Kinematic peculiarities of Gould Belt stars     

V. V. Bobylev 《Astronomy Letters》2004,30(11):785-796

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Occultations of stars brighter than 15<Superscript>m</Superscript> by the largest trans-Neptunian objects in 2004–2014     

D. V. Denissenko 《Astronomy Letters》2004,30(9):630-633

We computed the occultations of stars brighter than 15^m by the largest trans-Neptunian objects (TNOs) for the next ten years. In our search, we used the following catalogs: Hipparcos; Tycho2 with the coordinates of 2838666 stars taken from UCAC2 (Herald 2003); and UCAC2 (Zacharias et al. 2003) with 16356096 stars between \(12\mathop .\limits^m 00\) and \(14\mathop .\limits^m 99\) north of ?45° declination. We predicted the occultations of stars by the seventeen largest numbered TNOs, the recently discovered 2004 DW, and four known binary Kuiper Belt objects. We selected 64 events at solar elongations of no less than 30°, including the extremely rare occultation of a \(6\mathop .\limits^m 5\) star by the double asteroid (66652) 1999 RZ₂₅₃ on October 4, 2007. Observations of these events by all available means are extremely important, since they can provide unique information about the sizes of TNOs and improve our knowledge of their orbits dramatically.  相似文献   

Ejecta exchange and satellite color evolution in the Pluto system, with implications for KBOs and asteroids with satellites     

S. Alan Stern 《Icarus》2009,199(2):571-573

In this Note, I present first-order scaling calculations to examine the efficacy of impacts by Kuiper Belt debris in causing regolith exchange between objects in the Pluto system. It is found that ejecta can escape Nix and Hydra with sufficient velocity to reach one another, as well as Charon, and even Pluto. The degree of ejecta exchanged between Nix and Hydra is sufficient to cover these bodies with much more material than is required for photometrically change. In specific, Nix and Hydra may have exchanged as up to 10s of meters of regolith, and may have covered Charon to depths up to 14 cm with their ejecta. Pluto is likely unaffected by most Nix and Hydra ejecta by virtue of a combination of dynamical shielding from Charon and Pluto's own annual atmospheric frost deposition cycle. As a result of ejecta exchange between Nix, Hydra, and Charon, these bodies are expected to evolve their colors, albedos, and other photometric properties to be self similar. These are testable predictions of this model, as is the prediction that Nix and Hydra will have diameters near 50 km, owing to having a Charon-like albedo induced by ejecta exchange. As I discuss, this ejecta exchange process can also be effective in many KBOs and asteroids with satellites, and may be the reason that very many KBO and asteroid satellite systems have like colors.  相似文献   

Geochemical, Sr–Nd and zircon U–Pb–Hf isotopic studies of Late Carboniferous magmatism in the West Junggar, Xinjiang: Implications for ridge subduction?     

Hongyan Geng  Min Sun  Chao Yuan  Wenjiao Xiao  Weisheng Xian  Guochun Zhao  Lifei Zhang  Kenny Wong  Fuyuan Wu 《Chemical Geology》2009,266(3-4):373-398

Voluminous granitic intrusions are distributed in the West Junggar, NW China, and they can be classified as the dioritic rocks, charnockite and alkali-feldspar granite groups. The dioritic rocks (SiO₂ = 50.4–63.8 wt.%) are calc-alkaline and Mg enriched (average MgO = 4.54 wt.%, Mg^# = 0.39–0.64), with high Sr/Y ratios (average = 21.2), weak negative Eu (average Eu/Eu = 0.80) and pronounced negative Nb–Ta anomalies. Their Sr–Nd and zircon Hf isotopic compositions ((⁸⁷Sr/⁸⁶Sr)_i = 0.7035–0.7042, ε_Nd(t) = 4.5–7.9, ε_Hf(t) = 14.1–14.5) show a depleted mantle-like signature. These features are compatible with adakites derived from partial melting of subducted oceanic crust that interacted with mantle materials. The charnockites (SiO₂ = 60.0–65.3 wt.%) show transitional geochemical characteristics from calc-alkaline to alkaline, with weak negative Eu (average Eu/Eu = 0.75) but pronounced negative Nb–Ta anomalies. Sr–Nd and zircon Hf isotopic compositions ((⁸⁷Sr/⁸⁶Sr)_i = 0.7037–0.7039, ε_Nd(t) = 5.2–8.0, ε_Hf(t) = 13.9–14.7) also indicate a depleted source, suggesting melts from a hot, juvenile lower crust. Alkali-feldspar granites (SiO₂ = 70.0–78.4 wt.%) are alkali and Fe-enriched, and have distinct negative Eu and Nb–Ta anomalies (average Eu/Eu = 0.26), low Sr/Y ratios (average = 2.11), and depleted Sr–Nd and zircon Hf isotopic compositions ((⁸⁷Sr/⁸⁶Sr)_i = 0.7024–0.7045, ε_Nd(t) = 5.1–8.9, ε_Hf(t) = 13.7–14.2). These characteristics are also comparable with those of rocks derived from juvenile lower crust. Despite of the differences in petrology, geochemistry and possibly different origins, zircon ages indicate that these three groups of rocks were coevally emplaced at ~ 305 Ma.A ridge subduction model can account for the geochemical characteristics of these granitoids and coeval mafic rocks. As the “slab window” opened, upwelling asthenosphere provided enhanced heat flux and triggered voluminous magmatisms: partial melting of the subducting slab formed the dioritic rocks; partial melting of the hot juvenile lower crust produced charnockite and alkali-feldspar granite, and partial melting in the mantle wedge generated mafic rocks in the region. These results suggest that subduction was ongoing in the Late Carboniferous and, thus support that the accretion and collision in the Central Asian Orogenic Belt took place in North Xinjiang after 305 Ma, and possibly in the Permian.  相似文献   

Slab-fluid metasomatism in the Early Paleozoic forearc mantle deduced from the Motai serpentinites,South Kitakami Belt,northeast Japan     

Ayaka Okamoto  Yuji Ichiyama  Akihiro Tamura  Tomoaki Morishita 《Island Arc》2021,30(1):e12387

The present study examines the petrology and geochemistry of the Early Paleozoic Motai serpentinites, the South Kitakami Belt, northeast Japan, to reveal the subduction processes and tectonics in the convergent margin of the Early Paleozoic proto-East Asian continent. Protoliths of the serpentinites are estimated to be harzburgite to dunite based on the observed amounts of bastite (orthopyroxene pseudomorph). Relic chromian spinel Cr# [=Cr/(Cr + Al)] increases with decreasing amount of bastite. The compositional range of chromian spinel is similar to that found in the Mariana forearc serpentinites. This fact suggests that the protoliths of the serpentinites are depleted mantle peridotites developed beneath the forearc regions of a subduction zone. The Motai serpentinites are divided into two types, namely, Types 1 and 2 serpentinites; the former are characterized by fine-grained antigorite and lack of olivine, and the latter have coarse-grained antigorite and inclusion-rich olivine. Ca-amphibole occurs as isolated crystals or vein-like aggregates in the Type 1 serpentinites and as needle-shaped minerals in the Type 2 serpentinites. Ca-amphibole of the Type 1 serpentinites is more enriched in LILEs and LREEs, suggesting the influence of hydrous fluids derived from slabs. By contrast, the mineral assemblage, mineral chemistry, and field distribution of the Type 2 serpentinites reflect the thermal effect of contact metamorphism by Cretaceous granite. The Ca-amphibole of the Type 1 serpentinites is different from that of the Hayachine–Miyamori Ophiolite in terms of origin; the latter was formed by the infiltration of melts produced in an Early Paleozoic arc–backarc system. Chemical characteristics of the Ca-amphibole in the ultramafic rocks in the South Kitakami Belt reflect the tectonics of an Early Paleozoic mantle wedge, and the formation of the Motai metamorphic rocks in the forearc region of the Hayachine–Miyamori subduction zone system, which occurred at the Early Paleozoic proto-East Asian continental margin.  相似文献   

The δ13C–δ18O variations in marble in the Hida Belt,Japan     

Hironobu Harada  Tatsuki Tsujimori  Keitaro Kunugiza  Katsuyuki Yamashita  Shogo Aoki  Kazumasa Aoki  Hideko Takayanagi  Yasufumi Iryu 《Island Arc》2021,30(1):e12389

Marble has a great potential to understand a history of various geological events occurring during tectonic processes. In order to decode metamorphic–metasomatic records on C–O isotope compositions of marble at mid-crustal conditions, we conducted a C–O–Sr isotope study on upper amphibolite-facies marbles and a carbonate–silicate rock from the Hida Belt, which was once a part of the crustal basement of the East Asian continental margin. Carbon and oxygen isotope analyses of calcite from marbles (Kamioka area) and a carbonate–silicate rock (Wadagawa area) show a large variation of δ¹³C [VPDB] and δ¹⁸O [VSMOW] values (from −4.4 to +4.2 ‰ and +1.6 to +20.8 ‰, respectively). The low δ¹³C values of calcites from the carbonate–silicate rock (from −4.4 to −2.9 ‰) can be explained by decarbonation (CO₂ releasing) reactions; carbon–oxygen isotope modeling suggests that a decrease of δ¹³C strongly depends on the amount of silicate reacting with carbonates. The occurrence of metamorphic clinopyroxene in marbles indicates that all samples have been affected by decarbonation reactions. All δ¹⁸O values of calcites are remarkably lower than the marine-carbonate values. The large δ¹⁸O variation can be explained by the isotope exchange via interactions between marble, external fluids, and/or silicates. Remarkably low δ¹⁸O values of marbles that are lower than mantle value (~+5 ‰) suggest the interaction with meteoric water at a later stage. Sr isotope ratios (⁸⁷Sr/⁸⁶Sr = 0.707255–0.708220) might be close to their protolith values. One zircon associated with wollastonite in a marble thin-section yields a U–Pb age of 222 ± 3 Ma, which represents the timing of the recrystallization of marble, triggered by H₂O-rich fluid infiltration at a relatively high-temperature condition. Our isotope study implies that the upper amphibolite-facies condition, like the Hida Belt, might be appropriate to cause decarbonation reactions which can modify original isotope compositions of marble if carbonates react with silicates.  相似文献   

贺兰山构造带及邻区中-新生代构造事件:来自不整合面和裂变径迹的约束   总被引：1，自引：1，他引：0  

马静辉  何登发 《岩石学报》2019,35(4):1121-1142

贺兰山构造带及邻区的构造属性长期以来存在争议,确定该地区中新生代的构造事件及隆升过程是了解这一重要陆内变形带动力学机制的关键所在。本文采用不整合面分析法和低温热年代学方法,综合分析探讨了贺兰山构造带及邻区中新生代的构造事件及其构造演化过程。通过对该地区的野外地质调查,本次在中-新生代地层中由底到顶识别出6个不同类型的不整合面,它们分别是:(1) T_(2-3)/P平行不整合面;(2) J/AnJ角度不整合面-微角度不整合面;(3) K_1/AnK_1高角度不整合面;(4) E_3q/AnE_3;(5) N_1/AnN_1;(6) Q/An Q。在T_3d~3、J_2y和K_1变形前锋,可见与逆冲-褶皱造山带相关的同构造沉积生长地层,其在形态上表现为超覆、削截,在黄草滩等地局部与倒转背斜相伴生。这些不整合和生长地层是构造活动的直接证据。本次研究对采自该地区的12件样品分别进行了磷灰石、锆石裂变径迹测年及热史模拟分析。结果表明,裂变径迹年龄主要分布在4个区间,对应地质时代分别为中侏罗世-晚侏罗世(168～159Ma)、早白垩世末(139～91Ma)、晚白垩世末(79～66Ma)、始新世(59～50Ma),反映出该地区在这4个时期发生了明显的冷却抬升事件,且这4期构造事件与野外观察到的地质特征有很好的地质响应。同时,热史模拟表明该地区整体上经历了晚侏罗世、早白垩世、晚白垩世末-始新世3期快速隆升事件。综合研究表明,该地区主体逆冲褶皱的时间是从中侏罗世开始,早白垩世末构造运动最强烈,新生代又有所活动。  相似文献   

长江中下游成矿带钨矿床   总被引：5，自引：1，他引：4  

周涛发  聂利青  王世伟  汪方跃  张千明 《岩石学报》2019,35(12):3592-3608

长江中下游成矿带是我国重要的铜-铁-金多金属成矿带,近年来在长江中下游成矿带内发现多处白钨矿床和矿化点,为该成矿带的成矿学研究提供了新的研究课题。相比成矿带铜铁金多金属矿床研究程度,钨矿床成矿作用研究明显薄弱,尚未进行系统的成矿作用和成矿规律总结。成矿带内发育的钨矿床主要为北亚带的东顾山矿床、主带(中亚带)的阮家湾矿床和南亚带的桂林郑矿床和高家塝矿床。本文对这四个钨矿床及几个含钨矿床的地质和地球化学特征、成岩成矿时代、成矿岩体地球化学特征等方面的研究资料和成果进行了总结,讨论和试图阐明长江中下游成矿带钨矿床的成矿作用。研究显示,长江中下游成矿带存在三期钨成矿作用,分别为146～143Ma、127Ma和97Ma,在成矿带的铜主成矿期前和铁成矿期均有钨成矿作业发生。钨矿床中白钨矿的Sr-Nd同位素组成分别落入董岭式基底或江南式基底范围,表明长江中下游成矿带的董岭式和江南式基底是形成原始含矿岩浆的物质基础。长江中下游成矿带的钨矿床成矿岩体为中酸性岩,ε_(Hf)(t)值很低,且Zr/Hf、K/Rb比值小,表明成钨岩浆岩为古老地壳物质重熔并经历了较充分的分异演化,对比成矿带中成铜、成铁岩体,源区性质可能是导致长江中下游成矿带金属成矿差异的根本原因。燕山期的陆内俯冲是造成长江中下游成矿带钨矿床成矿的主导机制。  相似文献   

Convergence History of the Songliao and Jiamusi Blocks in the Eastern End of Central Asian Orogenic Belt: Evidence from Detrital Zircons of Late Paleozoic Sedimentary Rocks   总被引：1，自引：0，他引：1  

CHEN Zhaoxu  LIU Yongjiang  GUAN Qingbin 《《地质学报》英文版》2019,93(5):1417-1433

Central Asian Orogenic Belt(CAOB) is one of the largest accretionary orogenic belts in the world. The eastern segment of CAOB is dominated by Paleozoic Paleo Asian Ocean tectonic regime, Mesozoic Paleo-Pacific tectonic regime and Mongolian-Okhotsk tectonic regime. The Songliao and Jiamusi blocks are located in the easternmost part of the CAOB and are the key region to solve the problem about overprinting processes of multiple tectonic regimes. It is generally believed that the Mudanjiang Ocean between the two blocks was finally closed in the Mesozoic, but the Paleozoic magmatism also developed along the Mudanjiang suture zone, while on both sides of the suture zone, there were comparable Paleozoic strata, indicating that the two blocks had converged during the Paleozoic, and the evolution history of the two blocks in the Late Paleozoic remains controversial. The Carboniferous-Permian terrestrial strata mainly developed in Binxian, Wuchang and Tieli on Songliao Block, Baoqing and Mishan on Jiamusi Block. Samples from the Songliao and Jiamusi blocks in the Late Carboniferous-Early Permian and Late Permian are collected for comparative analysis. The LAICP-MS zircon U-Pb dating results show that the maximum depositional age of Middle Permian Tumenling Formation and Late Permian Hongshan Formation in Songliao Block is ～260 Ma, while that of Tatouhe Formation and Carboniferous strata in Jiamusi Block are ～290 Ma and ～300 Ma, respectively, which supports the previous stratigraphic division scheme. The age peaks of ～290–300 Ma, ～400 Ma, ～500 Ma appeared in the Late Carboniferous to Early Permian strata of Jiamusi Block and the Middle Permian strata of Songliao Block. The age peak of ～500 Ma in the Middle Permian strata of Songliao Block may come from the Cambrian basement, Mashan Complex, of Jiamusi Block, while the age peaks of ～420–440 Ma in the Carboniferous strata of Jiamusi Block may come from the Silurian magmatic arc in Zhangguangcai Range in the eastern margin of Songliao Block, reflects the history that they had been potential sources of each other, indicating that they may have combined in the Paleozoic. The Hongshan Formation of Songliao Block in the Late Permian lacks the age peak of ～500 Ma, which indicate that Jiamusi Block was not the provenance of Songliao Block in the Late Permian, that is, there was a palaeogeographic isolation between the two blocks. Combined with the ～210 Ma bimodal volcanic rocks developed along the Mudanjiang suture zone reported previously, we believe that the oceanic basin between the Songliao and Jiamusi blocks should have been connected in Late Permian and reopened during Late Permian to Late Triassic.  相似文献   

Final Closure Time of the Paleo‐Asian Ocean: Implication from the Provenance Transformation from the Yangjiagou Formation to Lujiatun Formation in the Jiutai Area,NE China   总被引：1，自引：0，他引：1  

ZHANG Qian  LIANG Chenyue  LIU Yongjiang  ZHENG Changqing  LI Weimin 《《地质学报》英文版》2019,93(5):1456-1476

The Jiutai area is tectonically situated at the eastern segment of the Central Asian Orogenic Belt(CAOB) and is close to the North China Craton(NCC) to the south, serving as an ideal place to investigations of the closure of the PaleoAsian Ocean(PAO). Sandstone samples collected from the Yangjiagou Formation and the Lujiatun Formation in this area have been studied in detail in terms of petrology, geochronology and geochemistry. The maximum depositional time of the Yangjiagou and Lujiatun formations has been constrained to early Middle Triassic(ca. 245 Ma) and middle Late Triassic(ca. 219 Ma), respectively. The Yangjiagou Formation, with a major provenance of dissected island arcs, is dominantly composed of Phanerozoic sediments from Northeastern China(NE China) massifs. The Lujiatun Formation, with major sediments from active continental margins, has a relatively larger proportion of Precambrian sediments, in which the ～1.85 Ga and ～2.5 Ga sediments are typical of the crystalline basements of the NCC and NE China massifs, which were uplifted and eroded during the closure of the PAO. Besides, both formations show the enrichment in LREEs and the depletion in HREEs, the common Eu negative anomalies, and trace element contents similar to that of the upper continental crust. Based on the provenance analysis of these two formations, the final closure time of the PAO in this area is constrained as from the early Middle Triassic(ca. 245 Ma) to the middle Late Triassic(ca. 219 Ma).  相似文献