- Isotopes of palladium
Naturally-occurring
palladium (Pd) is composed of sixisotope s. The most stableradioisotope s are 107Pd with ahalf-life of 6.5 million years, 103Pd with a half-life of 17 days, and 100Pd with a half-life of 3.63 days. Eighteen other radioisotopes have been characterized withatomic weight s ranging from 92.936 u (93Pd) to 119.924 u (120Pd). Most of these have half-lives that are less than a half an hour except 101Pd (half-life: 8.47 hours), 109Pd (half-life: 13.7 hours), and 112Pd (half-life: 21 hours).The primary
decay mode before the most abundant stable isotope, 106Pd, iselectron capture and the primary mode after isbeta decay . The primarydecay product before 106Pd isrhodium and the primary product after issilver .Radiogenic 107Ag is a decay product of 107Pd and was first discovered in theSanta Clara, California meteorite of1978 . [cite journal
author= W. R. Kelly, G. J. Wasserburg,
title = Evidence for the existence of 107Pd in the early solar system
journal =Geophysical Research Letters
year = 1978
volume = 5
issue =
pages = 1079–1082
doi = ] The discoverers suggest that the coalescence and differentiation of iron-cored small planets may have occurred 10 million years after anucleosynthetic event. 107Pd versus Ag correlations observed in bodies, which have clearly been melted since accretion of thesolar system , must reflect the presence of short-lived nuclides in the early solar system. [cite journal
author= J. H. Chen, G. J. Wasserburg
title = The isotopic composition of Ag in meteorites and the presence of 107Pd in protoplanets
journal =Geochimica et Cosmochimica Acta
year = 1990
volume = 54
issue = 6
pages = 1729–1743
doi = 10.1016/0016-7037(90)90404-9 ]
Standard atomic mass: 106.42(1) uTable
Notes
* The precision of the isotope abundances and atomic mass is limited through variations. The given ranges should be applicable to any normal terrestrial material.
* Geologically exceptional samples are known in which the isotopic composition lies outside the reported range. The uncertainty in the atomic mass may exceed the stated value for such specimens.
* Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
* Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC which use expanded uncertainties.References
* Isotope masses from [http://www.nndc.bnl.gov/amdc/index.html Ame2003 Atomic Mass Evaluation] by G. Audi, A.H. Wapstra, C. Thibault, J. Blachot and O. Bersillon in "Nuclear Physics" A729 (2003).
* Isotopic compositions and standard atomic masses from [http://www.iupac.org/publications/pac/2003/7506/7506x0683.html Atomic weights of the elements. Review 2000 (IUPAC Technical Report)] . "Pure Appl. Chem." Vol. 75, No. 6, pp. 683-800, (2003) and [http://www.iupac.org/news/archives/2005/atomic-weights_revised05.html Atomic Weights Revised (2005)] .
* Half-life, spin, and isomer data selected from these sources. Editing notes on this article's talk page.
** Audi, Bersillon, Blachot, Wapstra. [http://amdc.in2p3.fr/web/nubase_en.html The Nubase2003 evaluation of nuclear and decay properties] , Nuc. Phys. A 729, pp. 3-128 (2003).
** National Nuclear Data Center, Brookhaven National Laboratory. Information extracted from the [http://www.nndc.bnl.gov/nudat2/ NuDat 2.1 database] (retrieved Sept. 2005).
** David R. Lide (ed.), Norman E. Holden in "CRC Handbook of Chemistry and Physics, 85th Edition", online version. CRC Press. Boca Raton, Florida (2005). Section 11, Table of the Isotopes.
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