Courville Samuel W, Castillo-Rogez Julie C, Daswani Mohit Melwani, Robare Jordyn, O'Rourke Joseph G
School of Earth and Space Exploration, Arizona State University, 781 Terrace Mall, Tempe, AZ 85287, USA.
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91011, USA.
Sci Adv. 2025 Aug 22;11(34):eadt3283. doi: 10.1126/sciadv.adt3283. Epub 2025 Aug 20.
Ceres's surface mineralogy and density structure indicate an aqueous past. Observations from the Dawn mission revealed that Ceres likely hosted a global subsurface ocean in its early history, which was the site of pervasive aqueous alteration of accreted material. Subsurface environmental constraints inferred from Ceres's surface mineralogy, combined with Ceres's high abundance of carbon, suggest that the dwarf planet may have been habitable for microbial life. We present a coupled chemical and thermal evolution model tracking Ceres's interior aqueous environment through time. If the rocky interior reached ≳550 K, then fluids released by rock metamorphism would have promoted conditions favorable for habitability by introducing redox disequilibrium into the ocean, a source of chemical energy for chemotrophs. We find that this period would have been between ~0.5 and 2 billion years after Ceres's formation. Since then, Ceres's ocean has likely become a cold, concentrated brine with fewer sources of energy, making it less likely to be habitable at present.
谷神星的表面矿物学和密度结构表明它有过含水的过去。“黎明号”任务的观测结果显示,谷神星在其早期历史中可能存在一个全球地下海洋,这里是吸积物质普遍发生水蚀变的场所。从谷神星的表面矿物学推断出的地下环境限制,再加上谷神星高丰度的碳,表明这颗矮行星可能曾适合微生物生存。我们提出了一个化学和热演化耦合模型,用以追踪谷神星内部水环境随时间的变化。如果岩石内部温度达到≳550K,那么岩石变质作用释放的流体就会通过向海洋引入氧化还原不平衡(这是化学自养生物的化学能量来源)来促进有利于宜居性的条件。我们发现这个时期可能在谷神星形成后的约0.5至20亿年之间。从那时起,谷神星的海洋可能已经变成了一个寒冷、浓缩的卤水,能量来源较少,因此目前它不太可能适合居住。