The precision and CW characteristics of the new CEBAF electron accelerator will allow electromagnetic production of hypernuclear spectra with calculated resolutions between 200 and 300 keV. Experiments are planned to exploit this capability. The following paper reviews experimental considerations in the design of hypernuclear electroproduction, and provides estimates of expected rates and backgrounds. This hypernuclear program could begin in early 1996. Although hypernuclei have now been studied for a number of years, progress in the field has been slow because the experimental facilities available for these studies are not yet sufficient to answer some of the more important questions. Indeed, binding energies and decay properties of the light hypernuclei have not been significantly improved over the earlier nuclear emulsion and bubble chamber experi ments.0 However in the last decade, new counter techniques have been introduced, and new production mechanisms have been proposed and tested. Thus the promise of new physics now awaits new programs. There are a number of recent reviews on the status of hypernuclear physics. 2> Most of these reviews are connected, more or less, to the expectation that new accelerators or new experimental facilities will be introduced in the near future. Of particular relevance here, is the advent of the experimental program at the Continu ous Electron Beam Accelerator Facility, CEBAF, and the related reviews of hyperon electroproduction. 3> As there is no data on electroproduced hypernuclear spectra, and very little on the elementary process,4> P(r, K)A, these reviews concentrate on theoretically predicted spectra and their cross sections. While the calculations are useful in planning experimental programs, they may not completely reflect reality when the actual data become available. With this in mind, and without attempting to reproduce the existing reviews, this paper outlines an experimental view of the electroproduction of hypernuclei. The first section provides a short summary of the known elementary photoproduction process, particularly with respect to the impact of this data on the design of hypernu clear experiments. In later sections it discusses the expected results from a proposed set of measurements to be undertaken at CEBAF, and finally discusses the possibility