  We discuss the future possibilities for extragalactic star cluster research
with the expected new ground-based and space-based telescopes and
instrumentation. Significant gains are expected due to improved angular
resolution, sensitivity, and area coverage particularly in the infrared and
radio, accompanied by progress in evolutionary and dynamical modelling.
Improvements in angular resolution are anticipated, especially through new
adaptive optics systems (e.g., Keck, Gemini, VLT), and interferometry (e.g.,
Keck, VLT, LBT, ALMA, SMA, SkA), and space instrumentation (e.g., Chandra,
NGST), enabling studies even of deeply embedded, forming extragalactic star
clusters. Tidal disruption of Galactic clusters becomes observable through
wide-area surveys such as the SDSS, VISTA, PRIME, including proper motion
measurements through high-resolution imaging (e.g., HST, LBT, SIM, GAIA).
Sensitive new optical and infrared spectrographs (e.g., HET, SALT, GranTeCan,
Magellan, Keck, VLT, CELT, OWL, NGST) will push kinematic and abundance studies
to new limits, allowing us detailed comparisons with model predictions. One
important wavelength range for the study of young, massive star clusters, the
far UV, appears to be neglected by future planned instrumentation.
