Despite indications that classical cataclysmic variable (CV) stars are rare
in globular clusters in general, and in the cluster NGC 6624 in particular
, we have serendipitously discovered such a star similar to 6 " from the cl
uster center. A Hubble Space Telescope spectrum of the m similar to 22 obje
ct shows strong, broad emission lines typical of numerous field CVs, and th
e inferred optical and UV luminosity are also similar. Our accidental obser
vation also provides the first high-quality ultraviolet spectrum of a globu
lar cluster CV. That we have detected such an object in an observation that
includes just a few percent of the central area of the cluster may indicat
e that cluster CVs are more common than previously thought, at least near t
he core.