The advanced Moon micro-imager experiment (AMIE) on SMART-1: Scientific goals and expected results

被引：11

作者：

Pinet, P

Cerroni, P

Josset, JL

Beauvivre, S

Chevrel, S

Muinonen, K

Langevin, Y

Barucci, MA

De Sanctis, MC

Shkuratov, Y

Shevchenko, V

Plancke, P

Hofmann, BA

Josset, M

Ehrenfreund, P

Sodnik, Z

Koschny, D

Almeida, M

Foing, B

机构：

[1] Univ Toulouse 3, Dynam Terrestre & Planetaire UMR 5562, CNRS, GRGS,Observ Midi Pyrenees, F-31400 Toulouse, France

[2] IASF, Area Ric Cnr, I-00133 Rome, Italy

[3] Ctr Space Explorat, Space X, Neuchatel, Switzerland

[4] Helsinki Observ, Helsinki, Finland

[5] IAS, F-91405 Orsay, France

[6] Observ Paris, OBSPM, Meudon, France

[7] Kharkov Natl Univ, Inst Astron, UA-61022 Kharkov, Ukraine

[8] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia

[9] ESA, ESTEC Power & Control Data Div, NL-2201 Noordwijk, Netherlands

[10] Museum Hist Nat, Bern, Switzerland

[11] Univ Neuchatel, Inst Geol, CH-2000 Neuchatel, Switzerland

[12] Leiden Observ, NL-2300 RA Leiden, Netherlands

[13] Austrian Acad Sci, NL-2300 RA Leiden, Netherlands

[14] ESA Space Sci Dept, NL-2201 Noordwijk, Netherlands

来源：

PLANETARY AND SPACE SCIENCE | 2005年 / 53卷 / 13期

关键词：

Moon; SMART-1 ESA mission; orbital photometry; spectral imaging;

D O I：

10.1016/j.pss.2005.06.003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The advanced Moon micro-imager experiment (AMIE) is the imaging system on board ESA mission to the Moon SMART-1; it makes use of a miniaturised detector and micro-processor electronics developed by SPACE X in the frame of the ESA technical programme. The AMIE micro-imager will provide high resolution CCD images of selected lunar areas and it will perform colour imaging through three filters at 750, 915 and 960 nm with a maximum resolution of 46 m/pixel at the perilune of 500 km. Specific scientific objectives will include (1) imaging of high latitude regions in the southern hemisphere, in particular the South Pole Aitken basin (SPA) and the permanently shadowed regions close to the South Pole, (2) determination of the photometric properties of the lunar surface from observations at different phase angles (physical properties of the regolith), (3) multi-band imaging for constraining the chemical and mineral composition of the surface, (4) detection and characterisation of lunar non-mare volcanic units, (5) study of lithological variations from impact craters and implications for crustal heterogeneity. The AMIE micro-imager will also support a Laser-link experiment to Earth, an On Board Autonomous Navigation investigation and a Lunar libration experiment coordinated with radio science measurements. (c) 2005 Elsevier Ltd. All rights reserved.

引用

页码：1309 / 1318

页数：10

共 13 条

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Foing, BH
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Zender, J
Heather, J
Grande, M
Huovelin, J
Keller, HU
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Josset, JL
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Foing, BH
Josset, JL
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Yu. G. Shkuratov
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P. Pinet
V. V. Shevchenko
B. H. Foing
J.-L. Josset
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Koschny, D
Almeida, M
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[J]. PLANETARY AND SPACE SCIENCE, 2018, 151 : 141 - 148

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