  The Sirius AB binary system has masses that are well determined from many
decades of astrometric measurements. Because of the well-measured radius and
luminosity of Sirius A, we employed the TYCHO stellar evolution code to
determine the age of the Sirius A,B binary system accurately, at 225-250 Myr.
Note that this fit requires the assumption of solar abundance, and the use of
the new Asplund et al. primordial solar metallicity. No fit to Sirius A's
position is possible using the old Grevesse & Sauval scale. Because the Sirius
B white dwarf parameters have also been determined accurately from space
observations, the cooling age could be determined from recent calculations by
Fontaine et al. or Wood to be 124 +/- 10 Myr. The difference of the two ages
yields the nuclear lifetime and mass of the original primary star, 5.056
+0.374/-0.276 solar masses. This result yields in principle the most accurate
data point at relatively high masses for the initial-final mass relation.
However, the analysis relies on the assumption that the primordial abundance of
the Sirius stars was solar, based on membership in the Sirius supercluster. A
recent study suggests that its membership in the group is by no means certain.
