Schulze-Makuch Dirk, Irwin Louis N
Department of Geological Sciences, University of Texas at El Paso, El Paso, TX, USA.
Astrobiology. 2002 Spring;2(1):105-21. doi: 10.1089/153110702753621385.
While Europa has emerged as a leading candidate for harboring extraterrestrial life, the apparent lack of a source of free energy for sustaining living systems has been argued. In this theoretical analysis, we have quantified the amount of energy that could in principle be obtained from chemical cycling, heat, osmotic gradients, kinetic motion, magnetic fields, and gravity in Europa's subsurface ocean. Using reasonable assumptions based on known organisms on Earth, our calculations suggest that chemical oxidation-reduction cycles in Europa's subsurface ocean could support life. Osmotic and thermal gradients, as well as the kinetic energy of convection currents, also represent plausible alternative sources of energy for living systems at Europa. Organisms thriving on these gradients could interact with each other to form the complex energy cycling necessary for establishing a stable ecosystem.
虽然木卫二已成为存在外星生命的主要候选星球,但有人认为其明显缺乏维持生命系统的自由能源。在这项理论分析中,我们已经对原则上可从木卫二地下海洋中的化学循环、热量、渗透梯度、动能、磁场和引力中获取的能量进行了量化。基于地球上已知生物进行合理假设,我们的计算表明,木卫二地下海洋中的化学氧化还原循环可以支持生命存在。渗透梯度和热梯度,以及对流的动能,也代表了木卫二上生命系统可能的替代能源。依赖这些梯度生存的生物可能会相互作用,形成建立稳定生态系统所需的复杂能量循环。