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1.
太阳星云凝聚过程的岩石学模型：（1）球粒陨石的凝聚成因 总被引：2，自引：2，他引：2
建立类地行星区太阳星云凝聚过程的岩石学模型，对于合理解释陨石、地球和类地行星的成因关系，探讨地球起源和估算地球的整体成分都有着重要意义。本文中根据天体化学和太阳系演化学说关于太阳星云物理化学条件的基本分析，以及实验凝聚岩石学的研究结果，推断在太阳星云盘的类地行星区中可能有星云的气－固和气－液－固两种凝聚作用发生。通过对球粒陨石中球粒和基质矿物成分及结构构造特征的对比，论证了绝大多数球粒的气－液－固凝聚成因和基质的气－固凝聚成因，并讨论了球粒陨石各化学群的凝聚成因模式。 相似文献
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近年来有关太阳系天体中等挥发性元素的研究掀起了一波浪潮。锌作为中等挥发性元素,其稳定同位素对于高温挥发过程具有很好的指示作用。因此,在行星科学领域锌同位素逐渐成为研究星云和行星演化的一个理想工具。本文系统地归纳了各类陨石和行星天体储库的锌同位素组成,并对不同种类的陨石以及地外样品(碳质球粒陨石、普通球粒陨石、顽火辉石球粒陨石、橄辉无球粒陨石、铁陨石、石铁陨石、月球陨石和Apollo样品、火星陨石、灶神星陨石等)中的锌稳定同位素研究内容进行了较全面的总结。主要包括不同陨石和行星锌同位素组成的控制因素以及锌同位素对太阳系内星云过程和行星过程的指示;同时,简要论述了锌同位素在太阳系形成和演化过程中的分馏机制,并立足目前的研究基础,探讨锌同位素在行星科学领域的研究前景和发展趋势。 相似文献
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陨石是来自含气体-尘粒的太阳早期星云盘凝聚和吸积的原始物质,大多数原始物质因吸积后的作用过程而改变（如月球、地球及火星样品）,但有一些却完整的保存下来（如球粒陨石或球粒陨石中的难熔包体）。这些原始的物质通常依据同位素丰度特征来识别,依据其矿物-岩石学特征和成因可将已知的陨石划分许多更小的类型。陨石学及天体化学的新近进展包括：新近识别的陨石群;发现新类型球粒陨石及行星际尘粒中发现前太阳和星云组分;利用短寿命放射性核素完善了早期太阳系年代学;洞察宇宙化学丰度、分馏作用及星云源区及通过次生母体的作用过程阐释星云和前星云的记录。本文概述了早期太阳系内从星云到陨石的演化过程。依据这些资料,对早期太阳系所经历的多种核合成的输入、瞬时加热事件与星云动力学有一些新的认识,以及认识到小星子和行星体系的演化比以前预期的更快速。 相似文献
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造山带火山岩研究 总被引：17，自引：4，他引：17
造山带火山岩石学研究的主要目的在于重溯造山带的构造－岩浆演化历史。纵观我国以至全球的大陆造山带形成、演化历史，一个造山带往往经历了古大陆裂解、洋陆转换、陆块拼合－碰撞、陆内伸展－盆山耦合和新构造隆升（陆内造山）等众多不同的构造演化阶段，这些不同的构造演化阶段和不同的构造环境均有特定火山岩浆作用与这相伴。因此，可以根据造山带形成、演化不同阶段火山岩浆作用的特点来重溯造山带的构造－岩浆演化历史，进而从更大尺度上加以对比，探索全球动力学乃至比较行星动力学等重大科学问题。本文对造山带火山岩石学研究中的一些重要问题进行了讨论和评述，这些问题包括：板块内部火山岩浆活动、离散板块边界上的火山岩浆活动、会聚板块边缘的火山岩浆活动。 相似文献
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造山带火山岩浆作用 总被引：9，自引：2，他引：9
造山带火山岩石学研究的主要目的在于重溯造山带的构造－岩浆演化历史。纵观我国到至全球的大陆造山带形成－演化历史，一个造山带往往经历了古大陆裂解，洋陆转换，陆块拼合，碰撞，陆内伸展－盆山耦合和新构造隆升（陆内造山）等众多不同的构造演化阶段，这些不同的构造演化阶段和不同的构造环境均有特定火山岩浆民之相伴。因此，我们可以根据造山带形成－演化不同阶段火山岩浆作用的特点来重溯造山带的的构造－岩浆演化历史，并进而从更大尺度上加以对比，探索全球动力学乃至比较行星学等重大学问题。本文对造山带火山岩石学研究中的一些重要问题进行了讨论和评述，这些问题包括有：板块内部火册浆活动，离散板块边界上的火山岩浆活动，会聚板块边缘的火山岩浆活动。 相似文献
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普通球粒陨石是目前发现数量最多的陨石,对认识早期太阳星云演化和太阳系物质成分具有重要的意义。Northwest Africa (NWA) 15004是一块非洲西北部新发现的普通球粒陨石。本次研究使用光学显微镜、电子探针以及扫描电镜等分析仪器对该陨石进行详细的岩石学、矿物学及球粒特征研究。结果表明该陨石球粒轮廓较为模糊,基质重结晶明显,橄榄石平均Fa值为25.4 mol%(PMD为2.65%),低钙辉石的平均Fs值21.3 mol%(PMD为3.95%),硅酸盐矿物化学成分较为均一,根据岩相学及矿物学特征将其划分为L5型普通球粒陨石。橄榄石和辉石颗粒发育波状消光和面状破裂,且观察到有熔融囊的出现,表明该陨石受到S3以上的冲击变质作用。球粒的成因和形成的星云环境需要准确的球粒类型划分,球粒按结构类型分类较多,但其化学成分均一,该陨石所有球粒的橄榄石辉石的Mg#约为74.5,均为Ⅱ型富铁球粒,结合“CIPW标准”计算基质化学成分均为A5型球粒。利用共生单斜辉石和斜方辉石矿物对成分特征计算得到NWA 15004陨石热变质平衡温度为814℃,说明该陨石母体经历了较高程度热变... 相似文献
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类地行星挥发性元素普遍亏损很可能是由于太阳星云早期剧烈的太阳活动引起的。当气体、尘粒、挥发性元素和水被驱赶出内太阳系时，只有米级到公里级的物质保存下来并堆积成星子，最终吸积星子形成类地行星。我们认为类地行星的初始物质主要是已分异的星子和一些未分异的球粒陨石质星子或不同类型的陨石母体，最靠近太阳形成的星子具有最低的ＦｅＯ／（ＦｅＯ＋ＭｇＯ）值，水星是在靠近太阳的高度还原条件下吸积成分类似ＥＨ球粒陨石的星子形成的。地球的初始物质为分异的铁陨石及Ｈ群球粒陨石。随着距太阳距离增大及温度降低，陨石形成的部位大致为：ＥＨ、ＥＬ－ＩＡＢ－ＳＮＣ（辉玻无球粒陨石、辉橄无球粒陨石、纯橄无球粒陨石）－Ｅｕｃ（钙长辉长无球粒陨石）－Ｈ、Ｌ、ＬＬ－ＣＶ、ＣＭ、ＣＯ－Ｃｌ－彗星。物体之间、星子之间及行星与星子之间的碰撞对太阳系的形成和演化起着重要的作用。 相似文献
11.
Genetic types of diamond mineralization 总被引：1，自引：0，他引：1
A. A. Marakushev Sang Longkang You Zhendong I. A. Zotov N. N. Pertsev N. A. Paneyakh 《中国地球化学学报》1998,17(1):12-28
The paper describes the proposed models of diamond formation both in meteorites and in kimberlite and lamproite bodies, metamorphic
complexes and explosive-ring structures (“astroblemes”). The diamond distribution in meteorites (chondrites, iron meteorites
and ureilites) is restricted to taenite-kamasite phase. The diamond generation here is tied up with the first stage of evolution
of the planets. This stage is characterized by high pressure of hydrogen, leading to the formation of the planet envelope.
The second stage of planet evolution began with the progressive impoverishment of their atmospheres in hydrogen due to its
predominant emission into the space and to progressive development of oxidative conditions. The model appears to have proved
the relict nature of diamond mineralization in meteorites.
Diamond and other high-pressure minerals (its “satellites”) were crystallized without any exception in the early intratelluric
stages of peridotite and eclogite-pyroxenite magma evolution just before the magma intrusion into the higher levels of the
mantle and crust where diamond is not thermodynamically stable. The ultramafic intrusive bodies (bearing rich relict diamonds)
in the base of a platform appear to be the substrata for the formation of kimberlite-lamproite magma chambers as a result
of magmatic replacement. The model explains the polyfacial nature of diamondiferous eclogites, pyroxenites and peridotites
and discusses the process of inheritance of their diamond mineralization by kimberlites and lamproites.
Diamond productivity of metamorphic complexes is originated by the inheritance of their diamonds from the above-mentioned
primary diamondiferous rocks. Large diamondiferous explosive-ring structures were formed by high-energy endogenic explosions
of fluid which came from the Earth’s core. This high energy differs endogenic impactogenesis from explosive volcanism. It
proceeds at very high temperature to create diaplectic glasses (monomineral pseudomorphs) —the product of isochoric melting,
at the pressure high enough for the stable formation of very high-density minerals (coesite, stishovite, diamond, lonsdaleit,
and chaoite).
The research project was financially supported by the Russian Foundation of Fundamental Sciences (93-05-8566, 96-05-64307,
and 96-05-00026c0) and China National Natural Science Foundation (No.49794041, No.49611121831). 相似文献
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《International Geology Review》2012,54(4):504-519
ABSTRACTThe preservation of metastable diamond in ultrahigh-pressure metamorphic (UHPM) complexes challenges our understanding of the processes taking place during exhumation of these subduction zone complexes. The presence of diamonds in UHPM rocks implies that diamonds remained metastable during exhumation, and within thermodynamic stability of graphite for an extended period. This work studies the influence of pressure on the surface graphitization rate of diamond monocrystals in carbonate systems to understand the preservation of microdiamond during exhumation of UHP subduction complexes. Experiments were performed with 2–3 mm synthetic diamond monocrystals at 2–4 GPa in СаСО3 (1550°С) and К2СО3 (1450°С) melts using a high-pressure multi-anvil apparatus. The highest rate of surface graphitization took place at 2 GPa; diamond crystals were almost completely enveloped by a graphite coating. At 4 GPa, only octahedron-shaped pits formed on flat {111} diamond crystal faces. Our results demonstrate that the surface graphitization rate of diamonds in the presence of carbonate melts at 1450–1550°C increases with decreasing pressure. Decreased pressure alone can graphitize diamond regardless of exhumation rate. Metastable diamond inclusions survive exhumation with little or no graphitization because of excess pressure up to 2 GPa acting on them, and because inclusions are protected from interaction with C-O-H fluid. 相似文献
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Chepurov A. I. Zhimulev E. I. Sonin V. M. Tomilenko A. A. Pokhilenko N. P. 《Doklady Earth Sciences》2018,480(2):823-825
The first results are presented for the synthesis of diamond at 6.5 GPa and 1600°C during migration of molten iron through a silicate matrix, which is composed of olivine crystals with interstitial graphite. The experiment shows that diamonds in the Earth’s mantle and the terrestrial planets could have formed during differentiation. Diamond crystals, which were formed during iron segregation of the Earth’s differentiation, could be centers for further crystallization of mantle diamonds.
相似文献14.
对不同类型褐色钻石进行高温高压处理和结构特性研究是钻石研究中的难点和重点之一。前人对富氢钻石的研究主要集中于其特殊的生长结构以及其形成环境的探讨,而对富氢钻石经高温高压处理后的变化特征鲜有涉及。本文对经高温高压处理前后的富氢钻石的红外光谱、紫外可见吸收光谱以及光致发光光谱等谱学特征进行了对比,研究其鉴定特征。结果表明:高温高压处理前后的富氢钻石的光谱特征具有明显差异,特别是红外光谱,经处理后的钻石中与氮氢有关的吸收峰如3310 cm~(-1)、3232 cm~(-1)、3189 cm~(-1)等明显减弱甚至消失,并出现与孤氮有关的新的2688 cm~(-1)吸收峰;紫外可见光吸收光谱中,经处理的褐色钻石中的无选择性吸收(钻石呈褐色的原因)变为孤氮的典型吸收,即550 nm至短波的吸收以及N_3中心(415 nm)的吸收均明显增强,因此钻石也由原来的褐色变为黄色。钻石经处理前后的光致发光光谱中,与氮原子有关的缺陷类型、峰的强度以及缺陷组合也有变化。本文获得的光谱变化特征,为准确鉴定高温高压处理的黄色富氢钻石提供了依据,也为解释与氢和氮相关的晶格缺陷在高温条件下的变化机理提供了理论基础。 相似文献
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哈萨克斯坦北部Kumdy-Kol金刚石矿床地质与变质金刚石成因 总被引：1，自引：0，他引：1
Pavel NITSENKO 《地学前缘》2004,11(2):333-338
哈萨克斯坦北部Kokchetav地区的Kumdy Kol金刚石矿床是世界上惟一的变质金刚石矿床。对该金刚石矿床成因以及相关岩石的诸多研究成果不仅深化了对超高压变质岩的研究 ,而且推动了大陆动力学研究的进展。在该金刚石矿床中找到的岩相学证据证明 ,该金刚石矿床的主要含矿岩石大理岩曾经在俯冲带中循环到 >2 4 0km的深部。文章在介绍Kokchetav变质金刚石矿床的地质特征和大地构造背景的基础上 ,讨论了该变质金刚石矿床的形成过程以及变质金刚石的成因。Kokchetav变质金刚石主要表现出蜂窝状或草莓状的特征外形。这种蜂窝状或草莓状金刚石是快速生长条件下结晶的结果。结合最近的研究成果 ,笔者认为Kokchetav金刚石矿床中金刚石的形成与深俯冲大理岩中的白云石分解作用密切相关。白云石分解反应形成文石和菱镁矿组合 ,菱镁矿继续分解形成金刚石 (MgCO3 =金刚石 +MgO +O2 )。基于这个认识 ,Kokchetav金刚石矿床中碳 (金刚石和石墨 )的来源应该是碳酸盐岩 相似文献
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安徽铜陵典型矿区岩石包体研究及其岩浆——成矿作用过程探讨 总被引：27，自引：2，他引：25
铜陵地区岩浆岩中产有两类石包体,一类为属高于高角闪岩相的变质岩（残余）包体;另一类为属于二长岩－闪长岩类的岩浆岩包体,对这两类岩石包体进行了详细的岩石学和矿物学研究,并计算了了各类岩石包体的形成条件,在此基础上探讨了岩石包体与寄主岩浆岩之间的关系,分析了岩浆岩和有关矿床的物质来源和成岩成矿作用机制,提出了深部古老变质基底部分融－岩浆积聚,分异,并在不同层位就形,形成深位和浅位岩浆房－不同成分的岩浆混合－气液隐爆迁移沉淀这样一种与同熔型岩浆岩有关的新的层控矽卡岩矿床成矿模式。 相似文献
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变质核杂岩与岩浆作用成因关系综述 总被引：12，自引：0，他引：12
对岩浆与伸展作用的关系、伸展作用中岩浆的成因和需加强的工作进行了讨论,并重点论述了变质核杂岩形成机制与侵入作用的关系。在造山带重力势能差和深部作用等各种因素导致的拉伸应力场作用下,岩石圈地幔和地壳通过减压或深部热活动发生部分熔融而形成岩浆,岩浆的上涌强化了地壳伸展,对地壳的弱化作用触发伸展构造的发生。岩浆作用是变质核杂岩形成的主导因素之一,其主要包括对地壳的加热、弱化导致拆离断层的形成及由其浮力和密度产生不均一隆升而形成穹隆。 相似文献
18.
The paper presents the results of a comprehensive mineralogical study, including IR and UV spectroscopy, of diamonds and related solid inclusions from kimberlitic bodies and veins located adjacent to the Yubileinaya pipe, the largest (59 ha) in the Siberian Platform. This pipe is characterized by a complex structure with diatreme and crater facies of kimberlitic magmatism. The typomorphic features of diamonds from the Ozernaya kimberlitic pipe, Pervomaiskaya and Novogodnyaya veins, and Ottorzhenets kimberlitic body, as well as the Carboniferous-Permian terrigenous sedimentary rocks that overlie the Yubeleinaya pipe, are described and compared with those of the Yubileinaya pipe. The typomorphic features of diamonds from the earliest phase of kimberlitic magmatism are emphasized. Diamonds from the Ozernaya pipe are similar to those from the Komsomol’skaya pipe, which is characterized by a low content of typical round crystals and a high content of eclogite-type inclusions in high-quality diamonds of variety I after Yu.L. Orlov. The typomorphic and genetic features of diamonds testify to the multiphase nature of the kimberlitic magmatism of Middle Paleozoic age (about 360 Ma ago). These features are discussed in terms of variation in diamond genesis and types of this mineral. 相似文献
19.
Afanasiev V. P. Pokhilenko N. P. Egorova E. O. Lindenblot E. S. 《Doklady Earth Sciences》2019,489(2):1409-1412
Doklady Earth Sciences - Based on a study of diamond grains from placers of the northeastern Siberian Platform, it is shown that certain types of diamonds (rounded dodecahedroids, diamonds of the... 相似文献
20.
《International Geology Review》2012,54(6):545-554
Octahedral, tetrahedral, and cubic forms of graphite, interpreted here as pseudomorphs after diamond, have been discovered in situ in crustal metamorphic rocks from central Macedonia, northern Greece. Several types of rocks, mainly of sedimentary origin, including eclogite, phyllite, quartzite, schist, and amphibolite, have been identified as hosts to inferred diamonds. All assemblages are invariably graphitic and retrograded under greenschist-facies metamorphism. The graphitized diamonds themselves occur as inclusions in garnet, quartz, amphibole, and graphite, and range in size from approximately 2 to 300 μm. In marked contrast with previously published Raman spectra of graphitized diamonds from crustal metamorphic rocks, the Raman spectra of the Greek specimens indicate very poor carbon crystallinity. This probably resulted from a rapid phase transition induced by high contact compressive stress (i.e., non-hydrostatic pressure) at ultradeep shear zones and subsequent rapid pressure release. The presence of former microdiamonds invalidates previous models on the geotectonic evolution of the Internal Hellenide zones, and demarcates a new ultrahigh-pressure zone, the width of which is currently uncertain, and which probably represents a Late Paleozoic suture marking the collision of individual continental blocks of unknown provenance. 相似文献