Zobrazeno 1 - 6
of 6
pro vyhledávání: '"炭素質隕石"'
Autor:
Oba, Yasuhiro
Publikováno v:
低温科学. 78:47-59
窒素を含む複素環化合物である核酸塩基は，糖，リン酸とともに，生命の遺伝情報をつかさどる核 酸の構成成分である．これまでの研究で，炭素質隕石から隕石固有の核酸塩基数種（ウ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::da032729398d49d4bec6f23510b624cc
http://hdl.handle.net/2115/77765
http://hdl.handle.net/2115/77765
Publikováno v:
第40回月・惑星シンポジウム = Proceedings of the 40th ISAS Lunar and Planetary Symposium. :52-55
資料番号: AA0063723013
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::e552fd2da69bc3fb42d196ed18bc3cd4
http://id.nii.ac.jp/1696/00020427/
http://id.nii.ac.jp/1696/00020427/
Autor:
Miura, Yasunori
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :120-123
Carbon and Fe-Ni elements are considered to be stable elements at high temperature and pressure, and found during shock wave explosions at meteoritic craters and meteorites. The main purpose of the paper is to elucidate carbon-bearing solid from atmo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::a052b326087c893eee42086a9d351813
http://id.nii.ac.jp/1696/00020487/
http://id.nii.ac.jp/1696/00020487/
Autor:
Miura, Yasunori
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :116-119
Carbon element is considered to be stable and survived elements at high Temperature and Pressure (i.e. PT) during shock wave explosions at meteoritic craters and meteorites. The main purpose of the paper is to elucidate carbon-bearing solid with Fe o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::bdf764d5b45be9d17aaa7120a661b03b
http://id.nii.ac.jp/1696/00020486/
http://id.nii.ac.jp/1696/00020486/
Autor:
Kurosawa, Kosuke, Ishibashi, Ko, Sugita, Seiji, Kadono, Toshihiko, Ono, Sosuke, Matsui, Takafumi
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :202-205
Hydrogen Cyanide (HCN) is considered as one of most important compounds for the origin of life because it is a precursor of complex organic molecules, such as amino acids and nucleic acid bases. Although a number of different mechanisms of HCN format
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::0ba0df36a0065724dcf94fe8b755ff22
http://id.nii.ac.jp/1696/00020508/
http://id.nii.ac.jp/1696/00020508/
Publikováno v:
第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :177-177
The emission feature around 11.3 micrometer observed towards carbon stars is considered to be due to SiC grains condensed in the circumstellar envelopes. The isotopic anomalies of SiC discovered in carbonaceous meteorites strongly support the formati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::d80d939650a7ac4aca91496cd0a0cecf
http://id.nii.ac.jp/1696/00038408/
http://id.nii.ac.jp/1696/00038408/