| タイトル | Apollo 17 seismic profiling - Probing the lunar crust. |
| 著者（英） | Watkins, J. S.; Kovach, R. L. |
| 発行日 | 1973-06-08 |
| 言語 | eng |
| 内容記述 | Apollo 17 seismic data are interpreted to determine the structure of the lunar crust to a depth of several kilometers. Seismic velocity increases in a marked stepwise manner beneath the Taurus-Littrow region at the Apollo 17 site. A thickness of about 1200 meters is indicated for the infilling mare basalts at Taurus-Littrow. The apparent velocity is high (about 4 kilometers per second) in the material immediately underlying the basalts. |
| NASA分類 | SPACE SCIENCES |
| レポートNO | 73A32903 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/457149 |
