THE ISOTOPIC COMPOSITION AND ATOMIC-WEIGHT OF MOLYBDENUM

被引：38

作者：

QILU ^{[1
]}

MASUDA, A ^{[1
]}

机构：

[1] UNIV INNER MONGOLIA, HOHHOT, PEOPLES R CHINA

来源：

INTERNATIONAL JOURNAL OF MASS SPECTROMETRY | 1994年 / 130卷 / 1-2期

关键词：

MOLYBDENUM; ISOTOPIC COMPOSITION; ATOMIC WEIGHT; MASS SPECTROMETRY;

D O I：

10.1016/0168-1176(93)03900-7

中图分类号：

O64 [物理化学（理论化学）、化学物理学]; O56 [分子物理学、原子物理学];

学科分类号：

070203 ; 070304 ; 081704 ; 1406 ;

摘要：

The isotopic composition of molybdenum in a shelf reagent standard (MoO3, 99-99%), 13 molybdenites, and three iron meteorites has been determined with a thermal ionization mass spectrometer. No especially-evident variations of molybdenum isotopes among these samples have been found. The mass fractionation of molybdenum occurring in isotopes during the measurements is discussed and our preferred natural abundances of molybdenum isotopes are: Mo-92, 14.7287 +/- 0.001 0; Mo-94, 9.2118 +/- 0.0006; Mo-95, 15.8935 +/- 0.0011; Mo-96, 16.6731 +/- 0.001 1; Mo-97, 9.5692 +/- 0.0007; Mo-98, 24.2289 +/- 0.0017; Mo-100, 9.6950 +/- 0.0007. Thus, the atomic weight of molybdenum is 95.9415 +/- 0.0001 (the value currently accepted by IUPAC [IUPAC Inorganic Chemistry Division, Pure Appl. Chem., 63 (1991) 991] is 95.94 +/- 0.01). The uncertainties correspond to the 95% confidence limit calculated from all the terrestrial and meteoritic samples.

引用

页码：65 / 72

页数：8

共 15 条

[1]

BECKER S, 1981, ISOTIPENPRAXIS, V18, P70

[2] SYNTHESIS OF THE ELEMENTS IN STARS [J].