A new aluminum-bearing species, OAlNO, which has the
potential
to impact the chemistry of the Earth’s upper atmosphere, is
characterized via high-level, ab initio, spectroscopic
methods. Meteor-ablated aluminum atoms are quickly oxidized to aluminum
oxide (AlO) in the mesosphere and lower thermosphere (MLT), where
a steady-state layer of AlO then builds up. Concurrent formation of
nitric oxide (NO) in the same region of the atmosphere will lead to
the bimolecular formation of the OAlNO molecule. Molecular orbital
analysis provides fundamental insights into the chemical bonding and
energetic arrangement of the triplet (1 3A″) ground
state and singlet (1 1A′) excited-state species
of OAlNO. Additionally, unpaired electrons on the terminal oxygen
atom of triplet (1 3A″) OAlNO cause it to be reactive
to atmospheric species, potentially impacting climate science and
high-altitude chemistry. The triplet (1 3A″) ground-state
species exhibits a large permanent dipole moment useful for rotational
spectroscopic detection; however, similar rotational constants to
the singlet (1 1A′) excited-state species will hamper
differentiation in a spectrum. Strong infrared intensities will assist
in detection and discrimination of the different spin states and isomers.
Repulsive electronic excited states of OAlNO will lead to photolysis
of the Al–N bond and formation of various electronic states
of AlO + NO through nonadiabatic pathways. Reaction through the OAlNO
intermediate represents a means for the production of electronically
excited AlO, leading to new chemistry in the atmosphere. Excitation
to higher-lying electronic states will lead to fluorescence with a
minor Stokes shift, useful for laboratory investigation. Such physical
properties of this molecule will allow for new, unexplored chemical
pathways in the MLT to be considered.