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COSIMA-Rosetta calibration for in situ characterization of 67P/Churyumov-Gerasimenko cometary inorganic compounds

Krüger, Harald (author)
Max Planck Institute for Solar System Research, Germany
Stephan, Thomas (author)
University of Chicago, US
Engrand, Cécile (author)
CNRS, France; University of Paris-Sud, France
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Briois, Christelle (author)
CNRS, France; University of Orléans, France
Siljeström, Sandra (author)
RISE,Medicinteknik
Merouane, Sihane (author)
Max Planck Institute for Solar System Research, Germany
Baklouti, Donia (author)
CNRS, France; University of Paris-Sud, France
Fischer, Henning (author)
Max Planck Institute for Solar System Research, Germany
Fray, Nicolas (author)
LISA Laboratoire Interuniversitaire des Systèmes Atmosphériques, France
Hornung, Klaus (author)
Universität der Bundeswehr, Germany
Lehto, Harry (author)
University of Turku, Finland
Orthous-Daunay, Francois-Régis (author)
CNRS, France; Université Grenoble Alpes, France
Rynö, Jouni (author)
Finnish Meteorological Institute, Finland
Schulz, Rita (author)
ESA European Space Agency, Netherlands
Silén, Johan (author)
Finnish Meteorological Institute, Finland
Thirkell, Laurent (author)
CNRS, France; University of Orléans, France
Trieloff, Mario (author)
Heidelberg University, Germany
Hilchenbach, Martin (author)
Max Planck Institute for Solar System Research, Germany
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 (creator_code:org_t)
Elsevier, 2015
2015
English.
In: Planetary and Space Science. - : Elsevier. - 0032-0633 .- 1873-5088. ; 117, s. 35-44
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • COmetary Secondary Ion Mass Analyzer (COSIMA) is a time-of-flight secondary ion mass spectrometry (TOF-SIMS) instrument on board the Rosetta space mission. COSIMA has been designed to measure the composition of cometary dust particles. It has a mass resolution m/Δm of 1400 at mass 100 u, thus enabling the discrimination of inorganic mass peaks from organic ones in the mass spectra. We have evaluated the identification capabilities of the reference model of COSIMA for inorganic compounds using a suite of terrestrial minerals that are relevant for cometary science. Ground calibration demonstrated that the performances of the flight model were similar to that of the reference model. The list of minerals used in this study was chosen based on the mineralogy of meteorites, interplanetary dust particles and Stardust samples. It contains anhydrous and hydrous ferromagnesian silicates, refractory silicates and oxides (present in meteoritic Ca-Al-rich inclusions), carbonates, and Fe-Ni sulfides. From the analyses of these minerals, we have calculated relative sensitivity factors for a suite of major and minor elements in order to provide a basis for element quantification for the possible identification of major mineral classes present in the cometary particles.

Subject headings

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geofysik (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geophysics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Kemi -- Analytisk kemi (hsv//swe)
NATURAL SCIENCES  -- Chemical Sciences -- Analytical Chemistry (hsv//eng)

Keyword

comet
cometary dust
interplanetary dust
micrometeorite
Rosetta
time-of-flight secondary ion mass spectrometry (TOF-SIMS)

Publication and Content Type

ref (subject category)
art (subject category)

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