The rate constant k(O)(upsilon= 1) for NO(upsilon= 1) vibrational relaxatio
n by O has been measured at room temperature using a laser photolysis-laser
probe technique. Vibrationally excited NO and relaxer O atoms were formed
using 355 nm laser photolysis of a dilute mixture of NO2 in argon bath gas.
The time evolution of both the NO(upsilon= 1) and the O atoms was monitore
d using laser-induced fluorescence (LIF). The required absolute O-atom dens
ities were obtained through a comparison of O-atom LIF signals from the pho
tolysis source and from a titrated cw microwave source. At early times the
O atoms constitute the most important loss mechanism for the nascently prod
uced NO(upsilon= 1). Possible effects from NO(upsilon= 1) vibrational ladde
r-climbing and from thermal expansion have been shown to be minimal. The ra
te constant k(O)(upsilon= 1) = (2.4 +/- 0.5) X 10(-11) cm(3) s(-1) determin
ed herein is a factor of 2 to 3 lower than the generally accepted value of
k(O)(upsilon= 1) used in thermospheric modeling. The present value for k(O)
(upsilon= 1) is the same, within the error bars, as the k(O)(upsilon= 2,3)
previously measured in this laboratory using an entirely different techniqu
e, resonant infrared laser excitation of NO(upsilon= 0). This result sugges
ts that the collisional relaxation rates are independent of upsilon. A rece
nt quasiclassical trajectory calculation, in which both allowed NO-O surfac
es have been explicitly considered, predicts a collisional relaxation rate
which is in good agreement with the present result. The k(O)(upsilon= 1) va
lue, along with previously measured rate constants for NO-O high-pressure r
ecombination (k(rec)(infinity)) and isotope exchange (k(iso)), can serve as
a proxy for the rate coefficient k(C) describing the formation of a long-l
ived NO2* intermediate from O+NO collisions. The present value for k(O)(ups
ilon= 1) is significantly lower, however, than a recent determination of k(
rec)(infinity) and also the value of k(C) derived from k(iso). In the latte
r case the comparison is not as straightforward. (C) 1999 American Institut
e of Physics. [S0021-9606(99)00731-X].