| タイトル | Recent spectroscopic findings concerning clay/water interactions at low humidity: Possible applications to models of Martian surface reactivity |
| 本文（外部サイト） | http://hdl.handle.net/2060/19920004447 |
| 著者（英） | Coyne, L.; Scattergood, T. W.; Howard, L.; Bishop, J. |
| 著者所属（英） | NASA Ames Research Center |
| 発行日 | 1991-10-01 |
| 言語 | eng |
| 内容記述 | A feasibility study assessing the utility of the adaptation of near infrared correlation spectroscopy to quantifying iron and adsorbed water in some clay-based Mars soil analog materials (MarSAM's). The work was intended to constitute Phase 1 of an approach to identifying optical analytical wavelength regions, not only for important mineral classes, but for chemically active centers within them. Many of these centers are common to unrelated mineral classes and of disproportionate influence relative to the mineral structure as a whole in determining the surface reactivity of mineral surfaces. We previously reported linearity between reflectance and total iron and total moisture over a large range of both key variables. We also discovered interesting relationships between the intensity of iron bands and the relative humidity of the systems. These relationships were confirmed. We also show that, in the low humidity range, reflectance is linearly dependent on a different kind of water from that best representing the full humidity range (the kind of water associated, in clays, with surface acidity). These relationships and the sensitivity and capability of quantitation of near infrared data indicate high promise with the production of reactive surface intermediates of products of surface reactions. |
| NASA分類 | SPACE BIOLOGY |
| レポートNO | 92N13665 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/129596 |
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