mica schists yielded ion probe U/Pb ages between 3.70 and 3.71 Ga. One metaconglomerate sample yielded just a single zircon of 3.74 Ga age.The mica schist hosted zircons have U/Pb ages, Th / U ratios, REE patterns and Eu anomalies indistinguishable from zircon in the adjacent 3.71 Ga felsic metavolcanic unit. Trace element modelling requires the bulk of material in the metasediments to be derived from variably weathered mafic lithologies but some metasediments contain substantial contribution from more evolved source lithologies. The paucity of zircon in the mica schists is thus explained by incorporation of material from largely zircon-free volcanic lithologies. The absence of older zircon in the mica schists and the preponderance of mafic source material imply intense, mainly basaltic resurfacing of the early Earth. The implications of this process are discussed.Thermal considerations suggest that horizontal growth of Hadean crust by addition of mafic-ultramafic lavas must have triggered self-reorganisation of the protocrust by remelting. Reworking of Hadean crust may have been aided by burial of hydrated (weathered) metabasalt due to semi-continuous addition of new voluminous basalt outpourings. This process causes a bias towards eruption of Zr-saturated partial melts at the surface with O-isotope compositions potentially different from the mantle. The oldest zircons hosted in sediments would have been buried to substantial depth or formed in plutons that crystallised at some depth, from which it took hundreds of millions of years for them to be exhumed and incorporated into much younger sediments. 相似文献
5.
笔者在"关于板块运动启动时间的争论"一文(陆松年等,2016)基础上,参阅公开发表的部分文章,介绍了前板块岩浆洋和停滞盖研究的新进展,并再次讨论有关板块运动启动时间的不同认识和观点。根据太阳系30个类地行星天体图像资料,硅酸盐质行星体在它的生命期由于冷却和岩石圈增厚似乎经历过多种构造样式,包括岩浆洋、多类型停滞盖以及板块构造。硅酸盐类行星由于增生、分异、撞击和放射性活动,使星体变热,发生熔融反应而形成"岩浆洋"。硅酸盐星球体早期很可能是大面积但寿命很短的岩浆洋,之后的星球可能受两种构造模型控制:停滞盖构造和板块构造。已有资料表明,停滞盖构造是类地行星的主要构造类型,而板块构造在类地行星中是十分罕见的。停滞盖构造是一个单一的、围绕天体的板块,基本由硅酸盐质岩石圈组成。停滞盖构造有三种主要变化形态——热管、滴状及柱状体、拆沉及上涌流。板块构造启动时间从>4.4Ga到0.85Ga至少有11种不同观点:认为板块构造始于冥古宙的有1种、始于始-古太古代的有3种、始于中-新太古代的有4种、始于古元古代有1种、始于新元古代的有2种。本文重点介绍了地球冥古宙-太古宙板块运动启动的地质学证据和特点。 相似文献
6.
全球冥古宙的研究进展和存在问题 总被引：1，自引：0，他引：1
冥古宙是地球上最老的一个地质历史时期,由于缺少可靠的岩石记录一直没有得到国际地学界的重视和承认,到2004年才在建议的国际地层表中使用了冥古宙这一术语,定义从地球形成到出现地球最老岩石这段地球历史。但冥古宙与太古宙没有明确的地质界线,一些研究者提出了不同的年代界线(3.85Ga,4.0Ga,4.03Ga),目前还存在较大分歧。目前已知残存的冥古宙岩石只有两处,一处是加拿大的阿卡斯塔片麻岩(Acasta gneiss)中两个英云闪长岩和一个变质花岗闪长岩。前者锆石U-Pb年龄为4002±4Ma和4012±6Ma,后者为4031±1Ma。另一处是东南极索尼山(Mount Sones)的麻粒岩相英云闪长质片麻岩,已获得U-Pb年龄为3927±10Ma。世界上最老的表壳岩(≥3870Ma)出露在格陵兰。冥古宙年代久远,地球形成最初的600~700Ma的初始岩石经历了陨石撞击、地壳再循环、重熔等改造,甚至再循环到地幔,几乎已经消失殆尽。目前主要以年轻岩石中的碎屑锆石或继承锆石作为桥梁,来追索这些古老锆石原来母岩的类型、特征及成因。3800Ma的碎屑锆石已在全球十多个地区发现,而以西澳伊尔岗克拉通的杰克山最多最全,从3800Ma到4404Ma都有,在3840Ma,3900~3920Ma,4000~4200Ma,4260~4300Ma和4404Ma显示峰值,其中以3900~4200Ma最为发育,4404Ma是目前世界公认的最老碎屑锆石。此外在北美克拉通、南非克拉通、华北克拉通等古老克拉通以及一些年轻造山带中都发现有冥古宙的碎屑锆石,这些锆石是追索冥古宙地质事件的重要桥梁。通过对冥古宙碎屑锆石的研究提出了很多值得重视和进一步研究的课题和内容。包括早期地壳的性质,一些锆石具有与太古宙之后岩浆锆石特征相似的环带结构,因此这些碎屑锆石的母岩大部分被认为相当花岗质,来自老地壳的重熔。冥古宙碎屑锆石的Hf同位素等综合分析表明这些碎屑锆石来源于中性熔岩的结晶,或许表明早期地壳具有中性成分特征。冥古宙锆石的成因也是一个重要的课题,根据锆石中钛的含量、锆石Ti饱和温度计计算的温度以及锆石的一些结构特征,有的研究者提出冥古宙相当一部分碎屑锆石是陨石撞击导致的岩石熔融结晶产生的,是追溯地球早期撞击事件的重要手段。在4300Ma的碎屑锆石中包裹有金刚石和石墨晶体,前者表明锆石的母岩曾处于高压条件,而后者石墨的碳同位素接近有机碳,有人认为可能为生命起源的迹象。多个地区的碎屑锆石的边部Th/U比值低,U-Pb年龄为4000Ma左右,属于变质作用的产物,表明当时地壳已具有一定厚度。冥古宙碎屑锆石的研究提出了很多重要的问题,但是由于资料有限,有些认识还存在矛盾,还需要获得更多实际资料,才能对冥古宙的地质事件过程取得更可靠的科学认识。因此今后应加强可能赋存古老碎屑锆石地区的寻找,并发现更多古老碎屑锆石。对现有的古老碎屑锆石加强综合研究以及各地区的对比研究。 相似文献
7.
华夏地块龙泉地区发现亚洲最古老的锆石 总被引：2，自引：0，他引：2
锆石这一矿物是迄今为止所发现的地球最初500个百万年间(地质学界通常称为"冥古代")的唯一地壳物质残留,对于了解地球早期地壳演化过程至关重要。近年来,随着高精度SHRIMP测年技术的广泛运用,笔者最近在华夏地块龙泉地区发现了2颗约4100 Ma的碎屑锆石。其中一颗为目前发现亚洲最古老的锆石,其内部结构简单,具有正常的震荡环带,207Pb/206Pb年龄为(4127±4)Ma;其δ18O与地幔岩浆的氧同位素类似,可能来自于早期的幔源岩浆或者未经历地表过程的深部地壳物质的熔融。另外一颗锆石具有明显的核边结构,其核部结晶年龄约为4100 Ma,变质边年龄约为4070 Ma,外围还有2层岩浆增生边年龄介于3800~3600 Ma,代表了该4100 Ma的锆石核部在后期经历了复杂的地壳演化过程,4070 Ma的变质边是目前已获得最为可靠的全球变质年龄。上述发现表明冥古宙时地壳性质和构造环境存在多样性,为认识地球早期大陆演化过程提供了重要新信息。 相似文献
8.
北秦岭西段冥古宙锆石(4.1～3.9Ga)年代学新进展 总被引：15，自引：13，他引：2
2007年王洪亮等报道在北秦岭西段火山岩中获得一粒年龄为4079±5Ma的冥古宙捕虏锆石。之后,对这一发现开展了深入的调查研究,我们除利用SHIMP技术方法对原4079Ma的锆石进行验证外,新获得了两粒~(207)Pb/~(206)Pb年龄为4007±29Ma和3908±45Ma捕获的变质成因锆石,表明早在4.0Ga已经有变质作用的发生,这或许说明在冥古宙时期地球已经具有相当规模和厚度的地壳。同时开展的岩石学研究表明,蕴含古老锆石的母岩属于火山碎屑熔岩类而不是火山熔岩。 相似文献
9.
http://dx.doi.org/10.1016/j.gsf.2016.08.001 总被引：1，自引：1，他引：0
Geological observations indicate that there are only a few rocks of Archean Earth and no Hadean rocks on the surface of the present-day Earth. From these facts, many scientists believe that the primordial continents never existed during Hadean Earth, and the continental volume has kept increasing. On the other hand, recent studies reported the importance of the primordial continents on the origin of life, implying their existence. In this paper, we discussed the possible process that could explain the loss of the primordial continents with the assumption that they existed in the Hadean. Although depending on the timing of the initiation of plate tectonics and its convection style, subduction erosion, which is observed on the present-day Earth, might have carried the primordial continents into the deep mantle. 相似文献
10.
G. J. H. McCall 《Australian Journal of Earth Sciences》2013,60(3):349-355
An overturned angular fold in the Currabubula Formation at Tulcumba Ridge has a north‐south axial trace exposed along the western side of this ridge. The geometry and position of this fold adjacent to the Mooki Thrust is consistent with its formation as a fault‐propagation fold involving a thrust step‐up angle of ～ 30° from a décollement. Overturned strata also occur adjacent to the Mooki Thrust near the Rocky Creek Syncline to the north and to the south on Gunnan Ridge and in the Werrie Syncline. Overturning of strata in these areas may be the result of fault‐propagation folding. It is suggested that folding in the Tamworth Belt involves thin‐skinned deformation that is dominantly fault‐related. 相似文献