Building SPARCS, an Ultraviolet Science CubeSat for Exoplanet Habitability Studies, Technology Advancements, and Mission Training
Evgenya L. Shkolnik, David R. Ardila, Logan Jensen, April D. Jewell, Tahina Ramiaramanantsoa, Judd Bowman, Daniel Jacobs, Paul Scowen, Christophe Basset, Johnathan Gamaunt, Dawn Gregory, Maria C. Ladwig, Matthew Kolopanis, Shouleh Nikzad, Nathaniel Struebel, Joe Llama

TL;DR
SPARCS is a CubeSat mission designed to monitor UV radiation from low-mass stars to study exoplanet habitability, test advanced UV detectors, and serve as a platform for technology development and training.
Contribution
The paper presents the design, technology advancements, and mission goals of SPARCS, a CubeSat dedicated to UV observations and technology testing for future space missions.
Findings
Successful development of delta-doped UV detectors with high efficiency
Mission readiness for launch in late 2025
Enhanced training and collaboration opportunities for students and researchers
Abstract
The Star-Planet Activity Research CubeSat (SPARCS) is a NASA-funded 6U-CubeSat mission designed to monitor ultraviolet (UV) radiation from low-mass stars. These stars' relatively high-frequency and high-energy UV flares significantly affect the atmospheres of orbiting exoplanets, driving atmospheric loss and altering the conditions for habitability. SPARCS aims to capture time-resolved photometric data in the far-UV and near-UV simultaneously to better characterize the flares and detect the strongest and rarest among them. In addition, SPARCS is testing innovative technology, such as delta-doped detectors with near 100% internal quantum efficiency and detector-integrated metaldielectric UV bandpass filters. This mission will increase the technology readiness level of these critical components, positioning them for inclusion in future flagship missions like the Habitable Worlds…
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