Physical properties and average atomic numbers of chondrules using computed tomography

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Yogita Kadlag , David Haberthür , Ingo Leya , Ruslan Hlushchuk , Klaus Mezger
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Abstract

Micro-computed tomography is a fast and essentially non-destructive technique for studying 3D properties of solid objects. This study explores the use of a micro-CT technique to determine the physical properties and average atomic numbers of 44 chondrules from unequilibrated (petrologic type 3.00 to 3.6) ordinary, carbonaceous, and enstatite chondrites. Many chondrules deviate from a spherical geometry, implying that they were affected by strain during cooling and prior to complete solidification. The porosity of the studied chondrules ranges from 0.04 vol% to 5.3 vol%. Chondrules from carbonaceous chondrites show the highest porosity and the largest voids. The high porosity could be caused by the presence of oxidized precursors in the chondrule melt that escaped as a gas during high temperature processing and crystallization of the melt. In some chondrules, pores are associated with opaque phases, suggesting their formation either during solidification of metal phases and/or during aqueous alteration. The average atomic numbers of chondrules range from 35 ± 4 to 22 ± 2, independently of porosity and opaque content and is likely controlled by the variation of Mg/Fe in chondrule silicates. The absence of a consistent variation between the degree of deformation, chondrule diameter, and porosity among the studied chondrules from different groups, suggests that the processes responsible for the different physical properties of the chondrules are decoupled from each other and are likely universal to all chondrules.

用计算机断层扫描技术研究球粒的物理性质和平均原子序数
微型计算机断层扫描是研究固体物体三维特性的一种快速且基本上无损的技术。本研究探索了使用微CT技术来确定未平衡(岩石学类型3.00-3.6)普通、碳质和顽火辉石球粒陨石中44个球粒的物理性质和平均原子序数。许多球粒偏离球形几何形状,这意味着它们在冷却期间和完全固化之前受到应变的影响。所研究的球粒的孔隙率在0.04体积%至5.3体积%之间。碳质球粒陨石的球粒显示出最高的孔隙率和最大的空隙。高孔隙率可能是由于球粒熔体中存在氧化的前体,这些前体在熔体的高温加工和结晶过程中以气体形式逸出。在一些球粒中,孔隙与不透明相有关,这表明它们是在金属相凝固和/或水蚀变过程中形成的。球粒的平均原子序数范围为35±4至22±2,与孔隙率和不透明含量无关,可能受球粒硅酸盐中Mg/Fe的变化控制。在不同组的研究球粒之间,变形程度、球粒直径和孔隙率之间没有一致的变化,这表明导致球粒不同物理性质的过程是相互解耦的,并且可能对所有球粒都是普遍的。
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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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