Microscope spectrometer for the Phobos-Grunt mission

被引：2
|
作者：
Korablev, O. I. [1 ]
Bondarenko, A. V. [2 ]
Dokuchaev, I. V. [2 ]
Ivanov, A. Yu. [1 ]
Kozlov, O. E. [1 ]
Kottsov, V. A. [1 ]
Kiselev, A. B. [1 ]
Bibring, J. -P. [3 ,4 ]
Fourmond, J. -J. [3 ,4 ]
机构：
[1] Russian Acad Sci, Space Res Inst, Moscow 117810, Russia
[2] RASTR Technol Co, Moscow, Russia
[3] Univ Paris 11, Space Astrophys Inst, Orsay, France
[4] CNRS, F-91405 Orsay, France
来源：
SOLAR SYSTEM RESEARCH | 2010年 / 44卷 / 05期
关键词：
Solar System Research; Entrance Window; Scientific Payload; Phobos Grunt; Regolith Sample;
D O I：
10.1134/S0038094610050072
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Microscopy and spectroscopy are important methods of studies. The use of a microscope onboard a spacecraft is connected with the fact that the closer approach to the objects and the switch to the in situ measurement methods have become possible. The combination of taking an image and performing a spectral analysis forms a new type of instrument, so-called videospectrometers. The scientific payload of the Phobos-Grunt spacecraft includes the microscope spectrometer designed to analyze the composition of the surface regolith of Phobos in detail.
引用
收藏
页码：403 / 408
页数：6
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