Chondrule Destruction via Dust Collisions in Shock Waves
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arXiv
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| Hauptverfasser: | , , |
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| Format: | Preprint |
| Veröffentlicht: |
2024
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| _version_ | 1866916198313099264 |
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| author | Matsumoto, Yuji Kurosawa, Kosuke Arakawa, Sota |
| author_facet | Matsumoto, Yuji Kurosawa, Kosuke Arakawa, Sota |
| contents | A leading candidate for the heating source of chondrules and igneous rims is shock waves. This mechanism generates high relative velocities between chondrules and dust particles. We have investigated the possibility of the chondrule destruction in collisions with dust particles behind a shock wave using a semianalytical treatment. We find that the chondrules are destroyed during melting in collisions. We derive the conditions for the destruction of chondrules and show that the typical size of the observed chondrules satisfies the condition. We suggest that the chondrule formation and rim accretion are different events if they are heated by shock waves. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_05954 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Chondrule Destruction via Dust Collisions in Shock Waves Matsumoto, Yuji Kurosawa, Kosuke Arakawa, Sota Earth and Planetary Astrophysics A leading candidate for the heating source of chondrules and igneous rims is shock waves. This mechanism generates high relative velocities between chondrules and dust particles. We have investigated the possibility of the chondrule destruction in collisions with dust particles behind a shock wave using a semianalytical treatment. We find that the chondrules are destroyed during melting in collisions. We derive the conditions for the destruction of chondrules and show that the typical size of the observed chondrules satisfies the condition. We suggest that the chondrule formation and rim accretion are different events if they are heated by shock waves. |
| title | Chondrule Destruction via Dust Collisions in Shock Waves |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2404.05954 |