| タイトル | Strategies to Support Exploration of Mars' Surface |
| 著者（英） | Blaney, D.; Adams, J.; Sykes, M.; Farr, T.; Kirkland, L. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 2003-04-22 |
| 言語 | eng |
| 内容記述 | Surface Visible infrared spectroscopy has a long history of providing fundamental compositional discoveries in the solar system. However, we are entering a new era of Mars exploration in which missions will take place nearly every 2 years.The visible infrared spectral community thus faces a more rapid influx in data volume and variety than it has previously handled.Visible- infrared instruments are on the 1996 Mars Global Surveyor, 2001 Mars Odyssey 2003 Mars Exploration Rovers, 2003 Mars Express, 2005 Mars Reconnaissance Orbiter; and likely on the 2007 and 2009 missions. Interpretations of those data sets provide a critical foundation for geologic and climatic interpretations as well as an opportunity to select landing sites. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | LPI-Contrib-1161 |
| 権利 | Copyright |
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