SMART-1 highlights and relevant studies on early bombardment and geological processes on rocky planets

  • B. H. Foing
  • , G. D. Racca
  • , J. L. Josset
  • , D. Koschny
  • , D. Frew
  • , M. Almeida
  • , J. Zender
  • , D. Heather
  • , S. Peters
  • , A. Marini
  • , L. Stagnaro
  • , S. Beauvivre
  • , M. Grande
  • , B. Kellett
  • , J. Huovelin
  • , A. Nathues
  • , U. Mall
  • , P. Ehrenfreund
  • , P. McCannon

Research output: Contribution to journalConference articlepeer-review

Abstract

We present results from SMART-1 science and technology payload, in the context of the Nobel symposium on 'Physics of Planetary Systems'. SMART-1 is Europe' first lunar mission (Foing et al 2000 LPSC XXXI Abstract #1677 (CDROM); Foing et al 2001 Earth, Moon Planets 85-86 523-31; Marini et al 2002 Adv. Space Res. 30 1895-900; Racca et al 2001 Earth Moon Planets 85-86 379-95, Racca et al 2002 Planet Space Sci. 50 1323-37) demonstrating technologies for future science and exploration missions, and providing advances in our understanding of lunar origin and evolution, and general planetary questions. The mission also contributes a step in developing an international program of lunar exploration. The spacecraft, launched on 27 September 2003 as an Ariane 5 Auxiliary passenger to geostationary transfer orbit (GTO), performed a 14-month long cruise using a tiny thrust of electric propulsion alone, reached lunar capture in November 2004, and lunar science orbit in March 2005. SMART-1 carried 7 hardware experiments (Foing et al 2003 Adv. Space Res. 31 2323, Foing et al 2005 LPI/LPSC XXXVI 2404 (CDROM)) performing 10 investigations, including 3 remote-sensing instruments, used during the cruise, the mission' nominal six-months and one-year extension in lunar science orbit. Three remote sensing instruments, D-CIXS, SIR and AMIE, have returned data that are relevant to a broad range of lunar studies. The mission provided regional and global x-ray measurements of the Moon, global high-spectral resolution NIR spectrometry, high spatial resolution colour imaging of selected regions. The South Pole-Aitken Basin (SPA) and other impact basins have been prime targets for studies using the SMART-1 suite of instruments. Combined, these should aid a large number of science studies, from bulk crustal composition and theories of lunar origin/evolution, the global and local crustal composition, to the search for cold traps at the lunar poles and the mapping of potential lunar resources. We present here SMART-1 results relevant to the study of the early bombardment and geological processes on rocky planets. Further information and updates on the SMART-1 mission can be found on the ESA Science and Technology web pages, at: http://sci.esa.int/smart-1/.

Original languageEnglish
Article number014026
JournalPhysica Scripta T
VolumeT130
DOIs
Publication statusPublished - 2008
EventNobel Symposium 135: Physics of Planetary Systems - Stockholm, Sweden
Duration: 18 Jun 200722 Jun 2007

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