JpGU-AGU Joint Meeting 2017

講演情報

[JJ] ポスター発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS10] [JJ] 太陽系における惑星物質の形成と進化

2017年5月22日(月) 13:45 〜 15:15 ポスター会場 (国際展示場 7ホール)

コンビーナ:臼井 寛裕(東京工業大学地球生命研究所)、宮原 正明(広島大学理学研究科地球惑星システム学専攻)、山口 亮(国立極地研究所)、癸生川 陽子(横浜国立大学 大学院工学研究院 機能の創生部門)

[PPS10-P06] Development of Laser Post-Ionization SNMS for In-Situ U-Pb chronology

*松田 貴博1河井 洋輔1宮 晃平1青木 順1本堂 敏信1石原 盛男1豊田 岐聡1中村 亮介2寺田 健太郎1 (1.大阪大学大学院理学研究科、2.大阪大学産学連携本部)

キーワード:U-Pb年代分析、SIMS、SNMS

In space and planetary sciences, Secondary Ion Mass Spectrometer (SIMS) has been widely used for isotopic analyses at the micron scale. In the SIMS analysis, the surface of a sample is irradiated by a primary ion beam, and secondary ions of the sputtered materials are introduced into the mass spectrometer. However, the secondary ion yield of SIMS is very low (less than a few %). As a result, a large amount of material is wasted as neutral particles. In order to improve this disadvantage, we have been developing a Sputtered Neutral Mass Spectrometer (SNMS) with a femto-second laser.
The instrument consists of a focused ion beam system with a liquid metal gallium ion source (Ga-FIB) to attain an ultrahigh lateral resolution less than 1μm. After a sputtering by Ga-FIB, the sputtered secondary particles are ionized by irradiating the femto-second laser. The post-ionized ions are introduced into the multi-turn ToF analyzer (MULTUM) which achieves ultrahigh mass resolving power of 20000. In addition, we introduced a new detection method, ion counting system, to improve the detection sensitivity. As a result of measurement of a standard sample in U-Pb chronology, 91500 zircon (concentration of uranium is about 100 ppm), the signal peaks of uranium and uranium oxides could be detected, so we have confirmed that the detection limit of the present system is 100 ppm.
In this study, we measured cyrtolite which contains a high concentration of uranium (2 wt.%) and 91500 zircon to confirm whether SNMS can be applied to in-situ U-Pb chronology. As a result of measuring two samples, uranium, uranium oxides and lead signal peaks were detected. In addition, signal peaks of interfering ions, for example, hafnium oxides and gallium clusters, were separated from the peaks of lead by increasing the number of cycles in MULTUM. After the measurement, the diameter of the sputtered area was about 1μm. In this presentation, we will report the present performance of SNMS in in-situ U-Pb chronology.