| タイトル | The viscosity of Miranda |
| 本文（外部サイト） | http://hdl.handle.net/2060/19870013912 |
| 著者（英） | Cassen, P. M.; Reynolds, R. T.; Thomas, P. J.; Squyres, S. W. |
| 著者所属（英） | NASA Ames Research Center |
| 発行日 | 1987-05-01 |
| 言語 | eng |
| 内容記述 | Voyager 2 images of Miranda revealed a significant history of geological activity. Overlying an apparently ancient cratered terrain are assemblages of concentric ridges, scarps, and dark banded material. The problems that evolutionary thermal and structural modes of Miranda must face, to provide a convincing explanation for such topographic complexity, are examined. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 87N23345 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/150523 |
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