  We report new photometry for the cluster NGC 2121 in the Large Magellanic
Cloud, which shows a prominent hydrogen core exhaustion gap at the turnoff, and
a descending subgiant branch remniscent of Galactic open clusters. We achieve
an excellent fit using the Girardi isochrones, finding an age of 3.2 +/-
0.5Gyr, with [Fe/H]=-0.6 +/- 0.2. The isochrones fit the color and shape of the
turnoff and subgiant branch so precisely that we constrain the metallicity as
well as the age. The smae isochrones also fit SL 663 and NGC 2155, although our
photometry for these clusters has much larger errors. We find these clusters to
be 0.8 Gyr younger, and 0.4 dex more metal rich, than recently reported in the
literature. Consequently, we argue that NGC 2121, NGC 2155, and SL 663 are not
properly assigned to the age gap in the LMC, but instead are among the first
clusters to have formed int he relatively metal rich, younger group of LMC
clusters. We propose a new definition of the LMC Age Gap as extending from 3.2
to 13 Gyr, with ESO121-SCO3 still the only remaining candidate for membership
in the age gap.
