Space weathering on airless bodies: Resolving a mystery with lunar samples

被引:547
作者
Pieters, CM [1 ]
Taylor, LA
Noble, SK
Keller, LP
Hapke, B
Morris, RV
Allen, CC
McKay, DS
Wentworth, S
机构
[1] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[2] Univ Tennessee, Dept Geol Sci, Knoxville, TN 37966 USA
[3] MVA Inc, Norcross, GA 30093 USA
[4] Univ Pittsburgh, Dept Geol & Planetary Sci, Pittsburgh, PA 15260 USA
[5] NASA, Lyndon B Johnson Space Ctr, Houston, TX 77058 USA
[6] Lockheed Martin Space Operat, Houston, TX 77058 USA
来源
METEORITICS & PLANETARY SCIENCE | 2000年 / 35卷 / 05期
关键词
D O I
10.1111/j.1945-5100.2000.tb01496.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Using new techniques to examine the products of space weathering of lunar soils, we demonstrate that nanophase reduced iron (npFe(0)) is produced on the surface of grains by a combination of vapor deposition and irradiation effects. The optical properties of soils (both measured and modeled) are shown to be highly dependent on the cumulative amount of npFe(0), which varies with different starting materials and the energetics of different parts of the solar system. The measured properties of intermediate albedo asteroids, the abundant S-type asteroids in particular, are shown to directly mimic the effects predicted for small amounts of npFe(0) on grains of an ordinary chondrite regolith. This measurement and characterization of space weathering products seems to remove a final obstacle hindering a link between the abundant ordinary chondrite meteorites and common asteroids.
引用
收藏
页码:1101 / 1107
页数:7
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