Abstract

The nature of mineral precipitations in terrestrial alkaline soda lakes provides insights into the water chemistry of subsurface oceans on icy bodies in the outer solar system. Saturation analyses of terrestrial alkaline lakes have shown that the solution chemistries of lake waters are generally controlled by the presence of monohydrocalcite (MHC) and amorphous Mg-carbonate (AMC). However, direct observations of the formation of these metastable carbonates in natural alkaline lakes have been limited. This study provides evidence of in situ MHC formation in alkaline lakes, based on the water chemistry and mineralogy of suspended matter in Olgoy, Boon Tsagaan, and Orog Lakes (Valley of Gobi Lakes, Mongolia). The solution chemistries were close to saturation with respect to MHC and AMC, consistent with other alkaline lakes worldwide. Suspended matter was separated by the ultracentrifugation of lake water following freeze-drying. Our results show that MHC is the common mineral phase in the suspended matter. These observations confirm that MHC is the direct authigenic product of evaporation in alkaline lakes. The carbonate fraction in suspended matter from Olgoy Lake has a Mg/Ca ratio of 0.4, suggesting the formation of AMC in association with MHC. Based on the dissolution equilibria of AMC and MHC, we predict the Mg2+, Ca2+, and total dissolved carbonate concentrations in Enceladus’ ocean to be ~1 mmol/kg, ~10 μmol/kg, and 0.06–0.2 mol/kg, respectively, in the presence of AMC and MHC. We propose that the measurements of Mg contents in plumes will be key to constraining the total dissolved carbonate concentrations and chemical affinities of subsurface oceans on Enceladus and other alkaline-carbonate ocean worlds.

Highlights

  • The multiple ocean worlds in the outer solar system are icy bodies with subsurface liquid oceans beneath their icy crusts [1,2]

  • We investigated the water chemistries and mineralogical compositions of suspended matter in three alkaline lakes of the Valley of Gobi Lakes

  • The solution chemistries of the lake waters were close to saturation with respect to MHC and amorphous Mg-carbonate (AMC), consistent with other alkaline lakes worldwide

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Summary

Introduction

The multiple ocean worlds in the outer solar system are icy bodies with subsurface liquid oceans beneath their icy crusts [1,2]. The water chemistries of subsurface oceans on icy bodies that formed from ultramafic (e.g., chondritic) rocks beyond the CO2 snowline [3] should be saline, carbonate-rich, and have high pH [4,5,6,7,8], suggesting Na± , Cl− , CO3 2− , and HCO3 − as major dissolved species. This finding suggests that the carbonate phases initially formed directly from the lake water in alkaline lakes must be MHC and AMC, which are subsequently transformed into calcite and magnesite, respectively, after sedimentation The occurrence of this process would have affected the water chemistry on ocean worlds. We provide evidence for the in situ formation of MHC in terrestrial alkaline lakes, based on analyses of the water chemistries and the solid mineralogical compositions of the suspended matter in lake water from three alkaline lakes: Olgoy, Boon Tsagaan, and Orog Lakes (Valley of Gobi Lakes, central Mongolia)

Study Area
Methods
Water Chemistry
25 August 2015
Relationship between the activity
Mineralogy of Suspended Matter
Ch C Ch
Implications for the Water Chemistry of Enceladus’ Ocean
Conclusions
Full Text
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