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巨大衝突に始まる月形成:岩石破片円盤形成から揮発性物質散逸まで

巨大衝突に始まる月形成:岩石破片円盤形成から揮発性物質散逸まで
月球的形成始于巨大的撞击:从岩石碎片盘的形成到挥发性物质的消散
批准号:
12640405
负责人:
NAKAZAWA Kiyoshi
金额:
$2.3万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
2000
资助国家:
日本
项目状态:
已结题
起止时间:
2000 至 2001

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中文摘要
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英文摘要
The giant impact between a Mars size proto-planet and the Earth could produce the moon. This is the model of moon formation called "The Giant Impact Model". Today many scientists studying about the origin of the moon consider the model the most reliable one. In this study we investigated the model in two parts for two years. First part is study about the giant impact it self. Second is the accumulation process of the moon from the disk around the Earth.The accumulation of the moon in the circum earth disk was supported by strong mass transfer due to the axis-asymmetric gravitational field produced by density waves in the disk. The gravitational field carried the rock debris outer than the Roche limits. Then the debris accumulated to the single moon. We have confirmed the transfer process by N-body numerical simulation and formulate the transfer rate as a function of initial disk mass theoretically. In addition to that, we found that initially light disk could produce multiple moonlets … More outside the Roche limits and initially heavy one could produce massive single moon. So, we estimate the initial disk mass of the Earth which has single moon as heavier than 3 times the mass of the moon.The giant impacts between proto-planets could take place very frequently in the planetary formation process. So, it is important to investigate the impacts not only as the moon formation stage but also one of the important basic process in the planetary formation. We have investigated the giant impact process under the wide range of impact parameters rather than to concentrate on the moon formation process only. From the studies we have found that the proto planet deformed significantly at the impact instance, but the proto planet restore its global figure by its strong self gravity. In addition to that we confirmed that the restored proto planet was on the oval orbit around the Earth which never produces the giant impact any more. This fact implies that the giant impact process could play a role resemble to the "Capture process" in the moon formation. Less
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H. Tanaka, T. Takeuchi, W.R. Ward: "Three-Dimensional Interaction between a Planet and an Isothermal Gaseous Disk : I. Corotation and lindblad Torgues and Planet Migration"Astrophysical Journal. 565. 1257-1271 (2001)
H. Tanaka、T. Takeuchi、W.R. Ward:“行星与等温气态盘之间的三维相互作用:I. 共转、lindblad Torgues 和行星迁移”天体物理学杂志。
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M.Nagasawa, S.Ida, H.Tanaka: "Origin of high orbital eccentricity and"Earth, Planets and Space. 53. 1085-1091 (2001)
M.Nagasawa、S.Ida、H.Tanaka:“高轨道偏心率的起源和”地球、行星和空间。
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J.Kominami, S.Ida: "The Effect of Tidal Interaction with a Gas Disk on Formation of Terrestrial Planets"Icarus. (印刷中). (2002)
J.Kominami,S.Ida:“潮汐与气盘相互作用对类地行星形成的影响”(出版中)。
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M. Ikoma, K. Nakazawa, H. Emori: "Formation of Giant Planets : Dependences on Core Accretion Rate and Grain Opacity"Astrophysical Journal. 537. 1013-1025 (2000)
M. Ikoma、K. Nakazawa、H. Emori:“巨行星的形成:对核心吸积率和颗粒不透明度的依赖”天体物理学杂志。
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15
    Role of glycosaminoglycan-synthesizing enzymes in corneal transparency
    • 批准号:
      14571693
    • 项目类别:
      Grant-in-Aid for Scientific Research (C)
    • 资助金额:
      $0.96万
    • 财政年份:
      2002
    • 负责人:
      NAKAZAWA Kiyoshi
    • 依托单位:
    How does Proteoglycan synthesis by coraeal stromacytes respond to changes in environment around the cells?
    • 批准号:
      11671762
    • 项目类别:
      Grant-in-Aid for Scientific Research (C)
    • 资助金额:
      $1.34万
    • 财政年份:
      1999
    • 负责人:
      NAKAZAWA Kiyoshi
    • 依托单位:
    The origin of diversity of extrasolar planets formation of giant gasous planets and orbital evolution
    • 批准号:
      09440089
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $1.09万
    • 财政年份:
      1997
    • 负责人:
      NAKAZAWA Kiyoshi
    • 依托单位:
    Planetary Formation relevant to Titius-Bode's Law
    • 批准号:
      07454114
    • 项目类别:
      Grant-in-Aid for Scientific Research (B)
    • 资助金额:
      $4.99万
    • 财政年份:
      1995
    • 负责人:
      NAKAZAWA Kiyoshi
    • 依托单位:
    海外基金