Physical properties of meteorites—Applications in space missions to asteroids
Physical properties of meteorites—Applications in space missions to asteroids
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DOI：
10.1111/j.1945-5100.2008.tb00689.x
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发表时间：
2008-06
影响因子：
2.2
通讯作者：
T. Kohout;G. Kletetschka;T. Elbra;T. Adachi;V. Mikula;L. Pesonen;P. Schnabl;S. Šlechta
中科院分区：
文献类型：
--
作者：
T. Kohout;G. Kletetschka;T. Elbra;T. Adachi;V. Mikula;L. Pesonen;P. Schnabl;S. Šlechta
翻译后摘要-基于反射光谱和化学/矿物学遥感方法，一般认为，小行星的母体大多数陨石到达地球。然而，更详细的观察表明，小行星和陨石之间的成分存在差异，导致在寻找陨石-小行星匹配时遇到困难。
Abstract— Based on reflectance spectroscopy and chemical/mineralogical remote sensing methods, it is generally assumed that asteroids are parent bodies for most meteorites reaching the Earth. However, more detailed observations indicate that differences exist in composition between asteroids and meteorites resulting in difficulties when searching for meteorite‐asteroid match.