Unraveling the zebra: Clues to the Iapetus dark material composition

被引:28
作者
Vilas, F
Larson, SM
Stockstill, KR
Gaffey, MJ
机构
[1] UNIV ARIZONA,LUNAR & PLANETARY LAB,TUCSON,AZ 85721
[2] LUNAR & PLANETARY INST,HOUSTON,TX 77058
[3] RENSSELAER POLYTECH INST,DEPT EARTH & ENVIRONM SCI,TROY,NY 14853
基金
美国国家航空航天局;
关键词
D O I
10.1006/icar.1996.0202
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A linear mixing model has been used to separate the high-resolution visible/near-infrared reflectance spectrum of the Iapetus dark material from the spectra of the leading and trailing sides of Iapetus. A distinct absorption feature centered at 0.67 mu m is apparent in the spectrum. A slight inflection covering 0.4 to 0.6 mu m and a change in slope near 0.73 mu m suggesting the lower wavelength edge of an absorption are also present. These absorption features are attributed to the (6)A(1) --> T-4(2)(G) and (6)A(1)--> T-4(1)(G) charge transfer transitions in minerals such as goethite and hematite that are products of the aqueous alteration of anhydrous silicates. We confirm the strong, positive spectral slope attributed to organic material. (C) 1996 Academic Press, Inc.
引用
收藏
页码:262 / 267
页数:6
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