Models suggest BrHgONO
to be the major Hg(II) species formed in
the global oxidation of Hg(0), and BrHgONO undergoes rapid photolysis
to produce the thermally stable radical BrHgO•. We previously used quantum
chemistry to demonstrate that BrHgO• can, like •OH radicals, readily abstract hydrogen atoms from sp3-hybridized carbon atoms as well as add to NO and NO2. In the present work, we reveal that BrHgO• can
also add to C2H4 to form BrHgOCH2CH2
•, although this addition appears
to proceed with a lower rate constant than the analogous addition
of •OH to C2H4. Additionally,
BrHgO• can readily react with HCHO in two different
ways: either by addition to carbon or by abstraction of a hydrogen
atom. The minimum energy path for the BrHgO• + HCHO
reaction bifurcates, forming two prereactive complexes, each of which
passes over a separate transition state to form different products.
Rate constants computed using Master Equation simulations indicate
that hydrogen abstraction dominates over addition at atmospheric temperatures
(200 K ≤ T ≤ 333 K) and pressures (0.01
atm ≤ P ≤ 1 atm). Subsequently, we
compute the atmospheric fate of BrHgO• in a variety
of air masses and find that BrHgOH formation via hydrogen abstraction
will be the predominant fate (∼70–99%), with major competition
(∼20%) coming from addition to NO and NO2 in polluted
urban regions and stratospheric air. Given the absence of either field
data on the identity of Hg(II) compounds or experimental data on the
kinetics of BrHgO• reactions, the present manuscript
should provide guidance to a range of scientists studying atmospheric
mercury.