Refractory elements in the gas phase at comet 67P/Churyumov-Gerasimenko [EPA]

http://arxiv.org/abs/2112.08965


Results. 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 below 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, …) of larger parent and daughter species have been obtained. Furthermore, Si did not exhibit the same drop in signal like common cometary gases when the spacecraft was pointed away from the nucleus. The combined results suggest that direct release of elemental species from small grains on the surface of the nucleus and/or from small grains in the surrounding coma are more likely than release through dissociation of gaseous parent molecules.

Read this paper on arXiv…

M. Rubin, K. Altwegg, J. Berthelier, et. al.
Fri, 17 Dec 21
61/72

Comments: Accepted for publication in A&A