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With a detailed study on petrology, mineralogy and geochemistry of some important Ordovician carbonate well core samples in Tazhong uplift of Tarim Basin, the distinguishing symbols of hydrothermal karstification are first put forward as the phenomena of rock hot depigmentation, hot cataclasm and the appearance of typical hydrothermal minerals such as fluorite, barite, pyrite, quartz and sphalerite. The main homogenization temperatures of primary fluid inclusions in fluorite are from 260 to 310°C, indicating the temperature of hydrothermal fluid. The fluid affected the dissolved rocks and showed typical geochemistry features with low contents of Na and Mg, and high contents of Fe, Mn and Si. The ratio of 3He/4He is 0.02R a, indicating the fluid from the typical continental crust. The hydrothermal fluid karstification pattern may be described as follows: the hot fluid is from the Permian magma, containing dissolving ingredients of CO2 and H2S, and shifts along fault, ruptures and unconformity, and dissolves the surrounding carbonates while it flows. The mechanism of hydrothermal karstification is that the mixture of two or more fluids, which have different ion intensity and pH values, becomes a new unsaturated fluid to carbonates. The hydrothermal karstification is an important process to form hypo-dissolved pinholes in Ordovician carbonates of Tazhong uplift of Tarim Basin, and the forming of hydrothermal minerals also has favorable influence on carbonate reservoirs.
相似文献2.
HSU WeiBiao 《中国科学D辑(英文版)》2007,50(6):886-896
Numerous round to oblate opaque assemblages (OAs) are found in chondrules and matrix of the Ningqiang carbonaceous chondrite. They are mainly composed of Ni-rich metal,magnetite,Fe,Ni-sulfides,with minor amounts of phosphate,phosphoran-olivine,pyroxene and trace amounts of nano-sized platinum-group metal alloys. The mineralogy of Ningqiang OAs is very similar to that of OAs previously reported in Ca,Al-rich inclusions of CV chondrites. Being a rare mineral phase in nature,phosphoran-olivine is thought to form by nonequilibrium reactions between P-bearing molten metal and olivine crystals during rapid cooling. Its occurrence in Ningqiang OAs indicates that the precursor of OAs was locally produced during chondrule formation,rather than directly condensed from the solar nebula as previously thought. The petrographic and mineralogical characteristics of Ningqiang OAs reveal that OAs formed by low temperature alterations of pre-existing homogeneous alloys within chondrules on a planetary body. 相似文献
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HSU WeiBiao 《中国科学:地球科学(英文版)》2010,(3)
Miller Range (MIL) 05035 and LaPaz Icefield (LAP) 02224 are unbrecciated lunar basalt meteorites. In this report, we studied their petrography and mineralogy and made in situ uranogenic Pb/Pb dating of Zr-rich minerals. Petrography and mineralogy of these two lunar meteorites are consistent with previous investigations. The zirconolite Pb/Pb age of MIL 05035 is 3851±8 Ma (2σ), in excellent agreement with previous reports. This age suggests that MIL 05035 could be paired with Asuka 881757, a low-Ti mare basalt meteorite. The magmatic event related to MIL 05035 was probably due to the late heavy impact bom- bardment on the moon around 3.9 Ga. One baddeleyite grain in LAP 02224 shows a large variation of Pb/Pb age, from 3109±29 to 3547±21 Ma (2σ), much older than the whole-rock age of the same meteorite (~3.02±0.03 Ga). The other baddeleyite grain in LAP 02224 has an age of 3005±17 Ma (2σ). The result indicates that the minimum crystallization age of LAP 02224 is ~3.55 Ga and the younger ages could reflect late thermal disturbance on U-Pb system. 相似文献
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With a detailed study on petrology, mineralogy and geochemistry of some important Ordovician carbonate well core samples in Tazhong uplift of Tarim Basin, the distinguishing symbols of hydrothermal karstification are first put forward as the phenomena of rock hot depigmentation, hot cataclasm and the appearance of typical hydrothermal minerals such as fluorite, barite, pyrite, quartz and sphalerite. The main homogenization temperatures of primary fluid inclusions in fluorite are from 260 to 310°C, indicating the temperature of hydrothermal fluid. The fluid affected the dissolved rocks and showed typical geochemistry features with low contents of Na and Mg, and high contents of Fe, Mn and Si. The ratio of 3He/4He is 0.02R a, indicating the fluid from the typical continental crust. The hydrothermal fluid karstification pattern may be described as follows: the hot fluid is from the Permian magma, containing dissolving ingredients of CO2 and H2S, and shifts along fault, ruptures and unconformity, and dissolves the surrounding carbonates while it flows. The mechanism of hydrothermal karstification is that the mixture of two or more fluids, which have different ion intensity and pH values, becomes a new unsaturated fluid to carbonates. The hydrothermal karstification is an important process to form hypo-dissolved pinholes in Ordovician carbonates of Tazhong uplift of Tarim Basin, and the forming of hydrothermal minerals also has favorable influence on carbonate reservoirs. 相似文献
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With a detailed study on petrology, mineralogy and geochemistry of some important Ordovician carbonate well core samples in Tazhong uplift of Tarim Basin, the distinguishing symbols of hydrothermal karstification are first put forward as the phenomena of rock hot depigmentation, hot cataclasm and the appearance of typical hydrothermal minerals such as fluorite, barite, pyrite, quartz and sphalerite. The main homogenization temperatures of primary fluid inclusions in fluorite are from 260 to 310℃, indicating the temperature of hydrothermal fluid. The fluid affected the dissolved rocks and showed typical geochemistry features with low contents of Na and Mg, and high contents of Fe, Mn and Si. The ratio of 3He/4He is 0.02Ra, indicating the fluid from the typical continental crust. The hydrothermal fluid karstification pattern may be described as follows the hot fluid is from the Permian magma, containing dissolving ingredients of CO2 and H2S, and shifts along fault, ruptures and unconformity, and dissolves the surrounding carbonates while it flows. The mechanism of hydrothermal karstification is that the mixture of two or more fluids, which have different ion intensity and pH values, becomes a new unsaturated fluid to carbonates. The hydrothermal karstification is an important process to form hypo-dissolved pinholes in Ordovician carbonates of Tazhong uplift of Tarim Basin, and the forming of hydrothermal minerals also has favorable influence on carbonate reservoirs. 相似文献
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GRV 99027陨石是二辉橄榄岩质辉玻无球粒陨石(L-S)的火星陨石新成员,具有嵌晶、非嵌晶和冲击熔融袋结构。矿物模式组成以橄榄石(55%)、辉石(37．5%)为主,有少量熔长石(6%)、铬铁矿(1．5%)以及微量白磷钙石、陨硫铁等。其矿物的化学成分较为均一,无分带现象。橄榄石组分为Fo_(69．1～76．6)Fa_(23．4～30．9),平均Fo_(72．4)Fa_(27．6),低钙易变辉石为En_(59．3～75．1) Fs_(20．5～26．9)Wo_(3．1～14．9),平均En_(68．6)Fs_(23．5)Wo_(8．0),普通辉石为En_(46．6～53)Fs_(13．1～16．1)Wo_(31．9～37．8),平均En_(50．7)Fs_(14．5)Wo_(34．8),熔长石为An_(43．6～59．3) Ab_(40．2～54．6)Or_(0．5～1．8),平均An_(52．4)Ab_(46．7)Or_(0．8)。该陨石的结晶顺序是：亏损的火星幔源区部分熔融形成的原始母岩浆最先结晶的是嵌晶区的橄榄石和铬铁矿,随后易变辉石晶出,呈主晶包裹橄榄石和铬铁矿；此后,橄榄石、易变辉石、普通辉石持续结晶,直到残余熔体在晶隙形成斜长石和白磷钙石等。在这陨石中的易变辉石和普通辉石共存,二辉石温度计显示平衡温度为1000～1190℃(平均≈1146℃)。GRV 99027经历的亚固相再平衡,其程度为ALH 77005≈GRV 99027＞LEW 88516＞Y 793605。GRV 99027经受的冲击压力为30～45 GPa,,局部达到60～80GPa,冲击后温度可能＜600℃。 相似文献
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Dhofar 1180是一块新发现于阿曼地区的月球陨石,属混合岩质月球角砾岩。本文报道了Dhofar 1180的岩相学和矿物化学特征。该陨石含有辉长岩、斜长岩质辉长岩、辉长质斜长岩、橄长岩和微斑熔融角砾岩等多种类型岩屑,同时还存在含钛玻屑和长石质玻屑。主要的晶屑矿物有橄榄石、辉石、斜长石、和金属氧化物。辉长质斜长岩、橄长岩和微斑熔融角砾岩等岩屑中橄榄石相对富镁(Fo_(55～69)),斜长岩质辉长岩岩屑中橄榄石相对富铁(Fo_(31)),含钛玻屑中橄榄石包体成分变化较大(Fo_(7～54))。晶屑橄榄石相对富铁,且成分变化较大(Fo_(2～46))。Fe/Mn摩尔比主要在69～113之间变化(平均值为93),且Fe-Mn摩尔数变化趋势与典型的月球橄榄石一致。辉长质斜长岩、橄长岩、微斑熔融角砾岩等岩屑和含钛玻屑中的辉石相对贫钙,主要为易变辉石(分别为En_(63)Fs_(32)Wo_5,En_(66)Fs_(23)Wo_(11),En_(55)Fs_(38)Wo_7和En_(57)Fs_(35)Wo_8),而斜长岩质辉长岩和辉长岩岩屑中的辉石和晶屑辉石的成分变化比较大(分别为En_(31～33)Fs_(35～48)Wo_(19～34),En_(18～48)Fs_(23～51)Wo_(24～38) En_(1～9)Fs_(65～86)Wo_(14～26)和En_(11～53)Fs_(23～63) Wo_(6～36),为易变辉石和普通辉石,以及少量三斜铁辉石。含钛玻屑中辉石含有较高的Al_2O_3(2.79%)和TiO_2(1.57%)含量。辉石的Fe/Mn摩尔比主要在50～70之间变化(平均值为63),且其Fe-Mn摩尔数变化趋势也与典型的月球辉石一致。斜长石主要是钙长石,含有少量的Na_2O,An组分范围是91～98。金属氧化物主要为钛铁尖晶石-铬铁矿-尖晶石固溶体,存在少量的钛铁矿。Dhofar 1180的矿物学、岩石学和微量元素地球化学特征与已知的月球陨石和月岩样品有明显的差异,它来自月球表面的一个新的未知地区。对Dhofar 1180的矿物学、岩石学和化学成分的研究将更大地丰富我们对月球表面物质组成和演化的全面认识。 相似文献
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