在土卫六内部条件下对复杂有机物进行实验加热,支持对大气中N2和CH4的贡献

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2025-02-01 DOI:10.1016/j.gca.2024.12.026
K.E. Miller , D.I. Foustoukos , G.D. Cody , C.M. O’D. Alexander
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引用次数: 0

摘要

土卫六大气中丰富的N2和CH4气体是这颗卫星的显著特征,可能有助于限制它的起源和演化。先前的研究表明,大气CH4在地质短时间尺度上损失,可能从内部来源补充。同位素和稀有气体约束表明,N2可能来自NH3冰和有机物加热的混合物。在这里,我们报告了来自Murchison陨石的不溶性有机物和类似的不溶性有机物在与土卫六内部相关的温度和压力下的热液蚀变的实验结果。我们的结果表明,CH4和CO2都可以形成,两者之间的比例取决于多种因素,特别是温度,在较小程度上,水的介电常数和起始材料中的羰基丰度。如果温度高于250°C,土卫六的大气储存库就会产生足够的甲烷。氮主要以NH3的形式挥发,其丰度足以构成泰坦大气中至少50%的N2。挥发物质相对于起始有机物的同位素特征与目前对吸积复杂有机物和土卫六演化大气性质的限制是一致的。
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Experimental heating of complex organic matter at Titan’s interior conditions supports contributions to atmospheric N2 and CH4
Titan’s abundant atmospheric N2 and CH4 gases are notable characteristics of the moon that may help constrain its origin and evolution. Previous work suggests that atmospheric CH4 is lost on geologically short timescales and may be replenished from an interior source. Isotopic and noble gas constraints indicate that N2 may derive from a mixture of NH3 ice and heating of organic matter. Here, we report experimental results from hydrothermal alteration of insoluble organic matter from the Murchison meteorite and analog insoluble organic matter at temperatures and pressures that are relevant to Titan’s interior. Our results indicate both CH4 and CO2 are formed, with the ratio between the two depending on a multitude of factors, particularly temperature and, to a lesser degree, the dielectric constant of water and carbonyl abundance in the starting material. Sufficient CH4 is produced to source Titan’s atmospheric reservoir if temperatures are greater than 250 °C. Nitrogen is volatilized, primarily in the form of NH3, in sufficient abundances to source at least 50 % of Titan’s atmospheric N2. The isotopic characteristics of volatilized material relative to the starting organics are consistent with current constraints for the nature of the accreted complex organics and Titan’s evolved atmosphere.
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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