We report on the first space-VLBI observations of the OH 34.26+0.15 maser i
n two main-line OH transitions at 1665 and 1667 MHz. The observations invol
ved the space radio telescope on board the Japanese satellite HALCA and an
array of ground radio telescopes. The map of the maser region and images of
individual maser spots were produced with an angular resolution of 1 mas,
which is several times higher than the angular resolution available on the
ground. The maser spots were only partly resolved and a lower limit to the
brightness temperature 6 x 10(12) K was obtained. The maser seems to be loc
ated in the direction of low interstellar scattering, an order of magnitude
lower than the scattering of a nearby extragalactic source and pulsar.