We present the design of the Spectroscopic Ultraviolet Multi-object Observatory (SUMO) prototype and our plan to deploy this instrument on the INFUSE sounding rocket as an independent fly-along instrument. The SUMO prototype is part of the technology maturation program of SUMO - a mission concept designed for a future small satellite platform. SUMO is designed for astrophysics research in the Far-Ultraviolet (FUV) and Near-Ultraviolet (NUV) regimes encapsulating a wide range of programs, including efforts to understand the processes of star formation and galaxy evolution. Since the last major UV NASA missions, FUSE and GALEX, NASA has invested significantly into technology development for the UV bandpass. As a result, high reflectance mirror coatings and state-of-the-art detectors are now available. These technologies, along with the developed optical design, allow SUMO to achieve effective areas that are comparable to those achieved by FUSE and GALEX, at a fraction of the size and cost. The SUMO prototype consists of an 8 cm Cassegrain telescope and a Digital Micromirror Device (DMD)-based Multi-Object Spectrometer (MOS), with parallel imaging and spectroscopic channels. As part of this work, we are also developing a custom DMD controller, which is suitable for operation in the space environment. Given that current DMD-based spectrographs have been solely ground-based, this will be the first time a DMD-based instrument is deployed in space. Because the SUMO prototype will be deployed as a secondary payload, the spectrograph is also designed for completely autonomous operation. The SUMO prototype is tentatively scheduled for flight in 2025.
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