| Item type |
会議発表論文 / Conference Paper(1) |
| 公開日 |
2015-03-26 |
| タイトル |
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タイトル |
月レゴリスによる資源・エネルギーその場利用（ISRU）研究 |
| 言語 |
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言語 |
jpn |
| 資源タイプ |
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資源タイプ識別子 |
http://purl.org/coar/resource_type/c_5794 |
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資源タイプ |
conference paper |
| アクセス権 |
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アクセス権 |
metadata only access |
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アクセス権URI |
http://purl.org/coar/access_right/c_14cb |
| その他のタイトル（英） |
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その他のタイトル |
Lunalogy & In-situ Resources Utilization (ISRU) by Lunar Regolith |
| 著者 |
高柳, 昌弘
足立, 聡
福中, 康博
夏井坂, 誠
網野, 真樹
萩原, 理加
松岡, 俊文
安田, 秀幸
本間, 敬之
Takayanagi, Masahiro
Adachi, Satoshi
Fukunaka, Yasuhiro
Natsuisaka, Makoto
Amino, Masaki
Hagiwara, Rika
Matsuoka, Toshifumi
Yasuda, Hideyuki
Homma, Takayuki
Sadoway, D.R.
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| 著者所属 |
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宇宙航空研究開発機構宇宙科学研究本部 |
| 著者所属 |
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宇宙航空研究開発機構宇宙科学研究本部 |
| 著者所属 |
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宇宙航空研究開発機構宇宙科学研究本部 |
| 著者所属 |
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宇宙航空研究開発機構宇宙科学研究本部 |
| 著者所属 |
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宇宙航空研究開発機構宇宙科学研究本部 |
| 著者所属 |
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京都大学 |
| 著者所属 |
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京都大学 |
| 著者所属 |
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大阪大学 |
| 著者所属 |
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早稲田大学 |
| 著者所属（英） |
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en |
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) |
| 著者所属（英） |
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en |
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) |
| 著者所属（英） |
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en |
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) |
| 著者所属（英） |
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en |
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) |
| 著者所属（英） |
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en |
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) |
| 著者所属（英） |
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en |
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Kyoto University |
| 著者所属（英） |
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en |
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Kyoto University |
| 著者所属（英） |
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en |
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Osaka University |
| 著者所属（英） |
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en |
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Waseda University |
| 著者所属（英） |
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en |
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Massachusetts Institute of Technology (MIT) |
| 出版者 |
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出版者 |
宇宙航空研究開発機構宇宙科学研究本部 |
| 出版者（英） |
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出版者 |
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA) |
| 書誌情報 |
宇宙エネルギーシンポジウム
en : Space Energy Symposium
巻 29,
発行日 2010-02
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| 会議概要（会議名, 開催地, 会期, 主催者等） |
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内容記述タイプ |
Other |
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内容記述 |
第29回宇宙エネルギーシンポジウム(2010年2月26日, 宇宙航空研究開発機構宇宙科学研究本部相模原キャンパス) |
| 会議概要（会議名, 開催地, 会期, 主催者等）（英） |
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内容記述タイプ |
Other |
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内容記述 |
The twenty-ninth Space Energy Symposium (February 26, 2010, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara) |
| 抄録（英） |
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内容記述タイプ |
Other |
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内容記述 |
The present research team in ISS project office, JAXA is collaborating with Kyoto University, Waseda University and MIT. It focuses the fundamental researches of in-situ Resources Utilization on Lunar Base. It is financially supported as FY21 International Collaboration Mission. The research targets are deeply linked with the activities by the working group lead by Dr. K. Kinoshita(ISAS/JAXA), "Nano-meter Structured Materials Processing for Energy Devices for Space", which is regarded as the international topical team between ESA and JAXA, "Electrochemical Nucleation and Growth". It is developed from the accumulated information in the multi-disciplinary fields of Space Environment Utilization Science Field. The present program is composed of the following three categories.(1) Depth Distributions of Lunar Regolith followed by Resources Exploration: Resources exploration survey based on the laser sounder data supplied from JAXA lunar satellite "Kaguya", subsequentlyfollowed by regorith transportation and separation engineering under 1/6 gravity.(2) Characterization of Lunar Regolith and Solar Wind Implantation Mechanism: The design of gaseous component recovery system with regorith stimulant and the clarification of solar wind implantation into finer oxide particles.(3) In-situ Resources Utilization on Lunar Base: O2(g) and light metal extraction by molten salt electrolysis as well as energy conversion and storage processes.To begin with the projects, "Depth Distributions of Lunar Regolith" must be carefully examined, because Lunar regorith composition considerably varied according to the samples obtained in Apollo project. The thickness of lunar regolith becomes an important issue for resource development at Lunar surface. In order to delineate the thickness map of lunar regolith, we adopt sophisticated seismic data processing methodologies into "Kaguya"'s laser data. Especially the migration analysis becomes a key processing and Kirchhoff migration. Then, the project to characterize Lunar Regorith from the view point of gaseous component absorption and desorption mechanism is studied by exposing the lunar stimulant to hydrogen plasma. This research is deeply relating to clarification of solar wind implantation mechanism. The transportation of lunar regorith simulant and the separation technique based on electrostatic and electromagnetic gradient field must be designed. The third target is oxygen gas evolution as well as light metal production aimed at solar power generation. Molten salt electrolysis plays primarily a important role in such a non-equilibrium electrochemical processing. Three phase interfacial phenomena must be focused as well as the development of inert anode which can be applied to high temperature molten oxide. Computational chemistry is also an important tool as well as in-situ measurement technique based on Synchrotoron Radiation Technology. |
| 内容記述 |
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内容記述タイプ |
Other |
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内容記述 |
形態: カラー図版あり |
| 内容記述 |
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内容記述タイプ |
Other |
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内容記述 |
形態: CD-ROM1枚 |
| 内容記述（英） |
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内容記述タイプ |
Other |
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内容記述 |
Physical characteristics: Original contains color illustrations |
| 内容記述（英） |
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内容記述タイプ |
Other |
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内容記述 |
Note: One CD-ROM |
| 書誌レコードID |
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収録物識別子タイプ |
NCID |
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収録物識別子 |
AN10324356 |
| 資料番号 |
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内容記述タイプ |
Other |
|
内容記述 |
資料番号: AA0064737015 |
