A summary of the tests of 1 solar mass models is presented along with the comparison of globular cluster observed color-magnitude diagrams and the latest stellar models of VandenBerg. Using the distance scale set by nearby subdwarfs with trig parallax measures, the age of M92 is determined to be 15 +/- 2 Gyr. (gzipped postscript: text, 42kb; figure 1, 4kb; figure 2, 3kb; figure 3, 4kb; figure 4, 2kb;