共查询到19条相似文献，搜索用时 203 毫秒
1.
一种未定名的硫盐矿物——Pb_6Bi_7(Cu,Ag)S_(17) 总被引：1，自引：0，他引：1
在河北省涞源的铜铁矿床中,发现了一种未定名的Pb-Bi-Cu的硫盐矿物,它以不规则粒状产于黄铜矿之中,与它共生的有方铅矿、闪锌矿、碲银矿、硫银铋矿和自然银等。该矿物是铅灰色,金属光泽,直径0.003—0.72mm,在显微镜下呈白色微蓝,双反射弱,非均质性明显,H_v=119.75kg/mm~2(50g),D_x=7.04g/cm~3。六个颗粒的平均化学成分值是Pb 36.51,Bi 44.80,S 15.35,Cu 1.82,Ag 1.54,Cr0.105,总计100.135。理论化学式为Pb_6Bi_7(Cu,Ag)S_(17),其中Cu>Ag。X射线衍射的强线值:3.428(10,012),3.059(4.140),2.996(9,041),2.765(5,207),2.247(4,250),2.023(3,133);晶胞参数a=8.811,b=13.060,c=7.106,~(?)_(?)V=817.699~3。Z=1,斜方晶系。 相似文献
2.
钴硅锌矿是一种具有特征深蓝紫色、油脂光泽和玻璃光泽的钴锌硅酸盐矿物,属三方晶系。空间群:C_(3j)~2—R3、a=13.9559A,c=9.3364A,c/a=0.6690,V=1574.8104A~3,Z=18。该矿物理论式为(Zn,Co)_2SiO_4,实验式为:(Zn_(1.26),Co_(O.74))SiO_4。据红外光谱以及X射线粉晶分析,其结构与硅锌矿(Zn_2SiO_4)类似。 相似文献
3.
Fe,Sn氧化物矿产于四川雪宝顶钨锡矿床中,与之紧密共生的矿物是黑气电石,白云母,石英等,Fe-Sn氧化物呈细小的不规则颗粒嵌在锡石中,粒度大小为0.013 mm～0.052 mm之间,偶有个别大的颗粒(d=0.28 mm)淡红褐色,条痕无色,玻璃-金刚光泽,无解理,(因大小硬度无法测定),Dx=5.93 g/cm3.在偏光镜下淡黄褐色,多色性弱,明显的非均质性,按N=1+dk公式,获得N=2.11,矿物的的化学成份SnO273.70,TiO20.60,Fe 2O3 25.26,总计99.56(7个不同测点的平均值),计算出化学式为Fe 23+Sn3O9.矿物的强X射线值3.702(15,511),3.445(5,901),3.348(100,505),3.264(14,711),3.114(40,712),1.487(10,033),单斜晶系,晶胞参数a=3.375 nm,b=0.457 nm,c=2.001nm,β=93°24',V=3.080 74 nm3,Z=18. 相似文献
4.
钇硅磷灰石为乳白、玫瑰色,实测比重为4.35,二轴晶正光性,α=1.791;γ=1.784;电子探针分析计算晶体化学式为(Y_(2.82)Ca_(1.58)Ce_(0.27)Dy_(0.21)Er_(0.11…)_5[(Si_(2.95)P_(0.05))_3O_(12)](OH,F),空间群为C_2~2-P2_1,晶胞参数为a=0.9504±0.0005nm,b=0.9414±0.0004nm, c=0.6922±0.0002nm,r=119.71±0.04°,V=53.79±0.04nm~3,Z=2,结构参数经各向异性温度因子最小二乘法修正后R=0.111。结构分析表明:由磷灰石型的P6_3/m降低至钇硅磷灰石的P2_1,Y~(3+)替代Ca~(2+)成有序分布,导致结构中7角和9角多面体的畸变,同时Si~(4+)替代P~(5+),OH-替代F~-,加大了这种畸变,使得Y、Ca、Si、O及OH~-都偏离了赝六方P6_3/m的6h、4f、12i及2a等效点系位置,但钇硅磷灰石仍近似磷灰石型结构,最后对磷灰石型结构矿物的晶体化学进行了讨论。 相似文献
5.
吉林省石头口门硅岩之成因及构造环境 总被引：1，自引：1，他引：0
吉林省石头口门硅岩的岩石地层剖面,自下而上为碎屑岩-含锰结核碎屑岩-碎屑岩与硅岩夹玄武岩-细碧角斑岩与硅岩-硅岩与碎屑岩-碎屑岩夹碳酸盐岩-碎屑岩.硅岩经三次系统采样分析,仅一样发现似放射虫泡沫虫内核,碳酸盐岩中产晚石炭世威宁期的(竹蜓)类化石.硅岩的岩石化学成分平均值(wB/10-2),SiO2为90.98,TiO2为0.15,Al2O3、Fe2O3、FeO、Na2O、K2O分别为2.41、1.29、1.76、0.46、0.36.微量元素与其它一般正常海相沉积相比较,以Ba、Ni、Co、V、Cu、Pb、U等高含量为特征.稀土元素组成,以稀土总量低(平均值56.38×10-6),轻稀土富集(平均LREE/HREE=5.50)为主要特征;δEu弱负异常至正异常(平均0.89),特别是作为其沉积环境判别有效标志δCe,亦显示出弱负异常至正异常(0.57～1.01),平均0.80.所测一氧同位素样,δ18O为1.9‰(SMOW).在该区与硅岩共生的镁铁-超镁铁岩块(体),获得其Sm-Nd等时线年龄2 067±76.6Ma(置信度为0.999 569).表明硅岩为与海底火山作用有密切联系的热水沉积,下部及上部的硅岩受到正常海水的交换和陆源碎屑混入的影响.构造环境不同于洋中脊或深洋盆所形成之硅岩,而为陆缘活动带裂陷槽的海相沉积物. 相似文献
6.
本文通过对碧溪岭片麻岩综合研究表明,岩石化学成分高硅(SiO2=73.18%～75.60%)、低铝(Al2O3=11.93%～12.79%)、富碱(Na2O+K2O=6.11%～7.23%)和高钠(Na2O/K2O=1.51～1.94); 微量元素富集大离子亲石元素Rb、Ba、Th、U等和Pb,贫Nb、Ta、Zr、Hf、Ti等高场强元素; 稀土元素含量范围变化较大(TREE=142.38～308.44×10-6),富集轻稀土(LREE/HREE=5.93～6.01),和铕负异常明显(δEu=0.42～0.64)等。造岩矿物中斜长石聚片双晶常垂直晶体延长方向,以及继承锆石大部分是不同时代的岩浆碎屑锆石等,暗示其寄主岩是沉积岩; 锆石LA-ICP-MS定年结果: 1)获得超高压变质锆石U-Pb年龄为242 Ma; 2)继承锆石U-Pb年龄,除了有比较多的属于元古代(768～639 Ma),还有大量的属于古生代(590～358 Ma)等,表明其寄主岩的时代不会早于古生代。 相似文献
7.
对Allende陨石中一块富深绿辉石--钙长石-尖晶石难熔包体进行了岩石学和矿物化学研究。包体近似球形(半径~3 mm),边部为钙长石和方钠石(Mg O=1.04%~2.69%;Fe O1.57%)组成的矿物圈层(厚度~200μm),内部主要矿物有深绿辉石(Al2O3=7.63%~16.08%;Ti O2=1.73%~4.48%)、钙长石(Mg O0.41%;Na2O0.14%)和尖晶石(Fe O1.70%)。包体中残留黄长石(k70~85,Na2O0.22%),颗粒较小(10μm),大部分都被蚀变成为钙铝榴石、钙镁橄榄石和氯硅铝钙石(Mg O=5.07%~8.04%;Fe O0.31%)。包体规则的外形不可能由气—固凝聚形成,而可能是由熔融重结晶形成。黄长石含量较少以及残余黄长石非常富镁说明包体可能经历过蚀变作用,且方钠石与氯硅铝钙石的产状和成分差异说明包体可能经历了两次不同的蚀变事件。 相似文献
8.
德兴斑岩铜矿位于扬子地块江南隆起带东缘,含矿斑岩类型为花岗闪长斑岩。岩石主矿物组合为斜长石(中长石、更长石)+石英+钾长石+角闪石+黑云母,常见副矿物为磁铁矿、磷灰石、榍石、钛铁矿和锆石。斑岩主量元素具有高硅(SiO2=63.59%)、高铝(Al2O3=15.54%)、低镁(MgO=2.2%)的特征,岩石富钾贫钠(K2O=3.06%;Na2O=3.67%),高K2O/Na2O(0.89)比;ALK=6.66%,A/CNK=1.086,σ=2.18,A.R=2.07,显示岩石为弱过铝质高钾钙碱性系列;稀土元素特征表现为轻稀土富集(121.81×10-6),重稀土亏损(8.8×10-6),具有较大的LREE/HREE比值(13.93);微量元素表现为富集大离子亲石元素LILE(Rb、Ba、La、Sr)和亏损高场强元素HFSE(Nb、Ta、Y),具低Y(11.21×10-6)和Yb(1.23×10-6)含量特征,有较高Sr/Y(57.29)、La/Yb(28.93)比值,具较高的87Sr/86Sr比值(0.7040),弱的负Eu异常(δEu=0.91),以及负εNd值等特征,表明德兴花岗闪长斑岩为"C"型高钾钙碱性埃达克岩,埃达克岩浆来源于活动陆缘加厚下地壳的部分熔融。 相似文献
9.
兴凯地块南部构造演化复杂,缺乏精确的年代学证据和系统的地球化学研究.锆石U-Pb年龄测定结果表明:兴凯地块南部花岗岩侵位结晶年龄为晚三叠世末期(202~205 Ma),处于古亚洲洋和古太平洋构造体制的转换阶段.地球化学成分上,二长花岗岩和花岗闪长岩均以富硅(SiO2=69.61%~77.27%)、弱过铝(Al2O3=12.70%~15.28%)、较富碱(AKI=0.64~0.88)为特征.结合角闪石矿物的出现、较低的锆石饱和温度(TZr=679~787 ℃)等特征表明本区花岗岩为分异的Ⅰ型花岗岩.锆石的176Hf/177Hf比值较高(0.282 773~0.282 913),εHf(t)均为正值(4.39~9.32),二阶段Hf模式年龄较为年轻(0.65~0.96 Ga),反映其源区物质为新元古代期间从亏损地幔新增生的年轻地壳物质.结合岩石形成年龄、岩石组合等特征可以推断岩石应该形成于西太平洋开始俯冲的活动大陆边缘环境下. 相似文献
10.
捷尔碱性-超基性岩体的铂族元素矿物主要是等轴铁铂矿,该矿物有两个世代,即:①早期高温等轴铁铂矿,形成于纯橄榄岩中;②晚期世代等轴铁铂矿,多充填于纯橄榄岩致密块状铬铁矿透镜体或脉体的间隙中,有时呈立方体结晶分布于纯橄榄岩内金云母-磁铁矿单斜辉石岩岩墙或脉体中.高温等轴铁铂矿与晚期世代等轴铁铂矿的含铁性相近(kFe 7.5%~11.5%),其差别在于高温等轴铁铂矿含铂族元素较高(k),Ir5.3%、Os2.9%、Rh1.8%,而晚期等轴铁铂矿一般Ir不超过1.9%、Os1.0%、Rh0.6%.铂族元素的次要矿物有两类:①形成于岩浆期的矿物,如Os-Ir-Ru-Pt系的固溶体矿物(包括自然铂、自然锇,自然铱、自然钌);②岩浆后期矿物,如四方铁铂矿,四方铜铁铂矿、洪戈石、二硫锇矿-二硫钌矿、硫砷铱矿-硫砷铑矿、硫铂矿,铋化物,锑化物,碲化物,锡化物及氢氧化物等一系列新矿物(Pd-洪戈石、Rh-兴中矿,Pt-康捷尔矿,硫铱铅铜矿等).上述矿物在等轴铁铂矿颗粒的周围或边部多形成镶边.类似的产状亦见于低温等轴铁铂矿之周围,并形成有自然金,含银自然金至金银矿、银金矿等.此外,还见有含铜、含铜-铅、含铜-钯的自然金,其组成为Au3Cu至AuCu及AuCu3等. 相似文献
11.
Luobusaite： A New Mineral 总被引：6，自引：0，他引：6
BAI Wenji SHI Nicheng FANG Qingsong LI Guowu XIONG Ming YANG Jingsui RONG He 《《地质学报》英文版》2006,80(5):656-659
A group of mantle minerals including about 70-80 subtypes of minerals are discovered from a podiform chromitite in Tibet, China. Recovered minerals include diamond, coesite, moissanite, wustite, Fe-silides and a new mineral, luobusaite. All of these minerals were hand-picked from heavymineral separates of the podiform chromitite in the mantle peridotite of an ophiolite. The grains of luobusaite are as host mineral with inclusions of native silicon or as an intergrowth with native silicon and Fe-Si phase. Luobusaite occurs as irregular grains, with 0.1-0.2 mm in size, consisting of very finegrained aggregates. The mineral is steel-grey in color, metallic luster, and opaque. The empirical formula （based on 2 for Si） is Fe0.83Si2, according to the chemical compositions of luobusaite. X-ray powder-diffraction data： orthorhombic system, space group Cmca, a = 9.874 （14） A, b = 7.784 （5） A, c= 7.829（7） A, Z=16. 相似文献
12.
We report the results of SIMS isotopic analyses of carbon, nitrogen, oxygen, and silicon made on 849 small (approximately 1 micrometer) individual silicon carbide grains from the Murchison meteorite. The isotopic compositions of the major elements carbon and silicon of most grains (mainstream) are similar to those observed in larger grain studies suggesting an AGB star origin of these grains. In contrast, the trace element nitrogen shows a clear dependency on grain size. 14N/15N ratios increase with decreasing grain size, suggesting different stellar sources for grains of different size. Typically observed 14N/15N ratios in the small grains of this study are approximately 2700, clearly larger than the values expected from model calculations of AGB stars. In addition to the three dredge-up episodes characteristic for the evolution of AGB stars, extra-mixing of CNO-processed matter in low mass AGB stars appears to be a promising possibility in order to explain the high 14N/15N ratios of the small circumstellar SiC grains. A small fraction of grains shows a silicon isotopic signature not observed in larger circumstellar SiC grains from Murchison. Their stellar origin is still uncertain. The minor type A, B, Y, and X grains were found to be present at a level of a percent, which is similar to their abundance in the larger-grain SiC separates from Murchison. Oxygen isotopic compositions are normal within the experimental uncertainties of several 10%, indicating that oxygen of stellar origin is rare or even absent in the SiC grains. We conclude that most of the oxygen is a contaminant which was introduced into the SiC grains after their formation, e.g., during sample processing in the laboratory. We identified a nitride grain, most likely Si3N4 with little carbon, with highly anomalous isotopic compositions (12C/13C = 157 +/- 33, 14N/15N = 18 +/- 1, delta 29 Si = -43 +/- 56%, delta 30 Si = -271 +/- 50%). The isotopic patterns of carbon, nitrogen, and silicon resemble those of the rare SiC X grains suggesting that these two rare constituents of circumstellar matter formed in the same type of stellar source, namely, Type II supernovae. 相似文献
13.
SHI Nicheng BAI Wenji LI Guowu XIONG Ming FANG Qingsong YANG Jingsui MA Zhesheng RONG He X-ray Laboratory China University of Geosciences Beijing China Institute of Geology Chinese Academy of Geological Sciences Beijing China 《《地质学报》英文版》2009,83(1)
Yarlongite occurs in ophiolitic chromitite at the Luobusha mine (29°5′N 92°5′E,about 200 km ESE of Lhasa),Qusum County,Shannan Prefecture,Tibet Autonomous Region,People's Republic of China.Associated minerals are:diamond,moissanite,wiistite,iridium ("osmiridium"), osmium ("iridosmine"),periclase,chromite,native iron,native nickel,native chromium,forsterite, Cr-rich diopside,intermetallic compounds Ni-Fe-Cr,Ni-Cr,Cr-C,etc.Yarlongite and its associated minerals were handpicked from a large heavy mineral sa... 相似文献
14.
Taldybulak Levoberezhny(又称左岸)矿床位于吉尔吉斯斯坦北天山东段,是区内第三大金矿(金储量130 t,平均品位6.9 g/t)。长期以来,该矿床矿物学研究薄弱,成因类型存在争议,已有观点包括斑岩型、造山型、多阶段叠加成矿等。野外地质调查及室内岩相学鉴定发现：金矿化同时受韧性剪切带和岩体控制,局部显示一定的顺层特征;常见矿石类型包括浸染细脉浸染型、石英电气石硫化物型、块状硫化物型、稀疏浸染型、方解石硫化物脉型等;相关围岩蚀变以硅化、绢云母化、电气石化、碳酸盐化最为强烈,可见绿泥石化、绿帘石化、泥化等。电子探针分析发现,左岸金矿同时发育可见金和不可见金。前者包括银金矿(w(Au)=67.90%~80.86%,w(Ag)=14.24%~30.76%)、含银自然金(w(Au)=88.95%,w(Ag)=8.09%)等,以包体金、裂隙金或粒间金形式赋存于黄铁矿中。后者可赋存于黄铁矿和黄铜矿中(w(Au)=0.16%~0.33%)。不同类型矿石中黄铁矿的形态、结构、成分存在一定差异,显示了叠加成矿的可能性。浸染状细脉浸染型矿石中黄铁矿以中粗粒(30~1 300 μm,多数>200 μm)、半自形自形立方体为主,基本无碎裂或碎裂不明显,可含有自然金、银金矿或硅酸盐包体;成分上具有中等的As(0.03%~1.72%,平均0.66%)、Co(0.06%~0.19%,平均0.13%)、Te(0.03%~0.06%,平均0.04%)含量和As/S、Fe/S、Co/As比值,基本不含Cu、Pb、Zn、Ag。石英电气石硫化物型矿石中黄铁矿多呈中粗粒(30~2 000 μm)、半自形它形粒状,往往发生碎裂,并被黄铜矿、方铅矿等矿物交代;部分颗粒可含有银金矿或硅酸盐包体;总体具有较高的As(0.05%~2.05%,平均0.97%)、Co(0.05%~0.34%,平均0.15%)含量和As/S、Fe/S比值,Co/As比值较低。块状硫化物型矿石中黄铁矿多呈半自形它形粒状产出,但粒度变化较大(250~3 000 μm或者30~300 μm);化学成分上以较高的As(0.05%~2.20%,平均1.21%)、Te(0.04%~0.09%,平均0.06%)含量,高的As/S、Fe/S比值和低的Co/As比值为特征。稀疏浸染型矿石中黄铁矿呈中粒(集中于50~200 μm)、半自形它形粒状产出,内部可含有硫化物、硅酸盐、银金矿、自然金等包体;可发生碎裂并被黄铜矿等沿裂隙充填交代;化学成分变化较大,总体具有较高的Co(0.08%~1.04%,平均0.35%)含量和Co/As比值,几乎不含Te、Cu、Zn。方解石硫化物脉型矿石中黄铁矿呈中粗粒(40~480 μm)、半自形它形粒状产出,内部往往含硅酸盐等包体;黄铁矿以显著低的As(0.04%~0.08%,平均0.06%)、Co含量(0.04%~0.20%,平均0.10%)以及As/S、Fe/S比值为特征,Co/As比值较高,且不含Zn。从上述左岸金矿的控矿构造、矿化类型、围岩蚀变以及不同类型矿石中黄铁矿形态、结构、成分的差异等4方面特征显示,左岸金矿可能存在多期次矿化、叠加成矿。 相似文献
15.
到目前为止从陨石中分离出的太阳系外物质有金刚石、碳化硅、石墨、Ｓｉ３Ｎ４、刚玉及尖晶石等。除金刚石为纳米级大小外,其他为微米和次微米级颗粒。这些太阳系外物质主要存在于原始的球粒陨石的基质中,并通过化学分离的方法获得。金刚石携带分别由ｐ－过程和ｒ－过程产生的Ｘｅ同位素组分（Ｘｅ－ＨＬ）,其源区可能提超新星。绝大部分碳化硅相对于太阳系物质富＾２９．３０Ｓｉ和＾１３Ｃ,贫＾１５Ｎ,并携带ｓ－过程产生的各 相似文献
16.
Gold paragenesis and chemistry at Batu Hijau, Indoneisa: implications for gold-rich porphyry copper deposits 总被引：3，自引：0，他引：3
Gold is an important by-product in many porphyry-type deposits but the distribution and chemistry of gold in such systems remains poorly understood. Here we report the results of petrographic, electron microprobe, laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS), and flotation test studies of gold and associated copper sulfides within a paragenetic framework from the world-class Batu Hijau (914 mt @ 0.53% Cu, 0.40 g/t Au) porphyry copper–gold deposit, Indonesia. Unlike many other porphyry copper–gold deposits, early copper minerals (bornite–digenite–chalcocite) are well preserved at Batu Hijau and the chalcopyrite–pyrite overprint is less developed. Hence, it provides an excellent opportunity to study the entire gold paragenesis of the porphyry system. In 105 polished thin sections, 699 native gold grains were identified. Almost all of the native gold grains occurred either within quartz veins, attached to sulfide, or as free gold along quartz or silicate grain boundaries. The native gold grains are dominantly round in shape and mostly 1–12 m in size. The majority of gold was deposited during the formation of early A veins and is dominantly associated with bornite rather than chalcopyrite. The petrographic and LA-ICP-MS study results indicate that in bornite-rich ores gold mostly occurs within copper sulfide grains as invisible gold (i.e., within the sulfide structure) or as native gold grains. In chalcopyrite-rich ores gold mostly occurs as native gold grains with lesser invisible gold. Petrographic observations also indicate a higher proportion of free gold (native gold not attached to any sulfide) in chalcopyrite-rich ores compared to bornite rich ores. The pattern of free gold distribution appears to correlate with the flotation test data, where the average gold recovery value from chalcopyrite-rich ores is consistently lower than bornite-rich ores. Our data suggest that porphyry copper-gold deposits with chalcopyrite-rich ores are more likely to have a higher proportion of free gold and may require different ore processing strategies.Editorial handling: R. P. Richards 相似文献
17.
Study on presolar grains including diamond,silicon carbide,graphite,silicon nitrite(Si3N4),coundum and spinel isolated from meteorites is summarized in this paper.Except for nanometer-sized diamond,the other grains are micrometers to submicrometers in size.The presolar grains survived mainly in the fine-grained matrix of primitive chondrites and were isolated by chemical treatments.Diamond contains Xe isotopes(Xe-HL),typically produced in p-and r-processes,probably formed in supernovae.Mainstream silicon carbides are enriched in ^29,30Si and ^13C,but depleted in ^15N.They also contain various s-process products,consistent with calculations of AGB stars.Other silicon carbides exhibit much larger isotopic anomalies and are classified as groups X,Y,Z and AB.Among them,group X of SiC is characterized by enrichment of ^28Si and daughter isotopes of various short-lived nuclides,suggesting an origin from supernovae.Graphite can be divided into four density fractions with distince isotopic compositions.They may form in AGB stars,novae and supernovae,respctively,Si3N4 is similar to X-SiC in isotopic composition.Corundum is classified as four groups based on theid oxygen isotopic compositions.AGB and red giang stare are possible sources for the oxide.More comprehensive study of presolar grains,especially discovery of the other types of oxides and silicates,isotopic analyses of individual submicrometer-sized grains and distribution of presolar grains among various chemical groups and petropaphic types of chondrites will provide new information on nucleosynthesis,stellar evolution and formation of the solar nebula. 相似文献
18.
硒汞矿产于甘肃省拉尔玛金矿床中,主要共生矿物有石英、重晶石、辉锑矿、黑辰砂、自然金等。硒汞矿呈铅灰色到黑色,金属光泽,性脆。粒度0.01～0.36mm。比重D=8.27,摩氏硬度2.5。电子探针定量分析结果的平均值(%):Hg 71.50,Se 25.21,S 1.88,Au 0.19,Ag 0.07,Te 0.09,As 0.06,Sb 0.04,Fe 0.04,总和99.08。空间群。a=0.6081(1)nm,Z=4。 相似文献
19.
Yarlongite: A New Metallic Carbide Mineral 总被引：1，自引：0，他引：1
SHI Nicheng BAI Wenji LI Guowu XIONG Ming FANG Qingsong YANG Jingsui MA Zhesheng RONG He 《《地质学报》英文版》2009,83(1):52-56
Yarlongite occurs in ophiolitic chromitite at the Luobusha mine (29°5′N 92°5′E, about 200 km ESE of Lhasa), Qusum County, Shannan Prefecture, Tibet Autonomous Region, People’s Republic of China. Associated minerals are: diamond, moissanite, wüstite, iridium (“osmiridium”), osmium (“iridosmine”), periclase, chromite, native iron, native nickel, native chromium, forsterite, Cr-rich diopside, intermetallic compounds Ni-Fe-Cr, Ni-Cr, Cr-C, etc. Yarlongite and its associated minerals were handpicked from a large heavy mineral sample of chromitite. The metallic carbides associated with yarlongite are cohenite, tongbaite, khamrabaevite and qusongite (IMA2007-034). Yarlongite occurs as irregular grains, with a size between 0.02 and 0.06 mm, steel-grey colour, H Mohs: 5?-6. Tenacity: brittle. Cleavage: {0 0 1} perfect. Fracture: conchoidal. Chemical formula: (Cr4Fe4Ni)Σ9C4, or (Cr,Fe,Ni)Σ9C4, Crystal system: Hexagonal, Space Group: P63/mc, a = 18.839(2) ?, c = 4.4960 (9) ?, V = 745.7(2) ?3, Z = 6, Density (calc.) = 7.19 g/cm3 (with simplified formula). Yarlongite has been approved as a new mineral by the CNMNC (IMA2007-035). Holotype material is deposited at the Geological Museum of China (No. M11650). 相似文献