Emission of large hydrocarbons from frozen CH4 by keV proton irradiation


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Ever since the first description of the synthesis of molecules by impinging protons on ices1, the possibility of formation of various molecules on cold surfaces by particle radiation has


been widely discussed2–5. Because fluxes of light ions with energies of ∼1 keV AMU−1 exist in a wide variety of astrophysical sites6 there has been a dispute over whether molecules in space


are formed by such a process or by gaseous reactions7. We have recently studied sputtering of species by bombarding simple frozen gases such as water, carbon monoxide and ammonia with light


ions2. With these substances, only rather simple molecules were found. However, when bombarding methane, we detected much larger molecules in the sputtered beam—hydrocarbons containing up to


at least 13 atoms. We propose, therefore, that bombardment of frozen methane by keV protons may produce large molecules in the Solar system.


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