Instantaneous formation of interstellar minerals and mineral quantum dots

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<sup>-1</sup>) 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 SiO<sub>2</sub> 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.

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Publication Details

Journal
RSC Advances
Published
2025-01-01
DOI
https://doi.org/10.1039/d5ra01088h
Citations
3
Primary Topic
High-pressure geophysics and materials
Type
article
Field-Weighted Citation Impact
5.60

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article

Instantaneous formation of interstellar minerals and mineral quantum dots

M. Ambresh, Helene Z. Hill, Bhalamurugan Sivaraman, J. K. Meka et al.
3 citations
RSC Advances
High-pressure geophysics and materials
5.60
article

Instantaneous formation of interstellar minerals and mineral quantum dots

M. Ambresh, Helene Z. Hill, Bhalamurugan Sivaraman, J. K. Meka, Vijay Thiruvenkatam, Vankudoth Jayaram, Nigel John Mason, Anil Bhardwaj, Surendra V. Singh, R. Ramachandran, Arijit Roy, Ankan Das, V. Venkatraman, P. Janardhan
article en
3 citations

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<sup>-1</sup>) 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 SiO<sub>2</sub> 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.

RSC AdvancesVol. 15(16)
International Space University (FR), Physical Research Laboratory (IN), University of Kent (GB), Indian Institute of Technology Gandhinagar (IN), Indian Institute of Science Bangalore (IN), Vikram Sarabhai Space Centre (IN)
Indian Institute of Science, Indian National Science Academy
Openalex Percentile: Top 5%
High-pressure geophysics and materials
5.60
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