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  • Online Resource  (2)
  • EDP Sciences  (2)
  • Pestoni, B.  (2)
  • 2020-2024  (2)
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  • Online Resource  (2)
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  • EDP Sciences  (2)
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  • 2020-2024  (2)
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  • 1
    In: Astronomy & Astrophysics, EDP Sciences, Vol. 662 ( 2022-6), p. A69-
    Abstract: Context. Isotopic abundances in comets are key to understanding and reconstructing the history and origin of material in the Solar System. Data for deuterium-to-hydrogen (D/H) ratios in water are available for several comets. However, no long-term studies of the D/H ratio in water of a comet during its passage around the Sun have been reported thus far. Linear alkanes are important organic molecules that have been found on several Solar System bodies, including comets. To date, the processes of their deuteration are still poorly understood, only the upper limits of isotopic ratios for D/H and 13 C/ 12 C in linear alkanes are currently available. Aims. The aim of this work is to carry out a detailed analysis of the D/H ratio in water as a function of cometary activity and spacecraft location above the nucleus. In addition, a first determination of the D/H and 13 C/ 12 C ratios in the first four linear alkanes, namely, methane (CH 4 ), ethane (C 2 H 6 ), propane (C 3 H 8 ), and butane (C 4 H 10 ) in the coma of 67P/Churyumov-Gerasimenko is provided. Methods. We analysed in situ measurements from the Rosetta/ROSINA Double Focusing Mass Spectrometer (DFMS). Results. The D/H ratio from HDO/H 2 O and the 16 O/ 17 O ratio from H 2 16 O/H 2 17 O did not change during 67P’s passage around the Sun between 2014 and 2016. All D/H ratio measurements were compatible within 1 σ , with the mean value of 5.01 × 10 −4 and its relative variation of 2.0%. This suggests that the D/H ratio in 67P’s coma is independent of heliocentric distance, level of cometary activity, or spacecraft location with respect to the nucleus. Additionally, the 16 O/ 17 O ratio could be determined with a higher accuracy than previously possible, yielding a value of 2347 with a relative variation of 2.3%. For the alkanes, the D/H ratio is between 4.1 and 4.8 times higher than in H 2 O, while the 13 C/ 12 C ratio is compatible, within the uncertainties, with the available data for other Solar System objects. The relatively high D/H ratio in alkanes is in line with results for other cometary organic molecules and it suggests that these organics may be inherited from the presolar molecular cloud from which the Solar System formed.
    Type of Medium: Online Resource
    ISSN: 0004-6361 , 1432-0746
    RVK:
    RVK:
    Language: English
    Publisher: EDP Sciences
    Publication Date: 2022
    detail.hit.zdb_id: 1458466-9
    SSG: 16,12
    Location Call Number Limitation Availability
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  • 2
    In: Astronomy & Astrophysics, EDP Sciences, Vol. 647 ( 2021-3), p. A22-
    Abstract: The cyano radical (CN) is one of the most frequently remotely observed species in space, and is also often observed in comets. Data for the inner coma of comet 67P/Churyumov-Gerasimenko collected by the high-resolution Double Focusing Mass Spectrometer (DFMS) on board the Rosetta orbiter revealed an unexpected chemical complexity, and, recently, also more CN than expected from photodissociation of its most likely parent, hydrogen cyanide (HCN). Here, we derive abundances relative to HCN of three cometary nitriles (including structural isomers) from DFMS data. Mass spectrometry of complex mixtures does not always allow isolation of structural isomers, and therefore in our analysis we assume the most stable and abundant (in similar environments) structure, that is HCN for CHN, CH 3 CN for C 2 H 3 N, HC 3 N for C 3 HN, and NCCN for C 2 N 2 . For cyanoacetylene (HC 3 N) and acetonitrile (CH 3 CN), the complete mission time-line was evaluated, while cyanogen (NCCN) was often below the detection limit. By carefully selecting periods where cyanogen was above the detection limit, we were able to follow the abundance ratio between NCCN and HCN from 3.16 au inbound to 3.42 au outbound. These are the first measurements of NCCN in a comet. We find that neither NCCN nor either of the other two nitriles is sufficiently abundant to be a relevant alternative parent to CN.
    Type of Medium: Online Resource
    ISSN: 0004-6361 , 1432-0746
    RVK:
    RVK:
    Language: English
    Publisher: EDP Sciences
    Publication Date: 2021
    detail.hit.zdb_id: 1458466-9
    SSG: 16,12
    Location Call Number Limitation Availability
    BibTip Others were also interested in ...
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