A study of the carbonaceous matter in carbonaceous chondrites for evaluating the degree of alteration/thermal metamorphism in meteorite parent bodies.
A study of the carbonaceous matter in carbonaceous chondrites for evaluating the degree of alteration/thermal metamorphism in meteorite parent bodies.
批准号:
14540456
负责人:
KITAJIMA Fumio
金额:
$2.37万
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:
2002
资助国家:
日本
项目状态:
已结题
起止时间:
2002 至 2004
中文摘要
1.硫K边XAFS分析结果表明:(1)CM球粒陨石的典型XAFS谱显示了无机硫化物、硫酸盐和噻吩类(有机硫)杂质的富集;(2)CV(阿连德)和CO(奥尔南斯)的吸收光谱缺少硫酸根和噻吩的吸收,说明母体与CM的吸收光谱不同。(3)未加热或弱加热的碳酸盐的光谱显示出较强的噻吩吸收。(4)根据噻吩吸收的强度,可将样品分为以下几类:Ⅰ弱吸收,对应于强加热的碳酸盐; Ⅱ与硫化物吸收相当,对应于未加热或仅弱加热的碳酸盐;(5)塔吉什湖显示出相对较强的噻吩吸收,相对较弱的硫酸盐吸收是该样品的另一个特征。(6)实验室加热的Muchison样品的XAFS谱中缺少硫酸盐和噻吩类的结构,说明这些结构在加热过程中已经丢失。(7)对XAFS谱的定量处理表明,未加热或弱加热的玄武岩可分为两个亚类。2.利用同步辐射X射线衍射技术,确定了狭山中的矿物和筑波玄武岩中的CI样碎屑。筑波球粒陨石中的碎屑未被加热超过500℃,而狭山的氧同位素分析表明其在蚀变过程中经历了比Murchison等其他CM球粒陨石更高的温度(超过120℃)。
英文摘要
1.Sulfur K-edge XAFS analysis of the chondrites shows the following results :(1)A typical XAFS spectrum of a CM chondrite shows the absorptions of inorganic sulfide, sulfate, and thiophenic (organic sulfur) absorptions.(2)The spectra of the CV (Allende) and CO (Ornans) chondrites lack in the sulfate and thiophenic absorptions, indicating the difference of parenrt bodies from the CM chondrites.(3)The spectra of unheated or weakly heated chondrites show relatively strong thiophenic absorption.(4)Based on the intensity of thiophenic absorption, the samples can be classified into the following groups : I Weak, corrssponds to strongly heated chondrites, II Comparable to the sulfidic absorption, corresponds to unheated or only weakly heated chondrites, III CV and CO chondrites.(5)Tagish Lake shows relatively strong thiophenic absorption, and relatively weak sulfate absorption is another characteristic of this sample.(6)The XAFS spectrum of the Muchison sample heated in laboratory lacks in the sulfate and thiophenic absorptions, suggesting such partial structure have been lost during heating.(7)Quantitative treatment of the XAFS spectra suggests that the unheated or weakly heated chondrites can be classified into two subgroups.2.Minerals in the Sayama and the CI-ike clast in the Tsukuba chondrites were determined by X-ray diffraction using synchrotron irradiation. The clast in Tsukuba chondrite have not been heated more than 500℃, and Oxygen isotope analysis of Sayama shows that it have experienced higher temperature (more than 120℃) than the other CM chondrites such as Murchison during its alteration.3.The laboratory simulation of aqueous alteration using Ningqiang shows that Q-gas have not been lost during alteration, but Ar-rich gas have been lost.
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A super-hard, transparent carbon form, diamond, and secondary graphite in the Havero ureilite : A fine-scale microraman and synchrotron tomography.
Havero ureilite 中的超硬、透明碳形式、金刚石和次生石墨:精细尺度显微拉曼和同步加速器断层扫描。
DOI:
--
发表时间:
2004
期刊:
Meteorit.Planet.Sci. 39
影响因子:
--
作者:
[荻原成騎, 重田康成, Kitajima et al., 荻原成騎, Nakashima et al., S.Ogihara, Nakamura et al., S.Ogihara, El Goresy et al.]
通讯作者:
El Goresy et al.
Mineralogy of 100-mg test samples for Muses C mission. in "The First Open Competition for the MUSES-C Asteroidal Sample Preliminary Examination Team".
Muses C 任务的 100 毫克测试样品的矿物学。
DOI:
--
发表时间:
2003
期刊:
ISAS report SP 16
影响因子:
--
作者:
[Osawa T., Kagi H., Nakamura T., Noguchi T., Nagao K., Kitajima et al., Kitajima et al., Kitajima et al., Kitajima et al., Nozaki et al., Kitajima et al., Uesugi et al., Nakamura et al., Noguchi et al., Yada et al., Akaki et al., Tnui et al., Zolensky et al., Nakamura et al., Nakamura et al., Okazaki et al., Nakamura et al., Noguchi et al., Uesugi et al., Nakashima et al., Yada et al., Osawa et al., Nakamura et al.]
通讯作者:
Nakamura et al.
Noble gases in Kobe carbonaceous chondrite.
神户碳质球粒陨石中的稀有气体。
DOI:
--
发表时间:
2002
期刊:
Geochem.J. 36
影响因子:
--
作者:
[Nakamura T., Noguchi T., Takaoka et al.]
通讯作者:
Takaoka et al.
Cosmic ray exposure age and heliocentric distance of the parent body of H chondrites Yamato-75029 and Tsukuba.
H球粒陨石Yamato-75029和筑波母体的宇宙射线暴露年龄和日心距离。
DOI:
--
发表时间:
2002
期刊:
Antarctic Meteorite Research 15
影响因子:
--
作者:
[Nakamura T., Noguchi T., Takaoka et al., Tsuchiyama et al., Noguchi et al., Kitajima et al., Nakashima et al.]
通讯作者:
Nakashima et al.
Kitajima et al.: "Carbon K-edge NEXAFS study of carbonaceous matter in the Allende (CV3) carbonaceous chondrite"KEK Photon Factory Activity Report, Part B, Users' Report. 35 (2003)
Kitajima 等人:“阿连德 (CV3) 碳质球粒陨石中碳质物质的碳 K 边缘 NEXAFS 研究”KEK 光子工厂活动报告,B 部分,用户报告。
DOI:
--
发表时间:
期刊:
影响因子:
--
作者:
[]
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