Outbursts Upon Cooling of Low-Temperature Binary Mixtures: Experiments and Their Planetary Implications

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Journal of Geophysical Research: Planets Pub Date : 2024-10-05 DOI:10.1029/2024JE008457
S. M. Raposa, A. E. Engle, S. P. Tan, W. M. Grundy, J. Hanley, G. E. Lindberg, O. M. Umurhan, J. K. Steckloff, C. L. Thieberger, S. C. Tegler
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Abstract

For many binary mixtures, the three-phase solid-liquid-vapor equilibrium curve has intermediate pressures that are higher than the pressure at the two pure triple points. This curve shape results in a negative slope in the high-temperature region near the triple point of the less volatile component. When freezing mixtures in the negative slope regime, fluid trapped below confined ice has latent heat released with more vapor upon cooling, and thus increases in pressure. If the rising pressure of the confined fluid overcomes the strength of the confining solid, which may be its own ice, it can produce an abrupt outburst of material and an increase in the system's overall pressure. Here, we report experimental results of freezing-induced outbursts occurring in the N2/CH4, CO/CH4, and N2/C2H6 systems, and provide insight into the phenomenon through a thermodynamics perspective. We also propose other binary systems that may experience outbursts and explore the geological implications for icy worlds such as Titan, Triton, Pluto and Eris as well as rocky bodies, specifically Earth and Mars.

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低温二元混合物冷却时的爆发:实验及其行星影响
对于许多二元混合物,三相固液汽平衡曲线的中间压力高于两个纯三相点的压力。这种曲线形状导致在靠近挥发性较低组分三相点的高温区域出现负斜率。在负斜率条件下冷冻混合物时,被困在封闭冰下的流体在冷却时会释放出更多蒸汽潜热,从而增加压力。如果受限流体上升的压力超过了受限固体(可能是其本身的冰)的强度,就会产生突然的物质喷发,并增加系统的整体压力。在此,我们报告了在 N2/CH4、CO/CH4 和 N2/C2H6 系统中发生的冻结诱发爆发的实验结果,并从热力学的角度对这一现象进行了深入分析。我们还提出了其他可能发生爆发的双星系统,并探讨了对土卫六、海卫一、冥王星和阋神星等冰质世界以及地球和火星等岩质天体的地质影响。
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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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