Recent evidence has shown that the mesospheric sodium nightglow, a chemilum
inescent process which produces atomic sodium D-line radiation in the Earth
's upper atmosphere, proceeds through the first excited (A (2)Sigma (+)) el
ectronic state of NaO. The rate of D-line radiation production is proportio
nal to the rate constant for the reaction of NaO(A (2)Sigma (+)) + O(P-3) a
nd its branching ratio to produce excited Na(P-2) rather than ground-state
Na(S-2). The only previously published measurement of the NaO + O(P-3) reac
tion rate and branching ratio was performed under slow flow conditions and
almost certainly primarily represents the reaction of ground state NaO (X (
2)Pi). We present low-pressure measurements of the NaO + O reaction kinetic
s using an NaO source reaction known to produce NaO in the (A (2)Sigma (+))
state and determine the 290 K reaction rate constant to be (5.1 +/- 1.8) x
10(-10) cm(3) s(-1) and the branching ratio to produce Na(P-2) to be 0.14
+/- 0.04. New data on the termolecular rate coefficient for the reaction Na
+ O-2 + He --> NaO2 + He at 290 K are also presented.