Results. We found that gas-phase silicon was present throughout the Rosetta mission. Furthermore, the presence of sodium and iron atoms near the comet's perihelion confirms that sputtering cannot be the sole release process for refractory elements into the gas phase. Nickel was found to be below the detection limit. The search for parent species of any of the identified gas phase refractories has not been successful. Upper limits for a suite of possible fragment species (SiH, SiC, NaH, etc.) of larger parent and daughter species have been obtained. Furthermore, Si did not exhibit the same drop in signal as do common cometary gases when the spacecraft is pointed away from the nucleus. The combined results suggest that a direct release of elemental species from small grains on the surface of the nucleus or from small grains in the surrounding coma is a more likely explanation than the previous assumption of release via the dissociation of gaseous parent molecules.
@article{arxiv.2112.08965,
title = {Refractory elements in the gas phase for comet 67P/Churyumov-Gerasimenko},
author = {Martin Rubin and Kathrin Altwegg and Jean-Jacques Berthelier and Michael R. Combi and Johan De Keyser and Frederik Dhooghe and Stephen Fuselier and Tamas I. Gombosi and Nora Hänni and Daniel Müller and Boris Pestoni and Susanne F. Wampfler and Peter Wurz},
journal= {arXiv preprint arXiv:2112.08965},
year = {2022}
}