Abstract
Context. Formamide (NH2CHO) has been proposed as a potential prebiotic precursor in the scientific discourse on the origin of life. It has been observed in different environments in space, including protostellar regions and comets. The abundance and stability of NH2CHO in the early stages of star formation can be better understood by incorporating the formation and destruction data in astrochemical models. Aims. We carried out an experimental investigation to study the destruction of pure NH2CHO ice at 12 K as a result of the interaction with Lyα (121.6 nm) photons. Methods. We studied UV photo destruction of NH2CHO using Fourier-transform infrared spectroscopy. Results. After UV processing, the intensity of NH2CHO IR bands decreased and new bands corresponding to HCN, CO, NH4+ OCN−, HNCO, and CO2 appeared in the spectrum. We then derived the destruction and cumulative product formation cross-sections. Conclusions. A comparison of destruction rates derived from the cross-section in a cold and dense molecular cloud for different energetic processing agents reveals that UV photons induce NH2CHO destruction at a level that is one order of magnitude greater than that affected by cosmic rays; however, it is three orders of magnitude lower than that of H atoms.
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