| タイトル | Dark matter in the solar system |
| 著者（英） | Cruikshank, Dale P. |
| 著者所属（英） | Hawaii Univ. |
| 発行日 | 1987-01-01 |
| 言語 | eng |
| 内容記述 | Many small bodies in the solar system, including planetary satellites, comets, and asteroids, have a surface component consisting at least in part of a very low albedo (0.06 or less) solid substance of neutral or red color in the wavelength region 0.3-2.5 microns. Laboratory spectra of organic residues from meteorites and mixtures with hydrous silicates suggest that complex mixtures of complex organic molecules (kerogens) together with aqueous alteration products of igneous minerals may be the source of the dark matter that is distributed so widely throughout the solar system. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 88A19915 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/373589 |
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