Production of Oxidants by Ion Bombardment of Icy Moons in the Outer Solar System

Table 1

Summary of the experiments discussed in this paper.

Target H2O : CO2	Thickness 10^17 mol/cm^2	T (K)	Ion (E in MeV)	Electronic stopping power eV/Å^−1	Max dose (eV/16 u)
1 : 0	2.4	16	He^+(0.2)	16	186
1 : 0	2.3	77	He^+(0.2)	16	23
1 : 0	2.0	16	H^+(0.2)	7	180
1 : 0	2.5	77	H^+(0.2)	7	40
1 : 0	34	12	^58Ni^11+(46)	490	30
1 : 0	33	13	^129Xe^23+(92)	849	23
1 : 0	14	13	^58Ni^13+(52)	492	13
10 : 1	6.9	13	^58Ni^13+(52)	466	5
5 : 1	7.0	16	He^+(0.2)	15.1	75
2.5 : 1	4.5	77	He^+(0.2)	14.5	23
1 : 1	9.9	13	^58Ni^13+(52)	398	11
1 : 1	3.0	16	He^+(0.2)	13.8	22
0 : 1	7.5	13	^58Ni^13+(52)	668	12