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Reproduction of Chondrule from Levitated, Hypercooled Silicate Melts.

Reproduction of Chondrule from Levitated, Hypercooled Silicate Melts.
从悬浮的过冷硅酸盐熔体中再现球粒。
批准号:
16340163
负责人:
TSUKAMOTO Katsuo
金额:
$4.61万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (B)
财政年份:
2004
资助国家:
日本
项目状态:
已结题
起止时间:
2004 至 2005

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中文摘要
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英文摘要
Olivine ((Mg, Fe)_2SiO_4) and pyroxene ((Mg, Fe)SiO_3) chondrules have been successfully synthesized for the first time from levitated melt droplets. Solidification experiments have been performed by the use of a gas jet levitation system.In the case of levitated melts, the homogeneous nucleation required a large degree of supercooling (forsterite-Mg_2SiO_4 : ΔT【greater than or equal】1000 K) or was not possible at all (enstatite-MgSiO_3). In the latter case, only vitrification was observed even for long experiment times (t>1000 sec).These points out that heterogeneous nucleation centers have played a key role for the crystallization of meteoritic material during the formation of the early solar nebula. The most likely possibility for heterogeneous nucleation would have been the collision of the melt droplets with cosmic dusts, which had been universally present around chondrule formation.Although it was formerly assumed that the crystallization of chondrules was a slow process near equilibrium conditions, the present levitation data clearly demonstrates that crystallization of chondrule melts takes place in less than 10 seconds at a supercooling of approximately 700-1000 K for olivine chondrules and of 650-860 K for pyroxene chondrules.By collision with cosmic dusts, the chondrules have been crystallized from a hypercooled melt (about ΔT>500 K). In hypercooled melts, facetted crystals, like the ones present in porphyritic textures, can be formed because the hypercooled melt acts as a heat sink for the absorption of the latent heat of crystallization.A new cooling model for the chondrule formation is proposed based on the crystallization from hypercooled melts, in which the cooling rate of chondrules and the time, until the collision with cosmic dust particles, was considered. According to this model, a cooling rate larger than 100 K/s is needed for a melt droplet to realize crystallization. This is about 1000 times faster than previous models suggested.
期刊论文(22)
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会议论文
格子欠陥発生機構の解明に向けたたんぱく質結晶表面の高分解光学観察
蛋白质晶体表面的高分辨率光学观察阐明晶格缺陷产生的机制
DOI: --
发表时间: 2005
期刊: 応用物理 74
影响因子: --
作者: [佐崎元, 松井拓郎, 塚本勝男, 中嶋一雄]
通讯作者: 中嶋一雄
Growth mechanism of meteoritic fine olivine particles from rapidly cooled silicate vapor
快速冷却硅酸盐蒸气中陨石细橄榄石颗粒的生长机制
DOI: --
发表时间: 2006
期刊: Grain Formation Workshop 24(印刷中)
影响因子: --
作者: [H Kobatake, K.Tsukamoto, Jyun Nozawa, Hisao Satoh]
通讯作者: Hisao Satoh
古地磁気情報としてのシュードタキライト・隕石
作为古地磁信息的伪速石和陨石
DOI: --
发表时间: 2005
期刊: 地学雑誌 114
影响因子: --
作者: [中村教博, 植原稔]
通讯作者: 植原稔
DOI: --
发表时间: 2005
期刊: Journal of Crystal Growth 277
影响因子: --
作者: [C.Li, K.Tsukamoto, H.Satoh]
通讯作者: H.Satoh
16
    A Precursor for Chiral Separation during Crystallization
    • 批准号:
      23656005
    • 项目类别:
      Grant-in-Aid for Challenging Exploratory Research
    • 资助金额:
      $2.41万
    • 财政年份:
      2011
    • 负责人:
      TSUKAMOTO Katsuo
    • 依托单位:
    Ultra-high Speed Crystallization in the Primitive Solar System
    • 批准号:
      22244066
    • 项目类别:
      Grant-in-Aid for Scientific Research (A)
    • 资助金额:
      $29.04万
    • 财政年份:
      2010
    • 负责人:
      TSUKAMOTO Katsuo
    • 依托单位:
    海外基金