The ages of the oldest stars in our Galaxy can be estimated by compari
ng stellar populations in globular clusters to calibrated stellar mode
ls. The best data give cluster ages of about 15.8 +/- 2.1 Gyr, which c
onflicts with the age of the Universe estimated from measurements of t
he Hubble constant and the 'standard' cosmological model of a flat, ma
tter-dominated universe (8-13 Gyr).