X00: Coordinator Group
PI Akira Kouchi Hokkaido University
Co-I Shogo Tachibana Hokkaido University
Collaborator Hiroko Nagahara University of Tokyo
Collaborator Tomoko Fukazawa Meiji Univesity
Collaborator Satoshi Yamamoto University of Tokyo
Collaborator Hisayoshi Yurimoto Hokkaido University
Collaborator Hiroshi Naraoka Kyushu University
Collaborator Jun-ichi Watanabe National Astronomical Observatory of Japan
A01: Experiments on Molecular Cloud Processes
PI Akira Kouchi Hokkaido University
Co-I Tetsuya Hama Hokkaido University
Co-I Hiroshi Hidaka Hokkaido University
Co-I Shogo Tachibana Hokkaido University
Co-I Akihiro Yabushita Kyoto Unversity
Co-I Mitsunori Araki Tokyo University of Science
A02: Experiments on Protoplanetary Disk Processes
PI Hiroko Nagahara University of Tokyo
Co-I Yuki Kimura Tohoku University
Co-I Akira Tsuchiyama Kyoto University
Co-I Yusuke Tamenori Japan Synchrotron Radiation Research Institute
Co-I Masato Hoshino Japan Synchrotron Radiation Research Institute
Co-I Osamu Takahashi Hiroshima University
A03: Theoretical Modeling of Surface Processes and MC- and PP-disk chemistry
PI Tomoko Fukazawa Meiji Univesity
Co-I Hiroto Tachikawa Hokkaido Univesity
Co-I Hiroshi Miura Nagoya City Univesity
Collaborator Yuri Aikawa Kobe Univesity
Collaborator Hideko Nomura Kyoto Univesity
A04: Astronomical Observation of Young Stellar Objects
PI Satoshi Yamamoto University of Tokyo
Co-I Nami Sakai University of Tokyo
Co-I Yoshimasa Watanabe University of Tokyo
Co-I Takeshi Sakai University of Electro-Communications
Co-I Shuro Takano National Astronomical Observatory of Japan
Co-I Tomoya Hirota National Astronomical Observatory of Japan
Co-I Yoshinori Uzawa National Astronomical Observatory of Japan
Co-I Hiroyuki Maezawa Osaka Prefecture University
A05: Analyses of Organic Materials: Isotopes and Structures
PI Hisayoshi Yurimoto Hokkaido University
Co-I Hiroshi Naraoka Kyushu University
Co-I Hajime Mita Fukuoka Institute of Technology
Co-I Yoshinori Takano Japan Agency for Marine-Earth Science and Technology
Co-I Kenji Hamase Kyushu University
PI Sho-ichi Itoh Hokkaido University

 

46億年前に誕生した太陽系で
分子はどのように進化し
惑星や地球に至ったのか

ビッグバン以降,様々な構造が形成された宇宙の中で,46億年前に誕生した太陽系において分子がどのように進化し,惑星や地球,そして生命に至ったのかという疑問への答えに近づくことをめざします.宇宙で最も大量に存在する元素(H, C, O, N)からなる氷および有機物に着目し,星間分子雲から原始惑星系までの分子進化の全体像を実験・理論・観測・分析など多様な手法で探求し,惑星系形成の物理過程の解明に化学的視点を加えることをめざします.
 

領域代表:
香内 晃
〒060-0819 北海道札幌市
北区北19条西8丁目 北海道大学
低温科学研究所
E-mail: kouchi [at] lowtem.hokudai.ac.jp
TEL: 011-706-5500
FAX: 011-706-7142

領域事務局:
橘 省吾
〒060-0810 北海道札幌市
北区北10条西8丁目 北海道大学
大学院理学研究院 自然史科学部門
E-mail: tachi [at] ep.sci.hokudai.ac.jp
TEL/FAX: 011-706-3586