Owing
to the extremely low abundance of silver in the Earth’s
crust and mantle, it remains a major challenge to eliminate matrix
impurities to obtain accurate silver isotopic compositions in silicate
rocks. To determine precise and accurate silver isotopic data in silicates,
we have modified the traditional pretreatment procedures, assessed
isobaric interference and matrix effects, and analyzed silver isotopic
compositions in silicates. By modification of the silicate digestion
and ion-exchange procedures, efficient elution of silver was achieved.
The doping experimental results indicated that the matrix effect induced
by Ti and Cr could be satisfactorily corrected using the internal
standard Pd isotope pair of 108Pd–106Pd. The modified chemical chromatographic method effectively separates
Ni from Ag in silicate samples, thereby minimizing the significant
isobaric interference from Ni cations. As a result, the shifts in
the δ109Ag value caused by cations can be corrected
to less than 0.02‰. There are considerable shifts down to −0.82‰
in δ109Ag from the accepted δ109Ag value when soluble metasilicate is present in the solution, which
might explain the discrepancies in measured δ109Ag
values for silicate materials. To accurately analyze silver isotopic
compositions, especially of silicates with extremely low silver abundance,
a silver standard doping method with an optimum doping proportion
(sample-to-standard material ratio of 2:8) has been shown to produce
an acceptable measurement uncertainty from 0.04 to 0.06‰ (2SD).
The high-precision δ109Ag value determined in this
study for ultramafic rocks from Balmuccia and the basalt reference
material, BHVO-2, of −0.044 ± 0.062‰ is consistent
with that of −0.16 ± 0.07‰ reported by previous
studies. Our study paves the way for the more extensive use of silver
isotopes in studies of terrestrial/extraterrestrial rocks, something
that will be of help in constraining the sources of precious metals
in polymetallic ore deposits as well as core formation and volatile-element
depletion in the early solar system.