吉林大学学报(地球科学版)
吉林大學學報(地毬科學版)
길림대학학보(지구과학판)
Journal of Jilin University (Earth Science Edition)
2015年
6期
1667-1690
,共24页
段志明%李光明%王保弟%李应栩%黄勇%郭琳%段瑶瑶
段誌明%李光明%王保弟%李應栩%黃勇%郭琳%段瑤瑤
단지명%리광명%왕보제%리응허%황용%곽림%단요요
锆石 U Pb 定年%辉钼矿 Re Os 定年%主碰撞期%查个勒铅锌矿床%中冈底斯成矿带
鋯石 U Pb 定年%輝鉬礦 Re Os 定年%主踫撞期%查箇勒鉛鋅礦床%中岡底斯成礦帶
고석 U Pb 정년%휘목광 Re Os 정년%주팽당기%사개륵연자광상%중강저사성광대
zircon U Pb dating%molybdenite Re Os age%main collisional period%Chagele lead-zinc deposit%Middle-Gangdese metallogenic belt
查个勒铅锌矿床是西藏中冈底斯成矿带中段新发现的一个大型斑岩矽卡岩型矿床,但其成岩成矿时代一直缺乏年代学约束。本文对该矿床含矿斑岩进行了 LA ICP MS 锆石 U Pb 定年、辉钼矿Re Os 定年、主量和微量元素分析及 Sr Nd Hf 同位素组成研究,获得中冈底斯成矿带中段铜钼铅锌银矿化时代。含矿斑岩 LA ICP MS 锆石 U Pb 年龄为64.6~62.9 Ma ,代表岩浆的结晶年龄;辉钼矿 Re Os 等时线年龄为(62.3±1.4)Ma ,代表查个勒主成矿年龄,与其构造岩浆事件一致;结合区域林子宗群大规模火山活动(65~45 Ma)以及以亚贵拉铅锌矿床(68.6~65.0 Ma)为代表的成矿作用,表明在印度与欧亚大陆主碰撞过程中均可产生不同规模的成矿作用。查个勒含矿斑岩具富硅、富钾,贫钛、贫磷特征,铝饱和指数(A /CN K)为1.12~1.60,富集大离子亲石元素 Rb 、Th 、U ,亏损高场强元素 Nb 、Zr 等,与冈底斯成熟大陆地壳物质相比具相对高的εNd (t)值(-6.64~-5.79)和相对低的(87 Sr/86 Sr)i 值(0.711813~0.717307),并具不均一的锆石εHf (t)值(-7.02~-1.27)以及古老的锆石 Hf 同位素地壳模式年龄(TCDM =1093~1419 Ma),属于过铝质 S 型花岗岩类。本文认为中冈底斯成矿带中段古新世岩浆活动和成矿作用,很可能与雅鲁藏布江洋盆闭合之后的印亚大陆碰撞诱发幔源岩浆底侵导致的冈底斯地体古老地壳物质部分熔融有关,岩浆在上升过程中有不同程度的分离结晶。
查箇勒鉛鋅礦床是西藏中岡底斯成礦帶中段新髮現的一箇大型斑巖矽卡巖型礦床,但其成巖成礦時代一直缺乏年代學約束。本文對該礦床含礦斑巖進行瞭 LA ICP MS 鋯石 U Pb 定年、輝鉬礦Re Os 定年、主量和微量元素分析及 Sr Nd Hf 同位素組成研究,穫得中岡底斯成礦帶中段銅鉬鉛鋅銀礦化時代。含礦斑巖 LA ICP MS 鋯石 U Pb 年齡為64.6~62.9 Ma ,代錶巖漿的結晶年齡;輝鉬礦 Re Os 等時線年齡為(62.3±1.4)Ma ,代錶查箇勒主成礦年齡,與其構造巖漿事件一緻;結閤區域林子宗群大規模火山活動(65~45 Ma)以及以亞貴拉鉛鋅礦床(68.6~65.0 Ma)為代錶的成礦作用,錶明在印度與歐亞大陸主踫撞過程中均可產生不同規模的成礦作用。查箇勒含礦斑巖具富硅、富鉀,貧鈦、貧燐特徵,鋁飽和指數(A /CN K)為1.12~1.60,富集大離子親石元素 Rb 、Th 、U ,虧損高場彊元素 Nb 、Zr 等,與岡底斯成熟大陸地殼物質相比具相對高的εNd (t)值(-6.64~-5.79)和相對低的(87 Sr/86 Sr)i 值(0.711813~0.717307),併具不均一的鋯石εHf (t)值(-7.02~-1.27)以及古老的鋯石 Hf 同位素地殼模式年齡(TCDM =1093~1419 Ma),屬于過鋁質 S 型花崗巖類。本文認為中岡底斯成礦帶中段古新世巖漿活動和成礦作用,很可能與雅魯藏佈江洋盆閉閤之後的印亞大陸踫撞誘髮幔源巖漿底侵導緻的岡底斯地體古老地殼物質部分鎔融有關,巖漿在上升過程中有不同程度的分離結晶。
사개륵연자광상시서장중강저사성광대중단신발현적일개대형반암석잡암형광상,단기성암성광시대일직결핍년대학약속。본문대해광상함광반암진행료 LA ICP MS 고석 U Pb 정년、휘목광Re Os 정년、주량화미량원소분석급 Sr Nd Hf 동위소조성연구,획득중강저사성광대중단동목연자은광화시대。함광반암 LA ICP MS 고석 U Pb 년령위64.6~62.9 Ma ,대표암장적결정년령;휘목광 Re Os 등시선년령위(62.3±1.4)Ma ,대표사개륵주성광년령,여기구조암장사건일치;결합구역림자종군대규모화산활동(65~45 Ma)이급이아귀랍연자광상(68.6~65.0 Ma)위대표적성광작용,표명재인도여구아대륙주팽당과정중균가산생불동규모적성광작용。사개륵함광반암구부규、부갑,빈태、빈린특정,려포화지수(A /CN K)위1.12~1.60,부집대리자친석원소 Rb 、Th 、U ,우손고장강원소 Nb 、Zr 등,여강저사성숙대륙지각물질상비구상대고적εNd (t)치(-6.64~-5.79)화상대저적(87 Sr/86 Sr)i 치(0.711813~0.717307),병구불균일적고석εHf (t)치(-7.02~-1.27)이급고로적고석 Hf 동위소지각모식년령(TCDM =1093~1419 Ma),속우과려질 S 형화강암류。본문인위중강저사성광대중단고신세암장활동화성광작용,흔가능여아로장포강양분폐합지후적인아대륙팽당유발만원암장저침도치적강저사지체고로지각물질부분용융유관,암장재상승과정중유불동정도적분리결정。
The newly discovered Chagele skarn‐porphyry deposit is located in the Middle‐Gangdese metallogenic belt . This study focuses on the zircon U Pb age of the ore‐bearing porphyry and molybdenite Re Os ,the whole rock major elements ,trace elements ,and the Sr Nd Hf isotopic data of the ore‐bearing rocks in Chagele deposit .The zircon U Pb age of the ore‐bearing porphyry changes from 64 .6 to 62 .9 Ma ,which represents the magmatic crystallization age .The Re Os isotopic age shows that the deposit was formed at (62 .3 ± 1 .4) Ma ,which is consistent with the magmatic age in the study area .Combing with the extensive volcanic event of Linzizong Group ,these new data suggests that the different scales of mineralization were formed at different stages in the entire collision between India and Eurasia continent .The ore‐bearing porphyry of Chagele deposit has high contents of SiO 2 ,K2 O , Rb ,Th ,and U ,coupled with low contents of TiO 2 , P2 O5 ,negative anomalies of Nb ,Zr ,variableεHf (t) ( - 7 .02 ~ - 1 .27) ,and ancient TCDM (1 093 ~ 1 419 Ma) .In comparison with the Gangdese continental crust composition ,the ore‐bearing porphyry is high in εNd (t) ( - 6 .64 ~ - 5 .79) and low in (87 Sr/86 Sr)i (0 .711 813 ~ 0 .717 307) .These geochemical features indicate that the porphyry of Chagele deposit is similar to the peraluminous feature of S‐type granite .The above discussion suggests that the Paleocene magmatism and mineralization in the middle section of the Middle‐Gangdese metallogenic belt could be formed through partial melting of the ancient crust materials of Gangdese micro‐continent accompanying with fractional crystallization ,which was probably induced by upwelling of mantle‐derived magma in the main collision between Indian and Eurasia continent .