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Chemical reactions in the nitrogen-acetone ice induced by cosmic ray analogs: relevance for the Solar System

Status Report From: arXiv.org e-Print archive
Posted: Thursday, December 21, 2017

A. L. F. de Barros, D. P. P. Andrade, E. F. da Silveira, K. F. Alcantara, P. Boduch, H. Rothard
(Submitted on 23 Nov 2017)

The radiolysis of a nitrogen-acetone mixture, condensed at 11 K, by 40 MeV 58Ni11+ ions is studied. These results are representative of studies concerning solar system objects exposed to cosmic rays. In the Kuiper Belt, region of Trans-Neptunian Objects (TNOs), acetone, molecular nitrogen and other small molecules were detected and may be present on icy surfaces. Bombardment by cosmic rays triggers chemical reactions leading to synthesis of larger molecules. In this work, destruction cross sections of acetone and nitrogen in solid phase are determined from a sequence of infrared spectra obtained at increasing ion beam fluence. The results are analyzed and compared with those of previous experiments performed with pure acetone. It is observed that the molecular nitrogen column density decrease very fast, suggesting that nitrogen quickly leaves a porous sample under irradiation. The behavior of acetone in the mixture confirms that the ice formed by deposition of vapor mixture is more porous than that of pure acetone ice. The most abundant molecular species formed from the mixture during irradiation are: C3H6, C2H6, N3, CO, CH4 and CO2. Some N-bearing species are also formed, but with low production yield. Comparing with pure acetone results, it is seen that dissolving acetone in nitrogen affects the formation cross sections of the new species: CH4, CO2 and H2CO, for example, have formation cross section smaller than the respective values for irradiated pure acetone, while those for CO and C2H6 species are higher. This fact can explain the presence of C2H6 even in regions on Pluto where CH4 is not pure, but diluted in a N2 matrix together with less abundant species. These results also show the formation of more complex molecules, such as HNCO, acetic acid and, possibility, glycine.

Comments:    16 pages, 9 figures, 5 tables
Subjects:    Earth and Planetary Astrophysics (astro-ph.EP)
Journal reference:    Monthly Notices of the Royal Astronomical Society, 2017, stx2751
DOI:    10.1093/mnras/stx2751
Cite as:    arXiv:1712.01829 [astro-ph.EP] (or arXiv:1712.01829v1 [astro-ph.EP] for this version)
Submission history
From: Diana Andrade P. P.
[v1] Thu, 23 Nov 2017 20:16:18 GMT (1940kb)
https://arxiv.org/abs/1712.01829
Astrobiology

Astrochemistry

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