| タイトル | The source of sublimates on the Apollo 15 green and Apollo 17 orange glass samples |
| 著者（英） | Butler, P., Jr.; Meyer, C., Jr.; Anderson, D. H.; Mckay, D. S. |
| 著者所属（英） | NASA Johnson Space Center |
| 発行日 | 1975-01-01 |
| 言語 | eng |
| 内容記述 | Elemental analyses of the thin film of micromounds which coat the surfaces of Apollo 15 green glass and Apollo 17 orange glass are reported. It is thought that Zn, Ga, Pb, Cu, Tl, S, F, and Cl condensed as a sublimate on the outside surface of these glass particles in lava fountains about 3.4 and 3.6 b.y. ago (Apollos 15 and 17, respectively). The heavy metals enriched in these samples may have been mobilized in a halide- and sulfide-rich vapor, while the source of these elements and of the glass may be a sulfide- and halide-rich pyroxenite inside the moon. The isotopic composition of lead on the surface of individual particles was determined, and the composition is considered with respect to the evolution of the source region. The lead on the surfaces is similar to lead that has been mixed into other soils and breccias at nearby sites. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 78A46696 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/431575 |
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