The aims of gamma-ray astronomy were to establish both, the sources of
cosmic rays and the seats of nucleosynthesis. The 1950's could be cal
led the decade of predictions, when both roots came together and sourc
e strengths were predicted on the basis of radio-astronomical data and
expectations of steady state cosmology. The 1960's were the decade of
disappointment, because detectors employed then had too little sensit
ivity and too high background. The 1970's, the decade of discoveries w
ere opened with OSD III seeing the milky way in gamma-rays, followed b
y SAS 2, Cos-B, SMM and others. And the 1980's were the decade of prep
aration for the Compton gamma-Pay Observatory: by now, gamma-ray obser
vation have turned into a real astronomy and many of the original hope
s have been fulfilled.