The small oxoacids of sulfur (SOS),
H
x
SO
y
(x, y = 1, 2), are considered to be key
reactive intermediates in organic
synthesis, biochemical processes, and atmospheric chemistry. They
play a major role in the chemistry of S-rich planets and are likely
present in the interstellar medium (ISM). To shed light on the processes
in the ISM, the reactions of SO2 and sulfur monoxide (SO)
with H atoms were studied at 3.1 K in a para-H2 quantum-solid host. In the case of SO, the formation of both
HOS and hydroxysulfinyl (HSO) was observed. Although hydroxidooxidosulfur
(HOSO) is more favored thermodynamically, HSO2 is more
readily formed from SO2 due to kinetic (tunneling) control.
Regarding the doubly hydrogenated species, sulfoxylic acid (S(OH)2), sulfinic acid (HS(O)OH), and tentatively dihydrogen sulfone
(H2SO2) were identified among the products by
IR spectroscopy. HOS and H2SO2 were observed
for the first time, while the present IR spectroscopic data can contribute
to the identification of SOS in the atmosphere of celestial bodies,
e.g., Venus, Europa, or Io.