UV-induced diamond formation in interstellar clouds
星际云中紫外线诱导钻石形成
基本信息
- 批准号:15340180
- 负责人:
- 金额:$ 10.82万
- 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:2003
- 资助国家:日本
- 起止时间:2003 至 2004
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
New formation routes of diamond in interstellar clouds and parent bodies of carbonaceous chondrites are found based on laboratory experiments. It is shown that diamond precursor nucleated as a result of UV photolysis of interstellar ice mixtures in molecular clouds, and grew with further UV irradiation in diffuse clouds. The present study supports the occurrence of diamonds in interstellar clouds, and suggests that diamond is ubiquitous in space. Furthermore, we performed experiments on the aqueous alteration and the subsequent thermal metamorphism of organic materials formed in molecular cloud, and found that diamonds formed by this process in the parent bodies of carbonaceous chondrites. The various characteristics of nano-diamonds in chondrites and interplanetary dusts are well explained by these new formation routes.
在实验室实验的基础上,发现了星际云和碳质球粒陨石母体中金刚石形成的新途径。结果表明,金刚石前驱体是由于分子云中星际冰混合物的紫外光分解而成核的,并随着漫射云中紫外线的进一步照射而生长。目前的研究支持星际云中存在钻石,并认为钻石在太空中无处不在。此外,我们还对分子云中形成的有机物质的水蚀变和随后的热变质作用进行了实验,发现在碳质球粒陨石母体中通过这个过程形成了钻石。这些新的形成途径很好地解释了球粒陨石和星际尘埃中纳米钻石的各种特征。
项目成果
期刊论文数量(36)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Evaporation of interstellar organic materials in the solar nebula
太阳星云中星际有机物质的蒸发
- DOI:
- 发表时间:2003
- 期刊:
- 影响因子:0
- 作者:Nakano;H.
- 通讯作者:H.
Observation of resonance structures in 4d photoionization of Eu
Eu 4d 光电离共振结构的观察
- DOI:10.1016/j.elspec.2005.01.209
- 发表时间:2005
- 期刊:
- 影响因子:0
- 作者:T. Kojima;F. Chen;M. Kitajima;T. Koizumi;Y. Nakai;H. Yamaoka;N. Watanabe
- 通讯作者:N. Watanabe
Watanabe N.: "Thedependence of H2CO and CH3OH formation on the temperature and thickness of H2O-CO ice during successive hydrogenetion of CO"Astrophys.J.. 588. L121-L124 (2003)
Watanabe N.:“CO 连续氢化过程中 H2CO 和 CH3OH 形成对 H2O-CO 冰的温度和厚度的依赖性”Astrophys.J.. 588. L121-L124 (2003)
- DOI:
- 发表时间:
- 期刊:
- 影响因子:0
- 作者:
- 通讯作者:
Is Chaos on Europa caused by crust-penetrating impacts?
木卫二上的混乱是由地壳穿透撞击造成的吗?
- DOI:
- 发表时间:2005
- 期刊:
- 影响因子:0
- 作者:Cox;R.
- 通讯作者:R.
Nakano, H.: "Evaporation of interstellar organic materialsin the solar nebula"Astrophys.J.. 592. 1252-1262 (2003)
Nakano, H.:“太阳星云中星际有机物质的蒸发”Astrophys.J.. 592. 1252-1262 (2003)
- DOI:
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- 期刊:
- 影响因子:0
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KOUCHI Akira其他文献
KOUCHI Akira的其他文献
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{{ truncateString('KOUCHI Akira', 18)}}的其他基金
Observation of surface structure of amorphous ice and role of amorphous ice in surface atomic reactions at low temperatures
非晶冰表面结构观察及非晶冰在低温表面原子反应中的作用
- 批准号:
22340157 - 财政年份:2010
- 资助金额:
$ 10.82万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Evaluation of catalytic effect of amorphous ice on the surface atomic reactions
非晶冰对表面原子反应的催化效果评价
- 批准号:
17104006 - 财政年份:2005
- 资助金额:
$ 10.82万 - 项目类别:
Grant-in-Aid for Scientific Research (S)
Collisional sticking of organic grains in the solar nebula
太阳星云中有机颗粒的碰撞粘附
- 批准号:
12440142 - 财政年份:2000
- 资助金额:
$ 10.82万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Development of comet nucleus simulation experiments
彗核模拟实验进展
- 批准号:
10554027 - 财政年份:1998
- 资助金额:
$ 10.82万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Chemical reaction mechanism on the surafce of interstellar icy grains
星际冰粒表面化学反应机制
- 批准号:
07454128 - 财政年份:1995
- 资助金额:
$ 10.82万 - 项目类别:
Grant-in-Aid for Scientific Research (B)
Material evolution simulator
材料演化模拟器
- 批准号:
05554013 - 财政年份:1993
- 资助金额:
$ 10.82万 - 项目类别:
Grant-in-Aid for Developmental Scientific Research (B)
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The effect of aqueous alteration on the distribution of lithophile elements in carbonaceous chondrites
水蚀变对碳质球粒陨石中亲石元素分布的影响
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从热液蚀变碳质球粒陨石中探索的 C 型小行星的热演化
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22H01279 - 财政年份:2022
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2620686 - 财政年份:2021
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基于碳质球粒陨石的矿物和有机成分以及反射光谱特性研究含水小行星的多样性
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碳质球粒陨石和彗星颗粒的矿物学和岩石学:含水小行星演化的见解。
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16K05603 - 财政年份:2016
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未分组的碳质球粒陨石的研究:对早期太阳系母体形成和演化的影响。
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