International audienceContext. Detection of molecular oxygen and prediction of its abundance have long been a challenge for astronomers. The low abundances observed in few interstellar sources are well above the predictions of current astrochemical models. During the Rosetta mission, an unexpectedly high abundance of O2 was discovered in the comet 67P/Churyumov-Gerasimenko’s coma. A strong correlation between O2 and H2O productions is observed, whereas no such correlation is observed between O2 and either of CO or N2.Aims. We suggest that the O2 molecule may be formed during the evaporation of water ice. We propose a possible reaction: the dismutation of H2O2 (2 H2O2−→ 2 H2O + O2), a molecule which should be co-produced during the water ice...