Fluids on differentiated asteroids: Evidence from phosphates in differentiated meteorites GRA 06128 and GRA 06129

Paired meteorites Graves Nunatak 06128 and 06129 (GRA) represent an ancient cumulate lithology (4565.9 Ma +/- 0.3) containing high abundances of sodic plagioclase. Textures and stable isotope compositions of GRA indicate that superimposed on the igneous lithology is a complex history of subsolidus reequilibration and low-temperature alteration that may have extended over a period of 150 Myr. In GRA, apatite is halogen-rich with Cl between 4.5 and 5.5 wt% and F between 0.3 and 0.9 wt%. The Cl /(Cl + F + OH) ratio of the apatite is between 0.65 and 0.82. The Cl and F are negatively correlated and are heterogeneously distributed in the apatite. Merrillite is low in halogens with substantial Na in the 6-fold coordinated Na-site (approximate to 2.5%) and Mg in the smaller octahedral site. The merrillite has a negative Eu anomaly, whereas the apatite has a positive Eu anomaly. The chlorine isotope composition of the bulk GRA leachate is + 1.2 parts per thousand relative to standard mean ocean chloride (SMOC). Ion microprobe chlorine isotope analyses of the apatite range between -0.5 and + 1.2 parts per thousand. Textural relationships between the merrillite and apatite, and the high-Cl content of the apatite, suggest that the merrillite is magmatic in origin, whereas the apatite is a product of the interaction between merrillite and a Cl-rich fluid. If the replacement of merrillite by apatite occurred at approximately 800 degrees C, the fluid composition is f(HCl)/f(H2O) = 0.0383 and a HCl molality of 2.13 and f(HCl)/f(HF) = 50-100. It is anticipated that the calculated f(HCl)/f(H2O) and a HCl molality are minimum values due to assumptions made on the OH component in apatite and basing the calculations on the apatite with the lowest X-Cl. The bulk delta Cl-37 of GRA is a > 2 sigma outlier from chondritic meteorites and suggests that parent body processes resulted in fractionation of the Cl isotopes.