Roy, Arijit, Singh, Surendra V., Ramachandran, R., Meka, J. K., Ambresh, M., Vijay, T., Janardhan, P., Jayaram, V., Venkatraman, V., Das, A., and others. (2025) Instantaneous formation of interstellar minerals and mineral quantum dots. RSC advances, 15 (16). pp. 12309-12320. E-ISSN 2046-2069. (doi:10.1039/d5ra01088h) (KAR id:109774)
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Language: English
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| Official URL: https://doi.org/10.1039/d5ra01088h |
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Abstract
Our understanding of the formation pathways of interstellar mineral dust is still evolving. This study investigated the formation of astrophysical mineral dust, such as olivine, by shock processing. Low-velocity (∼1.8 km s-1) interstellar shock conditions were simulated using high-intensity shock tubes. These conditions enabled the examination of various cosmic mineral dust precursors such as the mixtures of Mg, Fe and SiO2 under a shock strength of approximately 5.6 M and temperatures around 7300 K. Analysis of the processed samples revealed the presence of Mg-rich olivine, forsterite, MgO quantum dots (QD), and magnetite. These results indicate that shockwaves can rapidly induce dust formation in interstellar space. Furthermore, we demonstrated that shock processing of mineral dust precursors could contribute to the formation of crystalline silicate dust observed in comets and the creation of chondrules, which are observed in chondritic meteorites.
| Item Type: | Article |
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| DOI/Identification number: | 10.1039/d5ra01088h |
| Projects: | Europlanet 2024 RI |
| Subjects: |
Q Science Q Science > QB Astronomy Q Science > QC Physics |
| Institutional Unit: | Schools > School of Engineering, Mathematics and Physics > Physics and Astronomy |
| Former Institutional Unit: |
Divisions > Division of Natural Sciences > Physics and Astronomy
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| SWORD Depositor: | JISC Publications Router |
| Depositing User: | JISC Publications Router |
| Date Deposited: | 28 Apr 2025 09:48 UTC |
| Last Modified: | 22 Jul 2025 09:22 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/109774 (The current URI for this page, for reference purposes) |
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https://orcid.org/0000-0002-4468-8324
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