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• W2522691507 endingPage "156" @default.
• W2522691507 startingPage "156" @default.
• W2522691507 abstract "The participation of condensed nitrogen in the surface chemistry of some objects in the outer solar system, such as Pluto and Triton, is very important. The remote observation of this species using absorption spectroscopy is a difficult task because N2 is not IR active in the gas phase. Water is also among the most abundant molecules in the surface of these objects; chemical reactions between N2 and H2O induced by cosmic rays are therefore expected. Although pure N2 ice is hardly identified by IR spectroscopy, the species produced through the processing of the surface ice by cosmic rays may give relevant clues indicating how abundant the N2 is in the outside layers of the surface of trans-Neptunian objects (TNOs). The objective of this work is to investigate the formation of nitrogenated species induced by cosmic-ray analogs in an ice mixture containing nitrogen and water. Experiments were performed in the GANIL Laboratory by bombarding N2:H2O (10:1) ice at 15 K with 40 MeV 58Ni11+ ions. Evolution of precursor and daughter species was monitored by Fourier transform infrared spectrometry. The main produced species are the nitrogen oxides NOk (k = 1–3), N2Oj (j = 1–5), N3, and O3. Among them, the N2O and N3 are the most abundant, representing ∼61% of the total column density of the daughter molecules at 1013 ions cm−2 fluence; the current results indicate that the yield of daughter species from this mixture is low, and this may be one of the reasons why NiOj molecules are not usually observed in TNOs." @default.
• W2522691507 created "2016-09-30" @default.
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• W2522691507 date "2015-09-10" @default.
• W2522691507 modified "2023-10-16" @default.
• W2522691507 title "RADIOLYSIS OF NITROGEN AND WATER-ICE MIXTURE BY FAST IONS: IMPLICATIONS FOR KUIPER BELT OBJECTS" @default.
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• W2522691507 doi "https://doi.org/10.1088/0004-637x/810/2/156" @default.
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