Identification of iron sulphide grains in protoplanetary disks

L. P. Keller (), S. Hony, J. P. Bradley, F. J. Molster, L. B. F. M. Waters, J. Bouwman, A. de Koter, D. E. Brownlee, G. J. Flynn, T. Henning and H. Mutschke
Additional contact information
L. P. Keller: Mail Code SR, NASA Johnson Space Center
S. Hony: Astronomical Institute Anton Pannekoek
J. P. Bradley: Georgia Institute of Technology
F. J. Molster: ESTEC/ESA, RSSD-ST
L. B. F. M. Waters: Astronomical Institute Anton Pannekoek
J. Bouwman: CEA, DSM, DAPNIA, Service d'Astrophysique, CEN Saclay
A. de Koter: Astronomical Institute Anton Pannekoek
D. E. Brownlee: University of Washington
G. J. Flynn: SUNY
T. Henning: Astrophysical Institute and University Observatory
H. Mutschke: Astrophysical Institute and University Observatory

Nature, 2002, vol. 417, issue 6885, 148-150

Abstract: Abstract Sulphur is depleted in cold dense molecular clouds with embedded young stellar objects1, indicating that most of it probably resides in solid grains. Iron sulphide grains are the main sulphur species in cometary dust particles2,3, but there has been no direct evidence for FeS in astronomical sources4, which poses a considerable problem, because sulphur is a cosmically abundant element. Here we report laboratory infrared spectra of FeS grains from primitive meteorites, as well as from pyrrhotite ([Fe, Ni]1-xS) grains in interplanetary dust, which show a broad FeS feature centred at ∼23.5 micrometres. A similar broad feature is seen in the infrared spectra of young stellar objects, implying that FeS grains are an important but previously unrecognized component of circumstellar dust. The feature had previously been attributed to FeO5,6,7. The observed astronomical line strengths are generally consistent with the depletion of sulphur from the gas phase1, and with the average Galactic sulphur/silicon abundance ratio8. We conclude that the missing sulphur has been found.

Date: 2002
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DOI: 10.1038/417148a

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