| タイトル | Passive seismic experiment - A summary of current status |
| 著者（英） | Horvath, P.; Ibrahim, A. K.; Dorman, H. J.; Nakamura, Y.; Latham, G. V.; Koyama, J. |
| 著者所属（英） | Marine Science Inst. |
| 発行日 | 1978-01-01 |
| 言語 | eng |
| 内容記述 | The data set obtained from the four-station Apollo seismic network including signals from approximately 11,800 events, is surveyed. Some refinement of the lunar model will result, but its gross features remain the same. Attention is given to the question of a small, molten lunar core, the answer to which remains dependent on analysis of signals from a far side impact. Seventy three sources of repeating, deep moonquakes have been identified, thirty nine of which have been accurately located. Concentrated at depths from 800 to 1000 km, the periodicities of these events have led to the hypothesis that they are generated by tidal stresses. Lunar seismic data has also indicated that the meteoroid population is ten times lower than originally determined from earth based observations. Lunar seismic activity is much lower and mountainous masses show no sign of sinking, in contrast to earth, as a result of the lunar crust being four times thicker. While much work remains to be done, significant correlation between terrestrial and lunar observations can be seen. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 79A39301 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/426672 |
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