ABSTRACT We examined the use of liquid-crystal (LC) technology to build an easily reconfigurable focal-plane slit system for multi-object spectroscopy (MOS). Several kinds of LC screens were analyzed in a spectrophotometer and at the focus of the spectrograph on the 24-inch telescope at Sommers-Bausch Observatory (SBO) on the CU Boulder campus. Depending on the crystal material used, transmission can be as high as > 80% in the clear state across the visible spectrum, and constrast ratios (ratio of clear- to opaque-state transmission) of >100:1 can be attained, but high contrast and high transmission are not both present in the same LCs. While significant difficulties exist in fabricating LCs as competitive MOS focal plane slits, there exist no fundamental obstacles to implementing this technology in an astronomical setting. The major problems for currently avaiable LCs include: 1. In order to obtain clear-state transmission of > 80% across one free spectral order, even the best contrast ratios currently available for a single screen ( 100:1) are not good enough for faint-object spectroscopy. 2. To use the LC types which yield high clear-state transmission, thin-film transistors (TFTs) must be used to address individual pixels. Currently, development costs for such devices are quite high, though remanufacture costs are low. Based on our tests, by stacking two screens of the best LCs currently available, an LC MOS slit assembly could be configured to give a clear-state transmission of 50-70% across the optical band with off-state opacities approaching 10 magnitudes in that same range. While these specifications are already competitive with other MOS schemes currently in use, the major drawback of an LC MOS at this time appears to be obtaining sufficient opacity between slits to obtain accurate sky subtraction.