A&A 641, A154 (2020) Astronomy https://doi.org/10.1051/0004-6361/201935477 & © ESO 2020 Astrophysics Vacuum ultraviolet photoabsorption spectroscopy of space-related ices: 1 keV electron irradiation of nitrogen- and oxygen-rich ices S. Ioppolo1, Z. Kanuchovᡠ2, R. L. James3, A. Dawes3, N. C. Jones4, S. V. Hoffmann4, N. J. Mason5, and G. Strazzulla6 1 School of Electronic Engineering and Computer Science, Queen Mary University of London, Mile End Road, London E1 4NS, UK e-mail:
[email protected] 2 Astronomical Institute of Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia 3 School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK 4 ISA, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, Denmark 5 School of Physical Sciences, University of Kent, Park Wood Rd, Canterbury CT2 7NH, UK 6 INAF – Osservatorio Astrofisico di Catania, Via Santa Sofia 78, Catania 95123, Italy Received 15 March 2019 / Accepted 24 July 2020 ABSTRACT Context. Molecular oxygen, nitrogen, and ozone have been detected on some satellites of Saturn and Jupiter, as well as on comets. They are also expected to be present in ice-grain mantles within star-forming regions. The continuous energetic processing of icy objects in the Solar System induces physical and chemical changes within the ice. Laboratory experiments that simulate energetic processing (ions, photons, and electrons) of ices are therefore essential for interpreting and directing future astronomical observations. Aims. We provide vacuum ultraviolet (VUV) photoabsorption spectroscopic data of energetically processed nitrogen- and oxygen-rich ices that will help to identify absorption bands and/or spectral slopes observed on icy objects in the Solar System and on ice-grain mantles of the interstellar medium.