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

  • P. Pinet*
  • , P. Cerroni
  • , J. L. Josset
  • , S. Beauvivre
  • , S. Chevrel
  • , K. Muinonen
  • , Y. Langevin
  • , M. A. Barucci
  • , M. C. De Sanctis
  • , Yu Shkuratov
  • , V. Shevchenko
  • , P. Plancke
  • , B. A. Hofmann
  • , M. Josset
  • , P. Ehrenfreund
  • , Z. Sodnik
  • , D. Koschny
  • , M. Almeida
  • , B. Foing
  • *Šī darba korespondējošais autors
  • Institut de Recherche en Astrophysique et Planétologie (IRAP)
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Space-X
  • Helsinki Observatory
  • Université Paris-Saclay
  • Observatoire de Paris
  • V. N. Karazin Kharkiv National University
  • Lomonosov Moscow State University
  • ESA/ESTEC Power and Control Data Division
  • Natural History Museum
  • University of Neuchatel
  • Leiden University
  • European Space Research and Technology Centre (ESTEC)

Zinātniskās darbības rezultāts: Devums žurnālamZinātniskais raksts (žurnālā)koleģiāli recenzēts

19 Atsauces (Scopus)

Kopsavilkums

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.

OriģinālvalodaAngļu
Lapas (no-līdz)1309-1318
Lapu skaits10
ŽurnālsPlanetary and Space Science
Sējums53
Izdevuma numurs13
DOIs
Publikācijas statussPublicēts - nov. 2005
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