The Laser Interferometer Space Antenna (LISA) will be the first
space-based gravitational wave observatory. LISA uses continuous-wave,
infrared laser beams propagating among three widely separated
spacecrafts to measure their distances with picometer accuracy via
time-delay interferometry. These measurements put very high demands on
the laser wavefront and are thus very sensitive to any deposits on
laser optics that could be induced by laser-induced molecular
contamination (LIMC). In this work, we describe the results of an
extensive experimental test campaign assessing LIMC related risks for
LISA. We find that the LIMC concern for LISA, even considering the
high demands on the laser wavefront, may be greatly reduced compared
to that observed at shorter wavelengths or with pulsed laser
radiation. This result is very promising for LISA as well as for other
space missions using continuous-wave, infrared laser radiation,
e.g., in free space laser communication or quantum key
distribution.