We report the detection of a strong jet-cloud interaction at a distanc
e of 120 kpc from the nucleus of the radio galaxy 3C 34, which has red
shift z = 0.69. Hubble Space Telescope images of the radio galaxy show
a long narrow region of blue emission orientated along the radio axis
and directed towards a radio hotspot. The William Herschel Telescope
has been used to provide long-slit spectroscopic data of this object,
and infrared observations made with the United Kingdom InfraRed Telesc
ope have enabled its spectral energy distribution to be modelled. We p
ropose that the aligned emission is associated with a region of massiv
e star formation, induced by the passage of the radio jet through a ga
laxy within the cluster surrounding 3C 34. A star formation rate of ab
out 100M. yr(-1) is required, similar to the values necessary to produ
ce the alignment effect in high-redshift radio galaxies. The consequen
ces of this result for models of star formation in distant radio galax
ies are discussed.