Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, Mountain View, CA, USA.
NASA Postdoctoral Program, Universities Space Research Association, Columbia, MD, USA.
Nat Commun. 2023 Apr 25;14(1):2388. doi: 10.1038/s41467-023-37770-9.
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 to 10mol/kg across the full range of carbonaceous chondrite compositions and reaction conditions considered, but are generally > 10mol/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.
在外太阳系的几颗卫星上都存在着液态水海洋。评估这些海洋世界宜居性的下一步关键是确定生命的基本要素和能量需求是否也能得到满足。磷是所有已知生命所必需的,而且通常在地球海洋中的生物生产力方面受到限制。这就提出了一种可能性,即其可用性可能会限制类似地球的海洋世界上生命的丰度或生产力。为了解决这个潜在问题,我们在这里计算了与水和岩石反应相关的平衡溶解磷酸盐浓度,这是海洋化学演化的关键驱动因素——在广泛的组成输入和反应条件下进行了计算。在考虑的所有碳质球粒陨石组成和反应条件范围内,平衡溶解磷酸盐浓度的范围从 10 到 10mol/kg,但对于大多数合理的情况,通常> 10mol/kg。与地球海洋中微生物的磷酸盐需求和吸收动力学相比,这种浓度足以支持最初的快速细胞生长和构建全球海洋细胞群体,其规模大于地球深海中观察到的群体。