| タイトル | Methane on Mars: Measurements and Possible Origins |
| 本文（外部サイト） | http://hdl.handle.net/2060/20110008019 |
| 著者（英） | Villanueva, Geronimo L.; Tokunaga, Alan; Hartogh, Paul; Kaufl, H. Ulrich; Novak, Robert E.; Radeva, Yana L.; Mumma, Michael J.; Encrenaz, Therese |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2011-02-08 |
| 言語 | eng |
| 内容記述 | The presence of abundant methane in Earth's atmosphere (~1.6 parts per million) requires sources other than atmospheric chemistry. Living systems produce more than 90% of Earth's atmospheric methane; the balance is of geochemical origin. On Mars, methane has been sought for nearly 40 years because of its potential biological significance, but it was detected only recently [1-5]. Its distribution on the planet is found to be patchy and to vary with time [1,2,4,5], suggesting that methane is released recently from the subsurface in localized areas, and is then rapidly destroyed [1,6]. Before 2000, searchers obtained sensitive upper limits for methane by averaging over much of Mars' dayside hemisphere, using data acquired by Marsorbiting spacecraft (Mariner 9) and Earth-based observatories (Kitt Peak National Observatory, Canada- France-Hawaii Telescope, Infrared Space Observatory). These negative findings suggested that methane should be searched at higher spatial resolution since the local abundance could be significantly larger at active sites. Since 2001, searches for methane have emphasized spatial mapping from terrestrial observatories and from Mars orbit (Mars Express). |
| NASA分類 | Lunar and Planetary Science and Exploration |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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