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Physical and Chemical Evolution of Dust Aggregate and their Physical Properties in the Primordial Solar Nebula

Physical and Chemical Evolution of Dust Aggregate and their Physical Properties in the Primordial Solar Nebula
原始太阳星云尘埃聚集体的物理化学演化及其物理性质
批准号:
07640640
负责人:
KOZASA Takashi
金额:
$1.22万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
1995
资助国家:
日本
项目状态:
已结题
起止时间:
1995 至 1996

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中文摘要
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英文摘要
The following subject had been investigated during the period supported by this grant.(1) Scattering properties and their dependence on the strusture and the chemical composition of dust aggregates : The discrete dipole approximation was applied to investigate the dependence of the scattering properties on the structure and the chemical composition of dust aggregates. The results show that the behavior of forward scattered light clearly reflects the overall size and the mean chemical composition of dust aggregates, otherwise the backward scattering is sensitive to the roughness of surface layr of dust aggregates.(2) Formation process of dust aggregates in the primordial solar nebula : A method was discussed to treat the formation process and the resulting structure of dust aggregates self-consistently in the primordial solar nebula, but the detailed calculation was not performed.(3) The crystallinity of silicate component in comet dust : On the basis of the Greenberg's interstellar dust model, the origin of crystalline silicate component in cometary dust was investigated ; in comparison with the observation of comet P/Halley the crystalline component was estimated to be the order of 10 to 20% in volume. The estimated value can be realized by the mechanism for the crystallization of silicate component developed in the framework of the evolution from interstellar dust to cometary dust.(4) Formation of dust grains in astrophysical environments ; The formation of dust grains was investigated in circumstellar envelopes of evolved stars. The formation process of core-mantle grains consisting of a SiC core and a carbon mantle was investigated to reproduce the 11.3mum feature observed towards carbon stars. In oxygen-rich AGB stars the observed 13mum feature can be attributed to dust grains consisting of a Al_2O_3 core and a silicate mantle. The possibility of the formation of dust grains in Ia supernovae was discussed.
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通讯作者:
T.Yamamoto: "Crystallization of amorphous silicate in cometary dust" Proc.29th ISAS Lunar and Planetary Symp. 29. 252-253 (1996)
T.Yamamoto:“彗星尘埃中无定形硅酸盐的结晶”Proc.29th ISAS Lunar and Planetary Symp。
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30
    The investigation of the role of supernovae as the source of interstellar dust from the dawn of the universe to the present time
    • 批准号:
      20340038
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $11.56万
    • 财政年份:
      2008
    • 负责人:
      KOZASA Takashi
    • 依托单位:
    Evolution of Dust and its Effects on the Cosmic Back Ground and Stellar Formation in the Early Universe
    • 批准号:
      16340051
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $5.89万
    • 财政年份:
      2004
    • 负责人:
      KOZASA Takashi
    • 依托单位:
    Formation of Dust Grains in the Early Universe and its Effects on the Observations.
    • 批准号:
      13640229
    • 项目类别:
      Grant-in-Aid for Scientific Research (C)
    • 资助金额:
      $1.15万
    • 财政年份:
      2001
    • 负责人:
      KOZASA Takashi
    • 依托单位:
    海外基金