The detection of solid phosphorus and fluorine in the dust from the coma of comet 67P/Churyumov–Gerasimenko

Author:

Gardner Esko1ORCID,Lehto Harry J1,Lehto Kirsi2,Fray Nicolas3,Bardyn Anaïs4,Lönnberg Tuomas5,Merouane Sihane6,Isnard Robin3,Cottin Hervé3,Hilchenbach Martin6,

Affiliation:

1. Tuorla Observatory, Department of Physics and Astronomy, University of Turku, F-20014 Turku, Finland

2. Molecular Plant Biology, Department of Biochemistry, University of Turku, F-20014 Turku, Finland

3. Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA), UMR CNRS 7583, Université Paris-Est-Créteil, Université de Paris, Institut Pierre Simon Laplace (IPSL), Créteil, France

4. Earth and Planets Laboratory, Carnegie Institution of Washington, 5241 Broad Branch Road, Washington, DC 20015, USA

5. Department of Chemistry, University of Turku, F-20014 Turku, Finland

6. Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany

Abstract

ABSTRACT Here, we report the detection of phosphorus and fluorine in solid particles collected from the inner coma of comet 67P/Churyumov–Gerasimenko measured with the COmetary Secondary Ion Mass Analyser (COSIMA) instrument on-board the Rosetta spacecraft, only a few kilometers away from the comet nucleus. We have detected phosphorus-containing minerals from the presented COSIMA mass spectra, and can rule out e.g. apatite minerals as the source of phosphorus. This result completes the detection of life-necessary CHNOPS-elements in solid cometary matter, indicating cometary delivery as a potential source of these elements to the young Earth. Fluorine was also detected with CF+ secondary ions originating from the cometary dust.

Funder

Deutsches Zentrum für Luft- und Raumfahrt

Centre National d’Etudes Spatiales

European Space Agency

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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