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Smallsat version of the European Moon Orbiting Observatory (MORO)

  • G. D. Racca*
  • , B. H. Foing
  • , J. B. Farrow
  • , C. P. Chaloner
  • *Šī darba korespondējošais autors
  • European Space Research and Technology Centre (ESTEC)
  • Airbus Group

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

Kopsavilkums

As the third medium-class mission in the ESA's Horizon 2000 science programme, a Moon Orbiting Observatory (MORO) was proposed for global mapping of lunar topography, mineralogy, geochemistry and gravity. The growing need to reduce the cost of the space missions led the study team to look for several approaches to limit the costs. It was decided therefore to study in parallel to the baseline a smallsat version of MORO which would just address the most important scientific issues in complement to Clementine, Lunar Prospector and Lunar A, notably gravimetry and high accuracy stereo imaging, topography, mineralogy and some elemental composition detection capability. This resulted in halving the payload mass (∼42 kg) and reducing substantially the spacecraft dry mass (≤300 kg). Such a small satellite can be placed into a lunar transfer orbit directly by a number of emerging new small-medium class launchers. The paper presents the mission and spacecraft design and describes the areas where the smallsat approach has allowed the largest cost reductions.

OriģinālvalodaAngļu
Lapas (no-līdz)121-131
Lapu skaits11
ŽurnālsActa Astronautica
Sējums39
Izdevuma numurs1-4
DOIs
Publikācijas statussPublicēts - 1996
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