| タイトル | Describing and Measuring the Chemical Signatures of Life |
| 著者（英） | Paszczynski, A.; Crawford, R. L.; Cheng, I. F.; Wells, R.; Anderson, T. J.; Corti, G.; Barnes, B.; Wai, C.; Lang, Q.; Allenbach, L. |
| 著者所属（英） | Idaho Univ. |
| 発行日 | 2000-07-01 |
| 言語 | eng |
| 内容記述 | Here we discuss an approach to remotely detecting extraterrestrial life forms on other planets or their moons by detection of specific types of organic molecules. The life entities to be detected would be presently active life forms, or those that are only recently dormant. The only place beside Earth's moon where humans have actually examined surface soils for the presence of organic molecules is Mars. This was accomplished using mass-spectrometry during the Viking mission, and results were negative. The lack of organic moieties, if they ever were present, probably resulted form their destruction over geologic time frames by the extraordinarily reactive surface soils found there. Thus, on Mars, detection of organic signatures of life probably would be possible only in subsurface soils, or perhaps in polar regions. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/538518 |
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