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School of Engineering and Science - Jacobs University

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The case <strong>of</strong> Ni determinations in carbonates has been mentioned previously,<br />

<strong>and</strong> the conclusion is that accurate Ni determinations in Ca- <strong>and</strong> Mg-rich rocks are<br />

only possible in HNO 3 acid matrices <strong>and</strong> by utilizing the 62 Ni isotope. Figures A2.1<br />

through A2.4 illustrate the numerous Ca <strong>and</strong> Mg interferences on 60 Ni <strong>and</strong> 62 Ni.<br />

Additionally, Figure A2.5 demonstrates that Al 2 O 3 abundances typical for shales (10-<br />

15%) that are analyzed in 0.5 M HCl are expected to contribute 2-3 mg/kg to the<br />

measured Ni concentration. The data suggest that 62 Ni, when measured in a HNO 3<br />

acid matrix, <strong>of</strong>fers the best isotope for Ni determinations in Mg-,Ca-, <strong>and</strong> Al-rich<br />

samples. However, 62 Ni is a low abundance isotope <strong>of</strong> Ni (3.63%), <strong>and</strong> will produce a<br />

relatively low signal response during ICPMS measurements, <strong>and</strong> this factor must be<br />

considered during attempts to quantify Ni.<br />

Figure A2.6 illustrates significant interferences on 88 Sr due to various Ca <strong>and</strong><br />

presumed Ar species ( 40 Ca 48 Ca, 40 Ar 48 Ca, <strong>and</strong> 44 Ca 44 Ca). These interferences exist<br />

regardless <strong>of</strong> the acid matrix used to prepare the samples for ICPMS analysis.<br />

Concentrations <strong>of</strong> Sr in many rocks are in the range <strong>of</strong> 50 to several hundred mg/kg<br />

(App. 1), <strong>and</strong> as Ca <strong>and</strong> Sr are both alkaline earth metals, their concentrations in<br />

many rocks vary proportionally. As a result, even though high Ca contents may<br />

produce an interference <strong>of</strong> 1-3 mg/kg on Sr, this frequently is <strong>of</strong> no great significance<br />

as Sr concentrations themselves may be high in the sample (e.g., ~115 mg/kg in the<br />

case <strong>of</strong> the JDo-1 dolomite).<br />

Interferences on Y due to high Fe contents in samples are presented in Figure<br />

A2.7 for informative purposes only. The impact <strong>of</strong> these interferences is likely to be<br />

small (~0.10 mg/kg) relative to typical Y contents in rocks (~10-50 mg/kg, see App.<br />

1), <strong>and</strong> will not be discussed further.<br />

Figures A2.8 <strong>and</strong> A2.9 demonstrate that significant interferences due to Mn<br />

<strong>and</strong> Fe may adversely impact determinations <strong>of</strong> Zr. The 90 Zr isotope suffers an<br />

interference <strong>of</strong> several mg/kg in 0.5 M HCl due to 55 Mn 35 Cl (Fig. A2.8). The effects<br />

<strong>of</strong> high Fe contents on measurements <strong>of</strong> 91 Zr are much greater due to 56 Fe 35 Cl, <strong>and</strong><br />

interferences <strong>of</strong> 10-20 mg/kg would be expected in Fe-rich samples such as IFs (Fig.<br />

A2.9). Smaller, but still significant effects are noted for 40 Ca 16 O 35 Cl interferences on<br />

91 Zr. These effects would be minimized by the use <strong>of</strong> HNO 3 as the diluting acid.<br />

Based upon these observations, the 91 Zr isotope is not recommended for most rock<br />

types, unless the use <strong>of</strong> HCl is avoided, or if Ca- <strong>and</strong> Fe-poor, Mn-rich samples<br />

require analysis.<br />

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