We discuss the physical nature of a remarkably faint pair of Lyα-emitting images discovered close to the giant cD galaxy in the lensing cluster Abell 2218 ( z = 0.18) during a systematic survey for highly magnified star-forming galaxies beyond z = 5. A well-constrained mass model suggests the pair arises via a gravitationally lensed source viewed at high magnification. Keck spectroscopy confirms the lensing hypothesis and implies that the unlensed source is a very faint ( I ~ 30), compact (<150 h pc), and isolated object at z = 5.576 whose optical emission is substantially contained within the Lyα emission line; no stellar continuum is detectable. The available data suggest the source is a promising candidate for an isolated ~10 6 M ☉ system seen producing its first generation of stars close to the epoch of reionization.
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