Separation of Platinum from Palladium and Iridium in Iron Meteorites and Accurate High-Precision Determination of Platinum Isotopes by Multi-Collector ICP-MS


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Date

2017-12

Publication Type

Journal Article

ETH Bibliography

yes

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Data

Abstract

This study presents a new measurement procedure for the isolation of Pt from iron meteorite samples. The method also allows for the separation of Pd from the same sample aliquot. The separation entails a two-stage anion-exchange procedure. In the first stage, Pt and Pd are separated from each other and from major matrix constituents including Fe and Ni. In the second stage, Ir is reduced with ascorbic acid and eluted from the column before Pt collection. Platinum yields for the total procedure were typically 50–70%. After purification, high-precision Pt isotope determinations were performed by multi-collector ICP-MS. The precision of the new method was assessed using the IIAB iron meteorite North Chile. Replicate analyses of multiple digestions of this material yielded an intermediate precision for the measurement results of 0.73 for ε192Pt, 0.15 for ε194Pt and 0.09 for ε196Pt (2 standard deviations). The NIST SRM 3140 Pt solution reference material was passed through the measurement procedure and yielded an isotopic composition that is identical to the unprocessed Pt reference material. This indicates that the new technique is unbiased within the limit of the estimated uncertainties. Data for three iron meteorites support that Pt isotope variations in these samples are due to exposure to galactic cosmic rays in space.

Publication status

published

Editor

Book title

Volume

41 (4)

Pages / Article No.

633 - 647

Publisher

Wiley-Blackwell

Event

Edition / version

Methods

Software

Geographic location

Date collected

Date created

Subject

Pt isotopes; Pd isotopes; multi-collector ICP-MS; ion-exchange chemistry; iron meteorites

Organisational unit

03946 - Schönbächler, Maria / Schönbächler, Maria check_circle

Notes

Funding

279779 - Accretion and Differentiation of Terrestrial Planets (EC)

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