We studied the effects of 100 keV proton irradiation on films of ammonia-water mixtures between 20 and 120 K. Irradiation destroys ammonia, leading to the formation and trapping of H2, N2 NO, and N2O, the formation of cavities containing radiolytic gases, and ejection of molecules by sputtering. Using infrared spectroscopy, we show that at all temperatures the destruction of ammonia is substantial, but at higher temperatures (120 K), it is nearly complete (approximately 97% destroyed) after a fluence of 10(exp 16) ions per square centimeter. Using mass spectroscopy and microbalance gravimetry, we measure the sputtering yield of our sample and the main components of the sputtered flux. We find that the sputtering yield depends on fluence. At...
International audiencePhysico-chemical modifications induced by swift heavy ions on methane-water (C...
The transport and exchange of material between bodies in the outer solar system is often facilitated...
Deep inside dense molecular clouds and protostellar disks, interstellar ices are protected from stel...
We investigated chemical and physical processes in electron-irradiated ammonia-water ices at tempera...
We present new laboratory experiments investigating various water ice samples, ranging from thin ice...
We have conducted experiments on the sputtering of water ice by 100 keV Ar+ between 20 and 150 K. Ou...
We measured the total sputtering yield of amorphous water ice for 100 keV H+ as a function of the pr...
We present results of a range of experiments of sputtering of water ice together with a guide to the...
We performed quantitative laboratory radiolysis experiments on cubic water ice between 40 and 120 K,...
International audienceABSTRACT Water ices at 15 and 144 K were bombarded by swift heavy ions, 45.8 M...
International audienceContext. The nitrogen reservoir in planetary systems is a long-standing proble...
International audienceDeep inside dense molecular clouds and protostellar disks, interstellar ices a...
We elucidate mechanisms of electron-induced radiolysis in cosmic (interstellar, planetary, and comet...
International audiencePhysico-chemical modifications induced by swift heavy ions on methane-water (C...
The transport and exchange of material between bodies in the outer solar system is often facilitated...
Deep inside dense molecular clouds and protostellar disks, interstellar ices are protected from stel...
We investigated chemical and physical processes in electron-irradiated ammonia-water ices at tempera...
We present new laboratory experiments investigating various water ice samples, ranging from thin ice...
We have conducted experiments on the sputtering of water ice by 100 keV Ar+ between 20 and 150 K. Ou...
We measured the total sputtering yield of amorphous water ice for 100 keV H+ as a function of the pr...
We present results of a range of experiments of sputtering of water ice together with a guide to the...
We performed quantitative laboratory radiolysis experiments on cubic water ice between 40 and 120 K,...
International audienceABSTRACT Water ices at 15 and 144 K were bombarded by swift heavy ions, 45.8 M...
International audienceContext. The nitrogen reservoir in planetary systems is a long-standing proble...
International audienceDeep inside dense molecular clouds and protostellar disks, interstellar ices a...
We elucidate mechanisms of electron-induced radiolysis in cosmic (interstellar, planetary, and comet...
International audiencePhysico-chemical modifications induced by swift heavy ions on methane-water (C...
The transport and exchange of material between bodies in the outer solar system is often facilitated...
Deep inside dense molecular clouds and protostellar disks, interstellar ices are protected from stel...