In spite of the recent successes of SIGMA, RXTE and Compton GRO, and the la
unch of INTEGRAL in 2001, a lot of questions will stay opened for the next
decades in gamma-ray astronomy. In this context we have to think about futu
re instrument concepts which will allow a new step in the understanding of
high-energy phenomena at work in many exciting objects: binary systems with
compact objects, active galactic nuclei, supernovae and novae, gamma ray b
ursters .. A short overview of these new types of instruments will be given
.