3D porosity, flow, and transport characteristics of two L chondrites reveal wet accretion-related cosmic web-like porosity

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Planetary and Space Science Pub Date : 2024-05-24 DOI:10.1016/j.pss.2024.105915
A.-J. Soini , I.T. Kukkonen , H. Suhonen , B. Lukić , A.V. Luttinen
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Abstract

Porosity, with its structure-dependent flow properties (permeability and tortuosity) and transport properties (thermal conductivity and thermal diffusivity), is closely related to the accretion, thermal metamorphism, and associated hydrothermal alteration of ordinary chondrite (OC) parent bodies. Using synchrotron radiation microtomography (SRμCT), we reveal the varying porosity structures in two L chondrite falls of low (Mezö-Madaras L3.7) and high (Bath Furnace L6) petrologic types and quantify porosity properties, such as shape and connectivity, and related effective permeability and tortuosity factor. Although the two specimens demonstrate similar effective permeabilities, they exhibit significantly different tortuosity factors and textures of porosity, which include notable differences in void throat diameters, complexity and density of the interconnected void network, heterogeneity in void distribution, and the extent of primary and secondary porosity. The complex relationships among porosity, permeability, tortuosity, and thermal conductivity can be explained by the varying void arrangements related to varying grain sizes among the petrologic types of OCs, which in turn reflect their varying evolutionary paths.

Electron microprobe and attached energy-dispersive X-ray spectrometer reveal signs of hydrothermal alteration in both petrologic types. High-energy SRμCT imaging (0.65 μm voxel size) reveals the presence of a new microporosity substructure resembling a microscopic cosmic web, which may be linked to fluid-assisted metamorphism and hydrothermal alteration during wet accretion of the parent body. Furthermore, the proportion of this continuous porosity may be related to the temperatures associated with different petrologic types, and the wet accretion model may resolve the lack of correlation between petrologic types and porosity of OCs. Finally, the uncovered cosmic web-like microporosity structure may explain the observed concurrent high thermal conductivity, low permeability, and high porosity of the high-petrologic-type OCs.

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两块L型软玉的三维孔隙度、流动和传输特征揭示了与湿吸积有关的宇宙网状孔隙度
孔隙度及其与结构相关的流动特性(渗透性和曲折度)和传输特性(热导率和热扩散率)与普通软玉母体的吸积、热变质和相关热液蚀变密切相关。利用同步辐射显微层析技术(SRμCT),我们揭示了低岩石类型(Mezö-Madaras L3.7)和高岩石类型(Bath Furnace L6)的两块L型软玉坠落物的不同孔隙结构,并量化了孔隙特性(如形状和连通性)以及相关的有效渗透率和曲折系数。虽然两个试样显示出相似的有效渗透率,但它们表现出明显不同的迂回系数和孔隙度质地,其中包括明显不同的孔喉直径、相互连接的孔隙网络的复杂性和密度、孔隙分布的异质性以及一级和二级孔隙度的程度。孔隙度、渗透率、迂回度和导热率之间的复杂关系可以通过不同岩石学类型的 OCs 中与不同晶粒大小相关的不同空隙排列来解释,这反过来又反映了它们不同的演化路径。高能 SRμCT 成像(体素尺寸为 0.65 μm)显示出一种新的微孔子结构,类似于微观宇宙网,这可能与母体湿吸积过程中的流体辅助变质作用和热液蚀变有关。此外,这种连续孔隙度的比例可能与不同岩石类型的相关温度有关,湿吸积模型可以解决岩石类型与 OCs 孔隙度之间缺乏相关性的问题。最后,未发现的宇宙网状微孔结构可以解释所观测到的高岩石类型 OC 同时具有的高导热性、低渗透性和高孔隙度。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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