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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
  • *Corresponding author for this work
  • European Space Research and Technology Centre (ESTEC)
  • Airbus Group

Research output: Contribution to journalArticlepeer-review

Abstract

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.

Original languageEnglish
Pages (from-to)121-131
Number of pages11
JournalActa Astronautica
Volume39
Issue number1-4
DOIs
Publication statusPublished - 1996
Externally publishedYes

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