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Thermal metamorphoses of cosmic dust aggregates: experiments by furnace, electrical gas discharge, and radiative heating

机译:宇宙尘埃聚集体的热变质:通过熔炉,气体放电和辐射加热进行的实验

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We experimentally investigated thermal Modifications Of Porous dust aggregates composed of micrometer-sized grains by furnace, electrical discharge, and laser radiation heating. In the furnace, porous SiO2 aggregates of 95% porosity at first underwent Surface diffusion sintering, which led to progressively increasing necking between adjacent particles. Subsequently, viscous flow dissolved the particulate Structure of the still Porous sample, and finally melting occurred. Exposing aggregates of various grain types to electrical discharges dispersed most of the sample and left it thermally unprocessed. Nevertheless, some material was thermally processed to sintered aggregates and a tiny fraction to solidified melt spherules with diameters of less than 180 mu m and most with interior bubbles. In comparison, radiative laser heating turned out to be a much more efficient process to produce melt spherules Of chondrule size, and voids were rarer than in discharge heating. Besides providing, material data for further applications, our work also allows a direct conclusion to be drawn on chondrule formation. Low energetic efficiency and aggregate destruction exclude chondrule formation from loosely-bound aggregates inside hypothetical nebular lightning channels. However, radiative heating of whatever origin, including possible lightning, remains a candidate process of chondrule formation.
机译:我们通过炉子,放电和激光辐射加热,对由微米级颗粒组成的多孔粉尘聚集体的热改性进行了实验研究。在熔炉中,首先对孔隙度为95%的多孔SiO2聚集体进行表面扩散烧结,这导致相邻颗粒之间的颈缩逐渐增加。随后,粘性流溶解了仍然多孔样品的颗粒结构,最终发生了熔化。各种晶粒类型的聚集体受到放电的影响,分散了大部分样品,并且未经热处理。尽管如此,一些材料还是经过热处理加工成烧结的聚集体,而很小的一部分被加工成直径小于180微米且大部分带有内部气泡的凝固的熔融小球。相比之下,辐射激光加热被证明是生产软骨尺寸的熔融小球的更有效的方法,并且与放电加热相比,空隙更罕见。除了为进一步的应用提供材料数据外,我们的工作还可以得出关于球状团簇形成的直接结论。低能效和聚集体破坏会从假设的星状闪电通道内松散结合的聚集体中排除软骨形成。但是,无论起源如何,包括可能的闪电辐射加热,都仍然是软骨形成的候选过程。

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