  We present Space-VLBI observations of the quasar 3C395 which show evidence of
the existence of a large bend in the inner parts of its jet, close to the core.
This bend would explain why previous Earth-based cm-VLBI observations could not
detect the ejection of new moving components, as expected from flux density
variability in this source. In general, the observational properties of the jet
in 3C395 are heavily marked by the existence of bends on different scales.
