NASA's Europa Clipper mission is designed to provide a diversity of measurements to further our understanding of the potential habitability of this intriguing ocean world. The Europa mission's Ultraviolet Spectrograph (Europa-UVS), built at the Southwest Research Institute (SwRI), is primarily a "plume finder" and tenuous atmosphere investigation. The science objectives of Europa-UVS are to: 1) Search for and characterize any current activity, notably plumes; and 2) Characterize the composition and sources of volatiles to identify the signatures of non-ice materials, including organic compounds, in the atmosphere and local space environment. Europa-UVS observes photons in the 55-206 nm wavelength range at moderate spectral and spatial resolution along a 7.5 degrees slit composed of 7.3 degrees x0.1 degrees and 0.2 degrees x0.2 degrees contiguous sections. A variety of observational techniques including nadir pushbroom imaging, disk scans, stellar and solar occultations, Jupiter transit observations, and neutral cloud/plasma torus stares are employed to perform a comprehensive study of Europa's atmosphere, plumes, surface, and local space environment. This paper describes the Europa-UVS investigation's science plans, instrument details, concept of operations, and data formats in the context of the Europa Clipper mission's primary habitability assessment goals.