| タイトル | Microcraters on lunar samples |
| 本文（外部サイト） | http://hdl.handle.net/2060/19780005021 |
| 著者（英） | Storzer, D.; Hartung, J. B.; Fechtig, H.; Nagel, K.; Gentner, W.; Neukum, G.; Schneider, E. |
| 著者所属（英） | Max-Planck-Inst. fuer Kernphysik |
| 発行日 | 1977-01-01 |
| 言語 | eng |
| 内容記述 | The lunar microcrater phenomenology is described. The morphology of the lunar craters is in almost all aspects simulated in laboratory experiments in the diameter range from less than 1 nu to several millimeters and up to 60 km/s impact velocity. An empirically derived formula is given for the conversion of crater diameters into projectile diameters and masses for given impact velocities and projectile and target densities. The production size frequency distribution for lunar craters in the crater size range from approximately 1 nu to several millimeters in diameter is derived from various microcrater measurements within a factor of up to 5. Particle track exposure age measurements for a variety of lunar samples have been performed. They allow the conversion of the lunar crater size frequency production distributions into particle fluxes. The development of crater populations on lunar rocks under self-destruction by subsequent meteoroid impacts and crater overlap is discussed and theoretically described. Erosion rates on lunar rocks on the order of several millimeters per 10 yr are calculated. Chemical investigations of the glass linings of lunar craters yield clear evidence of admixture of projectile material only in one case, where the remnants of an iron-nickel micrometeorite have been identified. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 78N12964 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/569573 |
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