Project/Area Number |
14340171
|
Research Category |
Grant-in-Aid for Scientific Research (B)
|
Allocation Type | Single-year Grants |
Section | 一般 |
Research Field |
地球化学
|
Research Institution | Kobe University |
Principal Investigator |
NAKAMURA Noboru Kobe University, Faculty of Science, Professor, 理学部, 教授 (90030791)
|
Co-Investigator(Kenkyū-buntansha) |
YAMASHITA Katsuyukii Kobe University, Faculty of Science, Assistant Professor, 理学部, 助手 (50322201)
OKANO Osamu Okayama University, Faculty of Science, Assistant Professor, 理学部, 助手 (10233355)
|
Project Period (FY) |
2002 – 2004
|
Project Status |
Completed (Fiscal Year 2004)
|
Budget Amount *help |
¥13,200,000 (Direct Cost: ¥13,200,000)
Fiscal Year 2004: ¥2,200,000 (Direct Cost: ¥2,200,000)
Fiscal Year 2003: ¥3,500,000 (Direct Cost: ¥3,500,000)
Fiscal Year 2002: ¥7,500,000 (Direct Cost: ¥7,500,000)
|
Keywords | Chondrites / Differentiated meteorites / Primitive achondrites / Kobe meteorite / Solar system chronology / Rare Earth elements / Radiometric ages / Extinct nuclides / 始原的隕石 / エイコンドライト / 隕石母天体 / 星雲過程 / 希土類元素パターン / 変成年代 / 塩素同位体 / 年代決定 / アルカリ金属 / 微量元棄 / アエンデ隕石 / 炭素質コンドライト / 年代測定 / 火星隕石 |
Research Abstract |
In order to obtain new evidences constraining the timing, origin and evolution of primitive and differentiated meteorites and their genetic relationships, we have carried out chemical, petrological and isotopic analyses for chondrites and achondrites. Results are summarized bellow : (1)Under international consortium for the Kobe (CK) meteorite, we obtained a unique REE pattern and detailed chemical and petrological features, which constrains nebular fractionations and meteorite parent body processes of CK chondrites yielding silicate-darkening of the meteorites. The age determination by U-Pb and Rb-Sr methods were carried out for the meteorite, indicating complicated thermal histories of CK chondrite parent body. (2)REE and Rb-Sr isotopes were analyzed for the most pure matrix materials or chondrules from the Allende (CV) meteorite, respectively. REE results suggest that the precursor of matrix formed by nebular processes. The 4.4Ga alteration event was newly discovered from Rb-Sr system of Allende. (3)The precise Sm-Nd isotopic analyses were carried out for 5 acapulcoites : We obtained a significantly young age (4.13±0.10Ga) for one acapulcoite, indicating young thermal event on the parent body. (4)The low Pb blank technique for U-Pb dating was established and precise U-Pb ages as well as Sm-Nd and Rb-Sr ages and REE patterns were obtained for three newly found Antarctic Martian meteorites. (5)The Mo isotopic anomalies derived from stellar processes were discovered in primitive meteorites. Precise Cr and Ba isotopic analysis techniques were established and new isotopic anomalies were found for primitive and differentiated meteorites. (6)Precise chlorine isotopic analyses were carried out for Allende and 9 standard rocks using thermal ionization mass spectrometry (TIMS). We also established a high sensitivity negative TIMS for Cl.
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