Sulphur-bearing species in the coma of comet 67P/Churyumov–Gerasimenko

Calmonte, Ursina Maria; Altwegg, Kathrin; Balsiger, Hans; Berthelier, J. J.; Bieler, André; Cessateur, G.; Dhooghe, F.; van Dishoeck, E. F.; Fiethe, B.; Fuselier, S. A.; Gasc, Sébastien; Gombosi, T. I.; Hässig, Myrtha; Le Roy, Léna; Rubin, Martin; Sémon, Thierry; Tzou, Chia-Yu; Wampfler, Susanne (2016). Sulphur-bearing species in the coma of comet 67P/Churyumov–Gerasimenko. Monthly notices of the Royal Astronomical Society, 462(Suppl1), S253-S273. Oxford University Press 10.1093/mnras/stw2601

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Several sulphur-bearing species have already been observed in different families of comets. However, the knowledge on the minor sulphur species is still limited. The comet’s sulphur inventory is closely linked to the pre-solar cloud and holds important clues to the degree of reprocessing of the material in the solar nebula and during comet accretion. Sulphur in pre-solar clouds is highly depleted, which is quite puzzling as the S/O ratio in the diffuse interstellar medium is cosmic. This work focuses on the abundance of the previously known species H2S, OCS, SO, S2, SO2 and CS2 in the coma of comet 67P/Churyumov–Gerasimenko measured by Rosetta Orbiter Spectrometer for Ion and Neutral Analysis/Double Focusing Mass Spectrometer between equinox and perihelion 2015. Furthermore, we present the first detection of S3, S4, CH3SH and C2H6S in a comet, and we determine the elemental abundance of S/O in the bulk ice of (1.47 ± 0.05) × 10−2. We show that SO is present in the coma originating from the nucleus, but not CS in the case of 67P, and for the first time establish that S2 is present in a volatile and a refractory phase. The derived total elemental sulphur abundance of 67P is in agreement with solar photospheric elemental abundances and shows no sulphur depletion as reported for dense interstellar clouds. Also the presence of S2 at heliocentric distances larger than 3 au indicates that sulphur-bearing species have been processed by radiolysis in the pre-solar cloud and that at least some of the ice from this cloud has survived in comets up the present.

Item Type:

Journal Article (Original Article)

Division/Institute:

08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences
10 Strategic Research Centers > Center for Space and Habitability (CSH)

UniBE Contributor:

Calmonte, Ursina Maria; Altwegg, Kathrin; Balsiger, Hans; Bieler, André; Gasc, Sébastien; Hässig, Myrtha; Le Roy, Léna; Rubin, Martin; Sémon, Thierry; Tzou, Chia-Yu and Wampfler, Susanne

Subjects:

500 Science > 520 Astronomy
600 Technology > 620 Engineering
500 Science > 530 Physics

ISSN:

0035-8711

Publisher:

Oxford University Press

Language:

English

Submitter:

Katharina Weyeneth-Moser

Date Deposited:

30 Jun 2017 14:37

Last Modified:

30 Jun 2017 14:37

Publisher DOI:

10.1093/mnras/stw2601

BORIS DOI:

10.7892/boris.97006

URI:

https://boris.unibe.ch/id/eprint/97006

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