Theoretical study on crystallization process from chondrule melt using phase-field method
Project/Area Number |
23740330
|
Research Category |
Grant-in-Aid for Young Scientists (B)
|
Allocation Type | Multi-year Fund |
Research Field |
Solid earth and planetary physics
|
Research Institution | Nagoya City University (2013) Tohoku University (2011-2012) |
Principal Investigator |
MIURA Hitoshi 名古屋市立大学, その他の研究科, 准教授 (50507910)
|
Project Period (FY) |
2011 – 2013
|
Project Status |
Completed (Fiscal Year 2013)
|
Budget Amount *help |
¥4,290,000 (Direct Cost: ¥3,300,000、Indirect Cost: ¥990,000)
Fiscal Year 2013: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2012: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2011: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
|
Keywords | コンドリュール / 結晶成長 / 凝固組織 / 組成累帯構造 / フェーズフィールド法 / 棒状カンラン石組織 / 急冷凝固 / Mg-Feオリビン / 偏析 / 初期トランジェント / 累帯構造 / 冷却速度 / 成長速度依存性 / 界面不安定 / 成長速度異方性 |
Research Abstract |
Chondrules are millimeter-sized, once-molten, spherical-shaped grains mainly composed of silicate material. They are considered to have formed from chondrule precursor particles that were heated and melted through flash heating events in the solar nebula and cooled again to solidify in a short period of time. To elucidate the formation process of their solidification textures, we carried out numerical simulations of solidification of olivine based on the phase-field method. The formation of barred-olivine texture can be explained by the morphological instability of solid-liquid interface during the rapid cooling. It was found that a cooling rate required to reproduce the typical width of olivine bars is about two orders of magnitude larger than that suggested previously. We also showed that the linear chemical zoning observed in overgrowth layer of olivine phenocryst have formed by such rapid cooling.
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Report
(4 results)
Research Products
(52 results)