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1.
Instrumental neutron activation analysis(INAA) of 14 single oldhamite grains separated from the Qingzhen chondrite (EH3) for refractory(La,Ce,Sm ,Eu,Yb,Lu,Ca,Sc,Hf, and Th),volatile (Na,Cr,Zn,Se,Br,etc.)and siderophile elements (Fe,Ni,Co,Ir,Au ,and As) revealed that oldhamite is highly rich in refractory elements.The mineral serves as the principal carrier of REE and contains about 80% of the REEs in the Qingzhen enstatite chondrite .Furthermore, the large enrichment of LREE relative to HREE is noticed in oldhamite from the Qingzhen .In general, the oldhamite from metal-sulfide assemblages is richer in REE than that from the matrix,i.e.,the earlier the oldhamite grains condensed, the richer they are in REE. Meanwhile.oldhamite is also rich in vol-atile elements such as Se,Br, etc.In terms of the distribution of trace elements in oldhamitc from the Qingzhen ,the chondrite is srggested to have resulted from high-temperature condensation of solar nebula.  相似文献   

2.
The Ningbo iron meteorite fell near Ningbo, Chekiang province, on October 4,1975. 103 days later, γ-ray spectrum of the meteorite, was undestructively measured by a low-level γ-ray spectrometer. It is shown that the specific activity of Mn^34 present in the Ningbo iron meteorite is ap proximately close to that of Mn^34 in the Bogou and Aroos meteorites, while the specific activity of Co^37 seems to be higher in the Bogou and Aroos than in the Ningbo.  相似文献   

3.
Based on structural observations and the concentrations of Cr, Co, Ni, Cu, Ga, Ge,As, Sb, Re, Ir and Au by neutron-activation analysis we have classified 14 Chinese iron meteorites. Thirteen are members of the large groups IAB, IIICD, IIICD,IIIAB and IVA.Leshan is an ungrouped iron meteorite that falls within the IIE field on some elementNi diagrams, but is distinctly outside this .fiel on plots of Cu, W, and Ir vs. Ni; it is very similar in Composition to Techado,another ungrouped iron. The high Cu content of Leshan is consistent with other evidence indicating that Cu is a valuable parameter for classifying, iron meteorites. IIICD Dongling appears not to be a new meteorite, but to be paired with Nantan; Dongling was recovered about 50 km from the location of the Nantan shower. Yungning is highly oxidized; we assign it to group LAB but cannot rule out IIICD. IVA-An Longchang has many characteristics of IVA irons, but has been remelted, prebably in a terrestrial setting, Five irons belong to group IVA, a remarkably large number. Three are identical in Composition, and we suspect that the two from Hubei, Guanghua and Huangling, are paired. Thus this set of 14 irons ineludes 12 independent fall.  相似文献   

4.
Polarization and radiation measurements and microwave studies show that the planets and the great majority of asteroids in the solar system are covered by soils similar to regolith on the moon surface.The soils repesent the composition of the asteroids and the geological elements of the planets. The spectral reflectance shows a tendency of decreasing from near ultraviolet,visible to near-infrared in order of LL→L→H→H with increasing Fe^0/Fet rato and toward to absorption for Jilin,Xinyang and Zanoyang ordinary chondrites and Qinzhen enstatite chondrite recently fallen in China,The same chemical group of meteorites feature deeper absorption valleys with increasing metamorphic grade.The spectal reflectance of igneous rocks varies from strong to what is like that of H-group chondrites in order of acid→basic→ultrabasic rocks.  相似文献   

5.
This paper deals with the effects of thermal and collision events which had been experienced by the Jilin(H5) and Qingzhen(EH3) chondrites before they fell to the earth .The HRTEM and opti-cal microscopic investigations show that the Jilin chondrite has undergone more extensive thermal heating and two stages of collision,while the Qingzhen chondrite has experienced weak thermal events after the accretion of its parent body and one stage of moderate collision.The schematic dia-grams of the process of formation and evolution of these two meteorites are given in the present pa-per.  相似文献   

6.
Iron meteorites from Nandan, Guangxi ; Wushike, Xinjiang; Shangdu, Hebei and Huangling, Hubei are investigated with a spark souree mass speetrometer for their Cr, Ni, Co, Cu, Zn, Ga, Ge, As, Mo, Ru, Rh, Pd, Os and Ir contents. The accuracy of the results and the factors affecting it are discussed. It is preliminarily concluded,while textural evidences of these meteorites are also taken into account, that the Nandan, Wushike and Shangdu meteorites belong to IA, Ⅲ .4 and ⅢE groups respectively. The Ni, Ga and Ge contents in the Huangling iron meteorite come close to that of mesosiderites.  相似文献   

7.
Preliminary results of our study an ancient meteorite records by the end of the Ching dynasty are presented in the present paper. Early in 645 B.C. there were formal records on meteorite falls and cosmoganesis of meteorites. The utinization of iron meteorites for making weapons alloyed with bronze has a history of more than 3000 years (in the Shang and Zhou dynasties). By the time of 1064 (in the Sung dynasty) iron meteorites were well doeum anted. The geographical distribution and falling time of meteorites are also mentioned. The maximum number of meteorite falls was recorded in May and June against the minimum number in December in a year.33 serious calamities caused by meteorite f alls themselves, and several interesting records on meteorite falls are also described in this paper.  相似文献   

8.
Petrography and mineral chemistry of 24 ordinary chondrites from the Grove Mountains, Antarctica, have been studied in order to identify their chemical-petrographic types. These samples were selected from a total of 4448 Grove Mountains (GRV) meteorites collected during the 19th Chinese Antarctic Research Expedition so as to make an estimation of the large GRV meteorite collection. The chemical-petrographic types of these meteorites are presented below: 1 H3,2 H4, 4 H5, 2 H6, 1 L4, 7 L5, 5 L6, 1 LL4 and 1 LL6. The new data weaken the previous report that unequilibrated ordinary chondrites are unusually abundant in the Grove Mountains region. However, this work confirms significant differences in distribution patterns of chemical-petrographic types between the Grove Mountains and other  相似文献   

9.
Huhehu Sag is a new battlefield for the future oil and gas exploration in the Hailar Basin. At present, exploration of this area stays at a low level and the understanding of the provenance system of the Nantun Formation is comparatively weak. So, to carry out the detailed depiction of the provenance system in the study area is significant for the sedimentary system reconstruction, for the prediction of reservoir distribution and favorable areas. Based on comprehensive analysis of paleogeomorphy, light-heavy mineral and seismic reflection features, sandstone thickness and sandstone percentage, this paper analyzes in detail the provenance system of the Nantun Formation in Huhehu Sag from various angles and levels. It shows that provenances of the Huhehu Sag mainly originated from the eastern Xilinbeier Salient and western Bayan Mountain Uplift. The provenances surrounding the lake basin converged to the center of the basin, among which, the steep slope belt and the gentle slope belt are the main provenances, and the southern uplift is a secondary one. The distribution framework of the provenance fundamentally determines the distribution rules of the depositional system and its sand body developing during the Nantun period.  相似文献   

10.
广西南丹铁陨石雨的发现   总被引:1,自引:0,他引:1  
The distribution and exterior characters of each individual meteorite are presented for the iron meteorite shower in Nantan County, Kwangsi Chuang Autonomous Regiou,China. Nineteen iron meteorites have been found up to date, umounting approximately to 9,500 kg in total weight and spreading over an area of about 30 square kilometers. As compared with other iron meteorites known in China, they are much larger in size and contuin much more mineral species. It is also interesting to note that a complete sample of various parts of a primitive meteorite can be expected. The discovery of this meteorite shower is considered to be of significant value in science.  相似文献   

11.
Cosmogenic radioactive nuclides, particularly K^40, Mn^54 and Co^57 are measured in meteorites Nos. Ⅰ,Ⅱ and Ⅴ from the Kirin meteorite shower which is very seldom to be met with in world history in the sense of its scale. Brief accounts are given of the distribution of cosmogenic nuclides with depth, the characteristics of cosmicray induced reactions and that of target nuclides, the energy region of bombarding particles, and the relative positions of meteorites Ⅰ,Ⅱ and Ⅴ with respect to the original meteoroid. The variations in Mn^54, Co^57 and K^40 with depth in No. I Kirin meteorite provides an excellent example for studies in this field.  相似文献   

12.
comparatively evident chondritie structure is observed in the Jilin meteorite. Chondrules range from 0.2 to 3mm in diameter, averaging 0.6mm. Chondrules can be divided into the following types according to the principal minerals crystallized and structure-texture characteristics: (1) Olivine chondrules. In terms of their structure they can be subdivided into prophyritic, grated, barred, sub swirlling internal flow and granular chondrulcs; (2) Orthopyroxene ahondrules. Textural types found are fan-like, radial,parallel fibrous, porphyritic and irregular; (3) Olivineorthopyroxene chondrules; (4)Glass or devitrified chondrules; (5) Ni-Fe chondrules and (6) Troilite-olivine chondrules. Among them, porphyritic and granular olivine chondrules and various kinds of radial orthopyroxene chondrules are most common. In addition, also have been recognized the overlapping of two or more chondrules and chondrules coated with glassy crust. The structure and texture of chondrules indicate that they were originated from molten silicate droplets through rapid cooling prior to the formation of the meteorite parent body. Rapid fusion may be induced on the surface of a few solidified chondrules by solar impulse wave or nebula lightning and, if rapid cooling followed, this would give rise to the appearance of glassy crust. Collision between chondrulcs may result in a variety of chondrule fragments and crystal debris. In some cases, collision is also considered to be responsible for the entrench, inclusion and overlapping textures in ehondrules. After the formation of the meteorite parent body recrystallization of chondrules may take place as a result of thermal metamorphism.  相似文献   

13.
The Indus River flows through Ladakh, one of the driest and coldest places on earth, in a tectonically active domain. Fluvial, glaciofluvial, lacustrine and debris dominated sequences represent the Late Quaternary sedimentary record along the river course. Karakoram Fault, a major crustal scaled feature reported to be active during the Quaternary, is associated with the Indus River drainage. Linkages between a major, active fault and deposits formed during the activity period of the fault are explored using heavy mineral deduced provenance and Optically Stimulated Luminescence(OSL) chronology.Five deposits in a ~200 km long stretch of the Indus River have been examined for a ~80 ka period to decipher the climate linked aggradation history. Damming of the Indus River at ~79 ka and existence of the Spituk Lake for >30 ka is demonstrated. Using geology of the provenance in relation to the mineralogical attributes of the Quaternary deposits, the major drainage reorganization when the connection of the Tangtse Valley to the Indus was blocked, is inferred at ~73 ka. It is supported by the geologicalgeomorphological evidence. The study demonstrates the application of provenance linked mineralogy in terrestrial aggradation in a tectonically active region.  相似文献   

14.
The geochemical composition of sandstones in the sedimentary basin is controlled mainly by the tectonic setting of the provenance, and it is therefore possible to reveal the tectonic setting of the provenance and the nature of source rocks in terms of the geochemical composition of sandstones. The major elements, rare-earth dements and trace elements of the Mesozoic-Cenozoic sandstones in the Lanping Basin are studied in this paper, revealing that the tectonic settings of the provenance for Mesozoic-Cenozoic sedimentary rocks in the Lanping Basin belong to a passive continental margin and a continental island arc. Combined with the data on sedimentary facies and palaeogeography, it is referred that the eastern part of the basin is located mainly at the tectonic setting of the passive continental margin before Mesozoic, whereas the western part may be represented by a continental island arc. This is compatible with the regional geology data. The protoliths of sedimentary rocks should be derived from the upper continental crust, and are composed mainly of felsic rocks, mixed with some andesitic rocks and old sediment components. Therefore, the Lanping Mesozoic-Cenozoic Basin is a typical continental-type basin. This provides strong geochemical evidence for the evolution of the paleo-Tethys and theb asin-range transition.  相似文献   

15.
The chemical leaching method is used for a systematic analysis of distribution characteristics of acid-soluble and acid-insoluble REE and other trace elements from the Luochuan loess deposits. The study shows that the acid-insoluble phase in loess and palaeosol is a stable component of old aeolian dusts and is characteristic of the provenance; the acid-soluble phase is the unstable component in the weathering pedogenic process and reflects rock-forming features after accumulation of aeolian dusts. The acid-insoluble REE and acid-soluble Sr and Pb can be used as geochemical indicators respectively to trace the provenance characteristics and the weathering pedogenic process.  相似文献   

16.
Opaque minerals in the Jilin meteorite inelude kamacite, taenite troilite, chromite, ilmenite, schreibersite, pyrite, pyrrhotite, chalcopyrite, sphalerite and graphite.Five of the above-mentioned minerals have been discussed in more detail in terms of optical and physical properties, chemical composition, coexisting relationship, and the order of crystallization. It is indicated from this study that, with the exception of a small amount of Ni-Fe cbondrules, silicate minerals are the first to erystallize followed by chromite, ilmenite at the early stage of nebula condensation, while Ni-Fe phase in the matrix is considered to be of a more later erigin. At the late stage of nebula condensation troilite resulted from the reaction of Ni-Fe metal with residual H2S vapor. As indicated by the occurrence of coarse grained Ni-Fe metal, the recrystallization of troilite and the apparent Neumann lines in kamaeite, it is expected that opaque minerals in the Jilin metevrite have undergone different degrees of thermal and impact metamorphisms.  相似文献   

17.
Tungsten isotope is a powerful tracer for the Earth’s accreting materials because of the distinct W isotope compositions of the non-carbonaceous meteorites and carbonaceous meteorites. To better understand the evolution of the early Earth, here we calculated the expected μ183W of the bulk silicate Earth for different assumed compositions of the proto-Earth’s mantle, the Moon-forming giant impactor, and the late veneer using a Monte Carlo approach. The result shows that the proto-Earth likely has a non-carbonaceous composition, while the carbonaceous chondrite-like materials were delivered to the Earth at the late stages of accretion. The predicted difference in μ183W values between the bulk silicate Earth and the non-carbonaceous meteorites of the scenarios assuming a pure carbonaceous composition for the giant impactor is slightly bigger than that of the scenarios assuming either a pure non-carbonaceous or a mixed carbonaceous-non-carbonaceous composition for the giant impactor (~5 ppm versus ~2 ppm). The ancient mantle reservoir that partially lacks the late veneer with carbonaceous composition should have a negative μ183W value (from ?3 to 0). Uncertainties introduced by the cosmogenic effects and mass-independent fractionation should be concerned during the high precision measurement of μ183W for meteorites and ancient terrestrial samples in further work.  相似文献   

18.
The Lunan stony meteorite recovered from Yunnan Province is an ordinary chondrite of high-iron Hs type. Thirteen kinds of minerals have been identified, of which natural copper contains 88--96% Cu. Compared with other meteorites of the same type,the Lunan meteorite has mere FeO and Ni.  相似文献   

19.
(U-Th)/He dating is a newly developed low temperature thermochronometry,and it elaborately reflects cooling history of geologic body under low temperature.It can be applied to analyze thermal evolution of the sedimentary basin,combining with vitrinite reflectance and fission track.(U-Th)/He dating of apatite and zircon from drilling cores in Puguang (普光)-Maoba (毛坝) area and outcrops in Tongjiang (通江) area indicates that the Northeast Sichuan (四川) basin underwent great uplift and denudation during the Tertiary and the Quaternary.During the period,denudation rates changed from 74.8 to 172.5 m/Ma and denudation thickness was between 2 800 and 3 000 m,geotemperature gradually declined into the current temperature,passing through helium closure temperature of apatite.The uplift and denudation relate to new tectonic movement response in the Sichuan basin aroused by the Qinghai (青海)-Tibet plateau.Drilling samples above 4 000 m did not undergo closure temperature of zircon,but the samples nearly 4 000 m might approach closure temperature of zircon and all the samples underwent closure temperature of apatite.According to (U-Th)/He ages of zircon,it is concluded that the Northeast Sichuan basin began to uplift in the Late Jurassic.From the Late Jurassic to the Paleogene,Northeast Sichuan basin was in slow uplift and denudation,but the denudation of Puguang-Maoba area was earlier than that of Tongjiang area.(U-Th)/He ages of zircon indicate the denudation time of provenance areas.On the basis of paleodrainage characteristics,provenance transport and other related data,provenance areas of the clastic rocks are decided,which is worthy to be investigated further.  相似文献   

20.
Glass and gas inclusions have been observed in olivine and other minerals in 30 doubly polished tin sections of Jilin meteorites, indicating that there must have been melting And condensation stages during the process of meteorite formation. Temperatures of formation have been determined by homogenization and quenching runs,giving 1050-200℃ and 502℃ for glass and gas inclusions respectively, Meanwhile,the fibrous radial crystals of pyroxene have been notieed to grow when heated over 800℃. These observations are in general agreement with the available experimental data and theoretical calculations regarding meteorite.  相似文献   

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