In this paper we present a detailed experimental study of the evolutio
n of frozen butane (10 K) before, during and after irradiation with 3
keV He ion beams. Because of irradiation, different molecular species
are formed, among which a refractory organic material that, upon furth
er irradiation, evolves towards an amorphous carbon. The techniques us
ed for the analysis are ''in situ'' infrared (IR) and Raman spectrosco
py. The results may have relevance in astrophysics: the produced refra
ctory residues are in fact good analogs of the organic mantles on inte
rstellar grains and of the organics found in carbonaceous meteorites s
uch as Orgueil and Murchison.