  The James Webb Space Telescope (JWST) has the potential to enhance our
understanding of near-Earth objects (NEOs). We present results of
investigations into the observability of NEOs given the nominal observing
requirements of JWST on elongation (85-135 degrees) and non-sidereal rates
($<$30mas/s). We find that approximately 75% of NEOs can be observed in a given
year. However, observers will need to wait for appropriate observing windows.
We find that JWST can easily execute photometric observations of meter-sized
NEOs which will enhance our understanding of the small NEO population.
