Westfälische Wilhelms-Universität Münster: Forschungsbericht 2003-2004 - Institut für Planetologie

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Institut für Planetologie

Tel. (0251) 83-33492
Fax: (0251) 83-36301
e-mail: ifp@uni-muenster.de
www: http://ifp.uni-muenster.de/
Wilhelm-Klemm-Str. 10
48149 Münster
Geschäftsführender Direktor: HDoz. Dr. Thomas Stephan

Forschungsschwerpunkte 2003 - 2004  
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Experimentelle und Analytische Planetologie
Combined LIPS/RAMAN spectrometer for planetary exploration

 
Planetary in-situ analysis is going to become one of the most important tools for exploring the accessible celestial bodies. Chemical, mineralogical, structural, isotopic, and molecular information will provide stringent boundary conditions for the origin and evolution of these bodies and hence of the solar system. The past showed some unprecedented examples of operating in-situ analysis instruments and even rather complex instrument facilities are at present underway. Although their capabilities are remarkable, these "first generation" instruments still suffer from constraints in terms of size, mass, and operations for the accommodating systems. They pose restrictions in particular on the most recently projected explorative missions such as ESA's EXOMARS mission that aims at large operating radii of some kilometers or some tens of kilometers. Whereas the classical operational scenario was more or less stationary, the high degree of mobility calls for a new type of instrumentation, which can be characterized as follows:
  • Short measurement duration: seconds instead of hours
  • High sensitivity, high repetition rate, high reproducibility
  • Low mass, size, and resource needs
  • High flexibility with respect to type, shape, and size of sample material
  • Robustness towards surface contamination.
Laser-Induced-Plasma-Spectrometry (LIPS) in combination with Raman spectroscopy has the potential to meet these requirements and to enable in-situ elemental and mineralogical analyses with a new level of accuracy, performance, and operational flexibility. In the EGS 2003 conference, the concept of a combined LIPS / Raman spectrometer has been introduced. With the work on a definition study for such an instrument terminated, the instrument has been proposed for ESA's ExoMars mission, passing the scientific peer review with a very positive result. This contribution describes the final results of the LIPS/Raman definition study, as well as the accommodation perspectives on different types of missions.

Drittmittelgeber:

ESTEC/ESA

Beteiligte Wissenschaftler:

R. Bertrand (von Hoerner Sulger GmbH, Schwetzingen, Germany); A. Del Bianco (IPAC Improve Process Analytics and Control GmbH, Villach, Austria); B. Harnisch (European Space Agency, Noordwijk, The Netherlands); E. K. Jessberger (Leiter); P. Peuser (EADS LG-ES, München, Germany); J. Romstedt (European Space Agency, Noordwijk, The Netherlands); K. Schneider (Star Optron Schneider GmbH, Mannheim, Germany)

Veröffentlichungen:

Bertrand R., Del Bianco A., Harnisch B., Jessberger E. K., Peuser P., Romstedt J. and Schneider K. (2004) Combined LIPS/Raman spectrometer for planetary exploration. EGU 1st General Assembly, Nice, #EGU04-A-04533.

 

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