Evolution of Molecules in Space

How do molecules evolve in space?  We aim at answering this question by an interdisciplinary study of laboratory experiments, theoretical modeling of surface  processes and molecular-cloud and protoplanetary-disk chemistry, observation of young stellar objects, and analyses of extraterrestrial materials.

Research Project on Evolution of Molecules in Space
Grant-in-Aid for Scientific Research on Innovative Areas
Supported by the Ministry of Education, Culture, Sports, Science & Technology, Japan

Contact: contact [at] astromolecules.org

-TOPICS-

International symposium "Molecular Evolution in Space"

08/05/2017 11:53

June 27-29
[symposium webpage]
Institute of Low Temperature Science, Hokkaido University

Solar-System symposium in Sapporo 2017

08/03/2017 11:48

Februrary 13-15, 2017
[symposium website]
Rusutsu, Hokkaido

Workshop#12

08/09/2016 11:29

August 23, 2016
"Future research direction of organics in space (2)"
Hamamatsu-cho, Tokyo

Annual Meeting for Evolution of Molecules in Space #4

08/08/2016 11:41

July 11-12, 2016
Institute of Low Temperature Science, Hokkaido University

Workshop#11

08/04/2016 11:37

March 30-31, 2016
"Molecular evolution in protoplanetary disks (2)"
Hiroshima University

Workshop#10

08/03/2016 11:25

February 29, 2016
"Future research direction of organics in space"
Hamamatsu-cho, Tokyo

Solar-System symposium in Sapporo 2016

20/02/2016 11:51

Februrary 17-19, 2016
[symposium website]
Rusutsu, Hokkaido

Workshop#9

08/11/2015 11:34

October 29, 2015
"Molecular evolution in protoplanetary disks"
Institute of Low Temperature Science, Hokkaido University

Annual Meeting for Evolution of Molecules in Space #3

08/11/2015 11:22

October 22-23, 2015
Institute of Low Temperature Science, Hokkaido University

Workshop#8

08/08/2015 11:31

July 27, 2015
"Hydrothermal reaction of organics in small bodies"
Institute of Low Temperature Science, Hokkaido University

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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