| タイトル | 2.7- to 4.1-micron spectrophotometry of icy satellites of Saturn and Jupiter |
| 著者（英） | Feierberg, M. A.; Lebofsky, L. A. |
| 著者所属（英） | Arizona Univ.|NASA Ames Research Center |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | Spectrophotometry is presented in the 2.7-4.1 micrometer spectral region for icy satellites of Saturn (Tethys, Dione, Rhea, Iapetus and Hyperion) and Jupiter (Europa, Ganymede and Callisto). The 3.6-micrometer reflectance peak characteristic of fine-grained water ice is observed prominently on the satellites of Saturn, faintly on the leading side of Europa, and not at all on Ganymede, Callisto or the dark side of Iapetus. The spectral reflectances of these icy satellites may be affected by their equilibrium surface temperatures and magnetospheric effects. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 86A10169 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/388267 |
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