Mg<sub>2</sub>SiO<sub>4</sub> particle aggregation aboard the ISS

نویسندگان

چکیده

Context. Particle aggregation in the solar nebula played a major role framework of planet formation; for example, primitive meteorites and their components formed by different processes. These processes are still not completely understood. Aims. Electrostatic forces probably influenced particle early Solar System. We developed an experiment that was carried out under long-term microgravity conditions aboard International Space Station (ISS) to expand knowledge charge-influenced aggregation. Methods. Aggregation freely floating, elongated, angular, polycrystalline Mg 2 SiO 4 -particles observed while being exposed electric fields as well low- high-energy discharges. Results. Nearly all particles aggregate, which floated sample chamber prior discharge experiments. The aggregate attracted electrodes partly disintegrated low-energy High-energy arc discharges accelerated particles, reassembled chains parallel field lines subsequent between electrodes. A strong shape-preferred orientation longest grain axis -particles. With increasing strength field, narrowed, leading formation compact aggregate. Conclusions. In conditions, electrostatic influence process terms growth rate, morphology, packing density, orientation. observations help us better understand compaction mechanism System aggregates.

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ژورنال

عنوان ژورنال: Astronomy and Astrophysics

سال: 2021

ISSN: ['0004-6361', '1432-0746']

DOI: https://doi.org/10.1051/0004-6361/202141330