Iron
sulphides have long been recognized as a major component of meteorites, but they
have escaped detection in observations of objects similar to the early solar nebulae.
This poses a dilemma, as sulphur is a cosmically abundant element. A broad feature
identified in infrared spectra of iron sulphide grains from meteorites and interplanetary
dust particles is now shown to match one seen in the Infrared Space Observatory
spectra of young stellar objects. The feature, previously attributed to iron oxide,
implies that iron sulphide grains are an important but previously unrecognized
component of circumstellar dust.
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 & H. MUTSCHKE Nature417, 148150 (9 May 2002)
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