月尘的性质及危害评述
Properties and Harmfulness of Lunar Dust: A Review
查看参考文献69篇
|
文摘
|
月尘是广泛分布于月球表面的微小颗粒, 大小约在30nm~20μm之间, 95%以上小于2μm, 中值粒径约为100~300nm, 形态复杂多变, 以玻璃小球、气泡构造、棱角状碎片为主, 含有大量纳米颗粒金属铁和玻璃质, 玻璃质含量超过50%, 尤其是<2μm的部分中, 玻璃质含量高达80%~90%, 化学成分与月壤基本类似, 在不同地貌单元也体现出SiO_2含量的差异.月尘的成分和颗粒特征使其具有独特的电磁性质和生物毒性, 容易粘附于航天器表面和进入航天员体内, 危害航天器和航天员的安全和健康, 严重影响月面探测的正常实施.因此, 对月尘的研究是保证月面探测工程正常实施的迫切需要;同时, 月尘是月球表面物质经历长期的太空作用形成的, 在颗粒成分和结构特征上保留了其演化过程的重要信息, 是研究月表物质和大气演化、太空风化作用等科学问题的关键线索.但是目前对月尘的颗粒微观成分和结构差异、电磁特性和光学特性, 纳米金属铁的特征和成因等方面的研究还不够深入, 限制了月表物质演化历史的研究和月尘粘结腐蚀性、生物毒理学具体机理的认识.在月尘研究中利用模拟月尘弥补月尘样品稀缺的局限, 并通过模拟实验加强以上方面的研究, 能够更好地满足科学问题和工程探测的实际需要. |
|
其他语种文摘
|
Lunar dust is the small particle widely distributed on the lunar surface, of which sizes range from 30 nm to 20 μm with the median diameter of 100-300 nm and more than 95% are less than 2 μm. The grains have complex shapes and usually show glass beads,vesicular texture, and angular shards. High contents of agglutinate glass and npFe~0 are the remarkable properties in mineral composition. The glass content is usually more than 50 vol%,and it can reach 80% to 90% in< 2.5 μm part Lunar dust is similar to lunar soil in elemental compositions, but it also shows different contents of SiO_2 in different areas. The composition and geometrical characteristics of lunar dust lead to special electromagnetic properties and biological toxicity. These properties might cause the lunar dust adhered to spacecraft and inhaled by astronauts easily, and then damage the spacecraft and threaten the health of astronauts. So, it is necessary to study lunar dust further to facilitate lunar surface exploration, which also can better the understanding of the evolution of lunar surface materials and lunar atmosphere due to the fact that lunar dust has been formed during a long time space weathering and conserves important information of space weathering history in the composition and microstructure of lunar dust grain Currently, the properties of lunar dust grains in micro-morphology and chemical composition, electromagnetic properties and spectral characteristics, the feature and origin of npFe~0 are still not clear, which challenges the understanding of the mechanism of lunar dust's adhesion,biological toxicity and space weathering. To meet the needs of lunar science and lunar exploration, studying the properties of lunar soil grains and process of space weathering by simulated experiments using lunar dust stimulants as a candidate might be an important trend in the coming decades. |
|
来源
|
地球科学
,2013,38(2):339-350 【核心库】
|
|
DOI
|
10.3799/dqkx.2013.033
|
|
关键词
|
月尘
;
颗粒
;
性质
;
危害
;
模拟月尘
|
|
地址
|
中国科学院地球化学研究所月球与行星科学研究中心, 贵阳, 550002
|
|
语种
|
中文 |
|
文献类型
|
研究性论文 |
|
ISSN
|
1000-2383 |
|
学科
|
地质学 |
|
基金
|
国家863计划
;
中国科学院地球化学研究所前沿领域项目
;
国家自然科学基金
;
中国科学院西部之光人才培养计划
|
|
文献收藏号
|
CSCD:4787735
|
参考文献 共
69
共4页
|
|
1.
Allen C C. Experimental Space Weathering of Lunar Soils.
Meteoritics,1995,30(5):479-480
|
CSCD被引
1
次
|
|
|
|
|
2.
Anand M. New Lunar Mineral HAPKEITE-Product of Impact-Induced Vapor-Phase Deposition in the Regolith.
34th Proceedings of Lunar and Planetary Science Conference,2003:1818-1819
|
CSCD被引
1
次
|
|
|
|
|
3.
Anand M. Space Weathering on Airless Planetary Bodies:Clues from the Lunar Mineral Hapkeite.
Proceedings of the National Academy of Sciences,2004,101(18):6847-6851
|
CSCD被引
12
次
|
|
|
|
|
4.
Batsura L D. Morphology of Experimental Pneumoconiosis Developing after Exposure to Lunar Soil.
Bulletin of Experimental Biology and Medicine,1981,92(9):376-379
|
CSCD被引
1
次
|
|
|
|
|
5.
Bentley P M. The Effect ofα-Fe Crystallites on the Magnetic Structures of Fe100-xZrx Glasses.
Journal of Physical: Conference Series,2010,200(3):3
|
CSCD被引
1
次
|
|
|
|
|
6.
Bernatowicz T J. Origin of Amorphous Rims on Lunar Soil Grains.
25th Lunar and Planetary Science Conference.XXV,1994:105-106
|
CSCD被引
1
次
|
|
|
|
|
7.
Bibring J P. Ultrathin Amorphouscoatings on Lunar Dust Grains.
Science,1972,175(4023):753-755
|
CSCD被引
8
次
|
|
|
|
|
8.
Buhler C R. Test Method for in Situ Electrostatic Characterization of Lunar Dust.
Institute of Electrical and Electronics Engineers,2007:1-19
|
CSCD被引
2
次
|
|
|
|
|
9.
Calle C I. Particle Removal by Electrostatic and Dielectrophoretic Forces for Dust Control during Lunar Exploration Missions.
Journal of Electrostatics,2009,67(2/3):89-92
|
CSCD被引
9
次
|
|
|
|
|
10.
Christoffersen R. Microstructure, Chemistry,and Origin of Grain Rims on Ilmenite from the Lunar Soil Finest Fraction.
Meteoritics & Planetary Science,1996,31(6):835-848
|
CSCD被引
5
次
|
|
|
|
|
11.
Doug R. Some Expected Mechanical Characteristics of Lunar Dust:A Gological View.
Space Technology and Applications International Forum. AIP Conf.Proc.,969,2008:949-955
|
CSCD被引
1
次
|
|
|
|
|
12.
Fischer E M. Remote Determination of Exposure Degree and Iron Concentration of Lunar Soils Using VIS-NIR Spectroscopic Methods.
Icarus,1994,111:475-488
|
CSCD被引
8
次
|
|
|
|
|
13.
Fuller M. The Magnetic Characterstics of Returned Lunar Samples and Their Implications for Regolith Processes.
Moon,1975,13:327-328
|
CSCD被引
1
次
|
|
|
|
|
14.
Gromme C S. Magnetic Properties of Lunar Samples 12502and 12065.Second Lunar Science Conference.
Geochimica et Cosmochimica Acta,1971,3(Suppl.2):2491-2499
|
CSCD被引
1
次
|
|
|
|
|
15.
Guthrie G D. Mineral Properties and Their Contribution to Particle Toxicity.
Environment Health Perspect,1997,105(Suppl.5):1003-1011
|
CSCD被引
1
次
|
|
|
|
|
16.
Hanneken J W. The Frequency Dependence of the Viscous Component of the Magnetic Susceptibility of Lunar Rock and Soil Samples.
Earth and Planetary Science Letters,1976,32(1):45-50
|
CSCD被引
1
次
|
|
|
|
|
17.
Hapke B W. The Vapor Deposition Model of Space Weathering:Strawman Pardigm for the Moon.
Workshop on New Views of the Moon:Integrated Remotely Sensed,Geophysical, and Sample Datesets,1998
|
CSCD被引
1
次
|
|
|
|
|
18.
Hapke B W. Space Weathering from Mercury to the Asteroid Belt.
Journal of Geophysical Research,2001,106(E5):10039-10073
|
CSCD被引
32
次
|
|
|
|
|
19.
Hapke B. Effects of Vapor-Phase Deposition Processes on the Optical,Chemical, and Magnetic Properties of the Lunar Regolith.
Earth, Moon,and Planets,1975,13(1/3):339-353
|
CSCD被引
12
次
|
|
|
|
|
20.
Heiken G H.
Lunar Sourcebook:A User's Guide to the Moon,1991
|
CSCD被引
15
次
|
|
|
|
|
了解气象卫星更多信息，请访问