We use the Hipparcos colour-magnitude diagram of field stars with Tych
o colours to make a new minimum age estimate for the Galactic disc. Th
e method is based on fits to the red envelope of subgiants in the Hipp
arcos colour-magnitude diagram with synthetic isochrones covering the
range of disc metal abundance. The colours and luminosities of the iso
chrones as a function of abundance are checked using new techniques in
volving 'red-clump' stars in the giant branch region and on the main s
equence using G and K dwarfs. We derive a minimum disc age of 8 Gyr, i
n good agreement with other methods.