TY - JOUR
T1 - Oxygen stable isotope fractionation behavior of cerussite and hydrocerussite
T2 - New results and reconciliation of the recent literature
AU - Melchiorre, Erik B.
AU - Gilg, H. Albert
N1 - Funding Information:
The authors thank the donors of the American Chemical Society Petroleum Research Fund for support of this work through a Type B research grant. Support was also provided by a NASA Astrobiology Institute Minority Institution Research Sabbatical (NAI-MIRS) program award to the lead author. Instrumentation was provided and supported by National Science Foundation EAR-0243135 (stable isotope mass spectrometer) and EAR-0941106 (SEM/EDS upgrade). We thank Karen Meech and Gary Huss of the Astrobiology Institute at University of Hawaii for access to instrumentation and valuable discussions. Christian Rewitzer provided photography assistance, and U. Struck of the Museum für Naturkunde, Berlin, Germany provided some isotope analyses.
PY - 2011/6/1
Y1 - 2011/6/1
N2 - Recent empirical and theoretical calculations of the temperature-dependant oxygen stable isotope fractionation behavior of cerussite have highlighted potential problems with earlier work on this topic. The synthetic cerussite which was used earlier by the lead author to determine fractionation factors was re-examined using energy dispersive X-ray analysis, and found to be internally contaminated with inclusions of the phase hydrocerussite at levels of 5-10% by volume. The volume of hydrocerussite present within the samples is not sufficient to explain the entire discrepancy between this work and the empirical and theoretical calculations made earlier by the second author of this paper. Regardless of the exact causes of experimental failure or kinetic effects, the hydrocerussite contamination and the difficulty of demonstrating that these experiments reached isotopic equilibrium suggest that the use of cerussite oxygen isotope fractionation factors determined by slow precipitation experiments be discontinued in favor of the empirically calibrated fractionation factor 1000lnαcerussite-water=2.29(106/T2)-3.56. In addition, we have determined that the oxygen isotope fractionation factor between hydrocerussite and water at 20°C is 1.0232.
AB - Recent empirical and theoretical calculations of the temperature-dependant oxygen stable isotope fractionation behavior of cerussite have highlighted potential problems with earlier work on this topic. The synthetic cerussite which was used earlier by the lead author to determine fractionation factors was re-examined using energy dispersive X-ray analysis, and found to be internally contaminated with inclusions of the phase hydrocerussite at levels of 5-10% by volume. The volume of hydrocerussite present within the samples is not sufficient to explain the entire discrepancy between this work and the empirical and theoretical calculations made earlier by the second author of this paper. Regardless of the exact causes of experimental failure or kinetic effects, the hydrocerussite contamination and the difficulty of demonstrating that these experiments reached isotopic equilibrium suggest that the use of cerussite oxygen isotope fractionation factors determined by slow precipitation experiments be discontinued in favor of the empirically calibrated fractionation factor 1000lnαcerussite-water=2.29(106/T2)-3.56. In addition, we have determined that the oxygen isotope fractionation factor between hydrocerussite and water at 20°C is 1.0232.
UR - http://www.scopus.com/inward/record.url?scp=79955463541&partnerID=8YFLogxK
U2 - 10.1016/j.gca.2011.03.013
DO - 10.1016/j.gca.2011.03.013
M3 - Article
AN - SCOPUS:79955463541
SN - 0016-7037
VL - 75
SP - 3191
EP - 3195
JO - Geochimica et Cosmochimica Acta
JF - Geochimica et Cosmochimica Acta
IS - 11
ER -