Stijn Glorie, Jay M. Thompson, Sarah E. Gilbert and A. Kate Souders
{"title":"LA-ICP-MS/MS†富稀土古近系辉钼矿Re-Os原位年代学","authors":"Stijn Glorie, Jay M. Thompson, Sarah E. Gilbert and A. Kate Souders","doi":"10.1039/D5JA00030K","DOIUrl":null,"url":null,"abstract":"<p >\r\n <em>In situ</em> Re–Os geochronology by LA-ICP-MS/MS was previously demonstrated by reacting Os with CH<small><sub>4</sub></small> or N<small><sub>2</sub></small>O reaction gasses. However, for both reactions, a minor proportion of the Re parent isotope also reacts, potentially leading to significant isobaric interferences of <small><sup>187</sup></small>Re on <small><sup>187</sup></small>Os, especially for young samples with little radiogenic in-growth. Here we present an interlaboratory comparison and compare three reaction gas mixtures (CH<small><sub>4</sub></small> + H<small><sub>2</sub></small> + He, N<small><sub>2</sub></small>O and N<small><sub>2</sub></small>O + He) with the aim to robustly date Palaeogene (66–23 Ma) molybdenite from the Bingham Canyon and Henderson deposits. CH<small><sub>4</sub></small> mixed with H<small><sub>2</sub></small> gas gives the highest sensitivity, while N<small><sub>2</sub></small>O and He gas buffer Re reaction. On balance, the analytical method involving N<small><sub>2</sub></small>O + He reaction gas is most suitable for dating Palaeogene molybdenite, resulting in age precision of 2.6% for Bingham and 5.8% for Henderson. For older, >1 Ga molybdenite, CH<small><sub>4</sub></small> + H<small><sub>2</sub></small> + He may give comparatively better age precision.</p>","PeriodicalId":81,"journal":{"name":"Journal of Analytical Atomic Spectrometry","volume":" 5","pages":" 1394-1402"},"PeriodicalIF":3.1000,"publicationDate":"2025-04-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"In situ Re–Os geochronology of Re-rich Palaeogene molybdenite by LA-ICP-MS/MS†\",\"authors\":\"Stijn Glorie, Jay M. Thompson, Sarah E. Gilbert and A. Kate Souders\",\"doi\":\"10.1039/D5JA00030K\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p >\\r\\n <em>In situ</em> Re–Os geochronology by LA-ICP-MS/MS was previously demonstrated by reacting Os with CH<small><sub>4</sub></small> or N<small><sub>2</sub></small>O reaction gasses. However, for both reactions, a minor proportion of the Re parent isotope also reacts, potentially leading to significant isobaric interferences of <small><sup>187</sup></small>Re on <small><sup>187</sup></small>Os, especially for young samples with little radiogenic in-growth. Here we present an interlaboratory comparison and compare three reaction gas mixtures (CH<small><sub>4</sub></small> + H<small><sub>2</sub></small> + He, N<small><sub>2</sub></small>O and N<small><sub>2</sub></small>O + He) with the aim to robustly date Palaeogene (66–23 Ma) molybdenite from the Bingham Canyon and Henderson deposits. CH<small><sub>4</sub></small> mixed with H<small><sub>2</sub></small> gas gives the highest sensitivity, while N<small><sub>2</sub></small>O and He gas buffer Re reaction. On balance, the analytical method involving N<small><sub>2</sub></small>O + He reaction gas is most suitable for dating Palaeogene molybdenite, resulting in age precision of 2.6% for Bingham and 5.8% for Henderson. For older, >1 Ga molybdenite, CH<small><sub>4</sub></small> + H<small><sub>2</sub></small> + He may give comparatively better age precision.</p>\",\"PeriodicalId\":81,\"journal\":{\"name\":\"Journal of Analytical Atomic Spectrometry\",\"volume\":\" 5\",\"pages\":\" 1394-1402\"},\"PeriodicalIF\":3.1000,\"publicationDate\":\"2025-04-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Analytical Atomic Spectrometry\",\"FirstCategoryId\":\"92\",\"ListUrlMain\":\"https://pubs.rsc.org/en/content/articlelanding/2025/ja/d5ja00030k\",\"RegionNum\":2,\"RegionCategory\":\"化学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"CHEMISTRY, ANALYTICAL\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Analytical Atomic Spectrometry","FirstCategoryId":"92","ListUrlMain":"https://pubs.rsc.org/en/content/articlelanding/2025/ja/d5ja00030k","RegionNum":2,"RegionCategory":"化学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"CHEMISTRY, ANALYTICAL","Score":null,"Total":0}
In situ Re–Os geochronology of Re-rich Palaeogene molybdenite by LA-ICP-MS/MS†
In situ Re–Os geochronology by LA-ICP-MS/MS was previously demonstrated by reacting Os with CH4 or N2O reaction gasses. However, for both reactions, a minor proportion of the Re parent isotope also reacts, potentially leading to significant isobaric interferences of 187Re on 187Os, especially for young samples with little radiogenic in-growth. Here we present an interlaboratory comparison and compare three reaction gas mixtures (CH4 + H2 + He, N2O and N2O + He) with the aim to robustly date Palaeogene (66–23 Ma) molybdenite from the Bingham Canyon and Henderson deposits. CH4 mixed with H2 gas gives the highest sensitivity, while N2O and He gas buffer Re reaction. On balance, the analytical method involving N2O + He reaction gas is most suitable for dating Palaeogene molybdenite, resulting in age precision of 2.6% for Bingham and 5.8% for Henderson. For older, >1 Ga molybdenite, CH4 + H2 + He may give comparatively better age precision.