{"title":"火星陨石Allan Hills 84001中40亿年前碳酸盐的原位U-Pb测年","authors":"R. Tartèse, I. Lyon","doi":"10.5194/gchron-4-683-2022","DOIUrl":null,"url":null,"abstract":"Abstract. In situ carbonate U–Pb dating studies have proliferated dramatically in recent years. Almost all these studies have targeted relatively young terrestrial calcite up to Carboniferous in age. To assess the robustness of the carbonate U–Pb chronometer in deep time, we carried out in situ U–Pb analyses in magnesite–ankerite–calcite carbonates in the martian meteorite Allan Hills\n(ALH) 84001. Carbonates in ALH 84001 formed at ca. 3.94 Ga, and there is little evidence that much happened to this rock since then, making\nit an ideal sample to test the robustness of the U–Pb system in old carbonates. We obtained a concordant date of\n3941 ± 49/110 Ma (n=14, MSWD = 2.0), which is identical to the step-leaching Rb/Sr date determined\npreviously. These results thus confirm that old carbonates are amenable to U–Pb dating in samples that have had a relatively simple\nhistory post-carbonate formation.\n","PeriodicalId":12723,"journal":{"name":"Geochronology","volume":"14 1","pages":""},"PeriodicalIF":2.7000,"publicationDate":"2022-12-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"In situ U–Pb dating of 4 billion-year-old carbonates in the martian meteorite Allan Hills 84001\",\"authors\":\"R. Tartèse, I. Lyon\",\"doi\":\"10.5194/gchron-4-683-2022\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Abstract. In situ carbonate U–Pb dating studies have proliferated dramatically in recent years. Almost all these studies have targeted relatively young terrestrial calcite up to Carboniferous in age. To assess the robustness of the carbonate U–Pb chronometer in deep time, we carried out in situ U–Pb analyses in magnesite–ankerite–calcite carbonates in the martian meteorite Allan Hills\\n(ALH) 84001. Carbonates in ALH 84001 formed at ca. 3.94 Ga, and there is little evidence that much happened to this rock since then, making\\nit an ideal sample to test the robustness of the U–Pb system in old carbonates. We obtained a concordant date of\\n3941 ± 49/110 Ma (n=14, MSWD = 2.0), which is identical to the step-leaching Rb/Sr date determined\\npreviously. These results thus confirm that old carbonates are amenable to U–Pb dating in samples that have had a relatively simple\\nhistory post-carbonate formation.\\n\",\"PeriodicalId\":12723,\"journal\":{\"name\":\"Geochronology\",\"volume\":\"14 1\",\"pages\":\"\"},\"PeriodicalIF\":2.7000,\"publicationDate\":\"2022-12-06\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geochronology\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.5194/gchron-4-683-2022\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochronology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.5194/gchron-4-683-2022","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
摘要近年来,原位碳酸盐U-Pb测年研究急剧增加。几乎所有这些研究的目标都是相对年轻的陆地方解石,年龄一直到石炭纪。为了评估碳酸盐U-Pb时计在深部时间的稳健性,我们对火星陨石Allan Hills(ALH) 84001中的菱镁石-铁白云石-方解石碳酸盐进行了原位U-Pb分析。ALH 84001中的碳酸盐形成于约3.94 Ga,几乎没有证据表明这块岩石在那之后发生了什么变化,这使得它成为测试古老碳酸盐中U-Pb系统坚固性的理想样本。我们得到了一个一致的日期3941±49/110 Ma (n=14, MSWD = 2.0),这与之前确定的阶梯浸出Rb/Sr日期相同。因此,这些结果证实,在具有相对简单的后碳酸盐岩形成历史的样品中,古老的碳酸盐适合于U-Pb定年。
In situ U–Pb dating of 4 billion-year-old carbonates in the martian meteorite Allan Hills 84001
Abstract. In situ carbonate U–Pb dating studies have proliferated dramatically in recent years. Almost all these studies have targeted relatively young terrestrial calcite up to Carboniferous in age. To assess the robustness of the carbonate U–Pb chronometer in deep time, we carried out in situ U–Pb analyses in magnesite–ankerite–calcite carbonates in the martian meteorite Allan Hills
(ALH) 84001. Carbonates in ALH 84001 formed at ca. 3.94 Ga, and there is little evidence that much happened to this rock since then, making
it an ideal sample to test the robustness of the U–Pb system in old carbonates. We obtained a concordant date of
3941 ± 49/110 Ma (n=14, MSWD = 2.0), which is identical to the step-leaching Rb/Sr date determined
previously. These results thus confirm that old carbonates are amenable to U–Pb dating in samples that have had a relatively simple
history post-carbonate formation.