Organics and other molecules in the surfaces of Callisto and Ganymede

被引:163
作者
McCord, TB
Carlson, RW
Smythe, WD
Hansen, GB
Clark, RN
Hibbitts, CA
Fanale, FP
Granahan, JC
Segura, M
Matson, DL
Johnson, TV
Martin, PD
机构
[1] CALTECH,JET PROP LAB,PASADENA,CA 91109
[2] US GEOL SURVEY,DENVER,CO 80225
[3] SCI & TECHNOL INT INC,HONOLULU,HI
关键词
D O I
10.1126/science.278.5336.271
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Five absorption features are reported at wavelengths of 3.4, 3.88, 4.05, 4.25, and 4.57 micrometers in the surface materials of the Galilean satellites Callisto and Ganymede from analysis of reflectance spectra returned by the Galileo mission near-infrared mapping spectrometer. Candidate materials include CO2, organic materials (such as tholins containing C=N and C-H), SO2, and compounds containing an SH-functional group; CO2, SO2, and perhaps cyanogen [(CN)(2)] may be present within the surface material itself as collections of a few molecules each. The spectra indicate that the primary surface constituents are water ice and hydrated minerals.
引用
收藏
页码:271 / 275
页数:5
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