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2017 Fiscal Year Final Research Report

Evolution of early solar system viewed from return sample analysis

Research Project

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Project/Area Number 25247091
Research Category

Grant-in-Aid for Scientific Research (A)

Allocation TypeSingle-year Grants
Section一般
Research Field Geochemistry/Cosmochemistry
Research InstitutionTohoku University

Principal Investigator

Nakamura Tomoki  東北大学, 理学研究科, 教授 (20260721)

Co-Investigator(Renkei-kenkyūsha) NAKASHIMA Daisuke  東北大学, 大学院理学研究科, 講師 (90734757)
Project Period (FY) 2013-04-01 – 2018-03-31
Keywords小惑星探査 / 始原隕石 / S型小惑星 / サンプルリターン / C型小惑星
Outline of Final Research Achievements

In order to clarify the evolution of early solar system, we performed (1) analysis of small dust particles returned by Hayabusa mission from S-type asteroid Itokawa, which showed that Itokawa experienced very strong impact that disrupted parent asteroid of Itokawa, (2) heating experiments of hydrous carbonaceous chondrites in order to understand spectral changes during hearting of C-type asteroids. The experiments were performed in vacuum and the heated samples were never exposed to atmosphere after heating and thus we obtained spectra that are free of atmospheric water.

Free Research Field

惑星科学

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Published: 2019-03-29  

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