| タイトル | The Electrostatic Environments of Mars and the Moon |
| 本文（外部サイト） | http://hdl.handle.net/2060/20110008730 |
| 著者（英） | Calle, Carlos I. |
| 著者所属（英） | NASA Kennedy Space Center |
| 発行日 | 2011-04-11 |
| 言語 | eng |
| 内容記述 | The electrical activity present in the environment near the surfaces of Mars and the moon has very different origins and presents a challenge to manned and robotic planetary exploration missions. Mars is covered with a layer of dust that has been redistributed throughout the entire planet by global dust storms. Dust, levitated by these storms as well as by the frequent dust devils, is expected to be electrostatically charged due to the multiple grain collisions in the dust-laden atmosphere. Dust covering the surface of the moon is expected to be electrostatically charged due to the solar wind, cosmic rays, and the solar radiation itself through the photoelectric effect. Electrostatically charged dust has a large tendency to adhere to surfaces. NASA's Mars exploration rovers have shown that atmospheric dust falling on solar panels can decrease their efficiency to the point of rendering the rover unusable. And as the Apollo missions to the moon showed, lunar dust adhesion can hinder manned and unmanned lunar exploration activities. Taking advantage of the electrical activity on both planetary system bodies, dust removal technologies are now being developed that use electrostatic and dielectrophoretic forces to produce controlled dust motion. This paper presents a short review of the theoretical and semiempirical models that have been developed for the lunar and Martian electrical environments. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | KSC-2011-053 |
| 権利 | No Copyright |
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