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Phosphate availability and implications for life on ocean worlds

Space Sciences

Phosphate availability and implications for life on ocean worlds

N. G. Randolph-flagg, T. Ely, et al.

Dive into the fascinating exploration of subsurface oceans on moons in our outer solar system, as researchers Noah G. Randolph-Flagg, Tucker Ely, Sanjoy M. Som, Everett L. Shock, Christopher R. German, and Tori M. Hoehler reveal that these hidden worlds might harbor enough phosphate to support life, surpassing even Earth's deep oceans.... show more
Abstract
Several moons in the outer solar system host liquid water oceans. A key next step in assessing the habitability of these ocean worlds is to determine whether life’s elemental and energy requirements are also met. Phosphorus is required by all known life and is often limited to biological productivity in Earth’s oceans. This raises the possibility that its availability may limit the abundance or productivity of Earth-like life on ocean worlds. To address this potential problem, here we calculate the equilibrium dissolved phosphate concentrations associated with the reaction of water and rocks—a key driver of ocean chemical evolution—across a broad range of compositional inputs and reaction conditions. Equilibrium dissolved phosphate concentrations range from 10⁻¹¹ to 10⁻¹⁴ mol/kg for the range of carbonaceous chondrite compositions and reaction conditions considered, but are generally >10⁻⁵ mol/kg for most plausible scenarios. Relative to the phosphate requirements and uptake kinetics of microorganisms in Earth’s oceans, such concentrations would be sufficient to support initially rapid cell growth and construction of global ocean cell populations larger than those observed in Earth’s deep oceans.
Publisher
Nature Communications
Published On
Apr 25, 2023
Authors
Noah G. Randolph-Flagg, Tucker Ely, Sanjoy M. Som, Everett L. Shock, Christopher R. German, Tori M. Hoehler
Tags
moons
ocean worlds
subsurface oceans
phosphate
habitability
life support
water-rock reactions
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