Saturn’s moon Enceladus has a potentially habitable subsurface water ocean that contains canonical building blocks of life (organic and inorganic carbon, ammonia, possibly hydrogen sulfide) and chemical energy (disequilibria for methanogenesis). However, its habitability could be strongly affected by the unknown availability of phosphorus (P). Here, we perform thermodynamic and kinetic modeling that simulates P geochemistry based on recent insights into the geochemistry of the ocean–seafloor system on Enceladus. We find that aqueous P should predominantly exist as orthophosphate (e.g., HPO
42−), and total dissolved inorganic P could reach 10
−7 to 10
−2 mol/kg H
2O, generally increasing with lower pH and higher dissolved CO
2, but also depending upon dissolved ammonia and silica. Levels are much higher than <10
−10 mol/kg H
2O from previous estimates and close to or higher than ∼10
−6 mol/kg H
2O in modern Earth seawater. The high P concentration is primarily ascribed to a high (bi)carbonate concentration, which decreases the concentrations of multivalent cations via carbonate mineral formation, allowing phosphate to accumulate. Kinetic modeling of phosphate mineral dissolution suggests that geologically rapid release of P from seafloor weathering of a chondritic rocky core could supply millimoles of total dissolved P per kilogram of H
2O within 10
5 y, much less than the likely age of Enceladus’s ocean (10
8 to 10
9 y). These results provide further evidence of habitable ocean conditions and show that any oceanic life would not be inhibited by low P availability.The search for habitable worlds is usually guided by the presence of liquid water. Apart from Earth, water oceans also exist in the subsurface regions of some icy bodies (e.g., Enceladus, Europa, and Titan) in the outer solar system. The evidence for an ocean is strongest at Enceladus, where a water-rich plume erupts from a subsurface ocean (
1,
2). Moreover, habitability is determined by other environmental factors, such as the availability of energy and CHNOPS elements (
3). Data from the Cassini spacecraft indicate that Enceladus’s ocean likely satisfies most of these other requirements for life. For example, the abundance of molecular hydrogen that coexists with CO
2 in the plume suggests the availability of chemical energy that could support methanogens (
4–
6). Carbon dioxide and a variety of organic compounds, which can serve as carbon sources for microorganisms, are also abundant in the plume (
4,
7–
9). Detected ammonia (
4) or organic amines (
8), and tentatively detected hydrogen sulfide (
9,
10), could provide biologically useable nitrogen and sulfur, respectively.However, a notable ingredient for habitability that has eluded detection on Enceladus is phosphorus. In terrestrial life, phosphorus in the form of orthophosphate (PO
43− and its conjugate acids) participates in biological and prebiological reactions. For example, it forms kinetically stable, charged linkages in genetic molecules and phospholipids and is used to transfer metabolic energy primarily via adenosine triphosphate (
11). Phosphorus is essential and its availability is often a limiting factor for biological productivity (
12,
13). Because phosphate is yet to be detected in the Enceladus plume or in Saturn’s E Ring (
14,
15), geochemical modeling is necessary to constrain the availability of this critical nutrient in Enceladus’s ocean. Existing models (
16–
18) predict a very low concentration of phosphate [<10
−10 mol/kg H
2O or molal, vs. ∼10
−6 molal in Earth’s oceans (
19)], which challenges the current perception of Enceladus’s ocean as a habitable environment. However, those models are not based on the latest understanding of the geochemistry of the ocean–seafloor system on Enceladus (
20–
22). In addition to phosphate, reduced forms of phosphorus could be present and might support prebiotic chemistry. Examples include phosphine (PH
3) acquired from the solar nebula (
23) or phosphite (HPO
32− and its conjugate acids) formed from aqueous alteration of accreted chondritic rocks (
24). Neither of these forms of phosphorus have been identified at Enceladus (
10), and it is unknown how stable these species would be in its ocean.Here, we present thermodynamic and kinetic modeling results on the chemical speciation and solubility of phosphorus in Enceladus ocean water. Our results suggest the predominant stability of orthophosphate (vs. instability of reduced forms of P) and relatively high solubility in alkaline and carbonate-rich water.
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