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SPARCS

From Wikipedia, the free encyclopedia

SPARCS (Star-Planet Activity Research CubeSat) is an American ultraviolet space nano-telescope in the CubeSat 6U format (30x20x10 cm at launch, 12 kg) whose objective is to study the near and far ultraviolet radiation of galactic red dwarfs.[1] The mission selected by NASA is developed and managed by Arizona State University with the participation of the Jet Propulsion Laboratory (JPL) which provides the telescope and its detectors.[2][3][4]

Objectives

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The objective of the SPARCS mission is to study the ultraviolet emissions of around ten red dwarfs in order to model its impact.[5] SPARCS is with ASTERIA one of the first space astronomy missions using the extremely miniaturized CubeSat format. This new category of satellite opens up prospects in the field of long-term observations of astronomical phenomena thanks to their reduced cost.[6][7]

Timeline

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SPARCS is expected to launch in 2027.[8]

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  • "Tiny satellite, big discoveries, from campus to cosmos - The Arizona State Press". www.statepress.com. Retrieved 2025-11-16.

References

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  1. ^ "SPARCS". sparcs.asu.edu. Retrieved 2021-12-18.
  2. ^ "ASU astronomers to build space telescope to explore nearby stars". EurekAlert!. Retrieved 2021-12-18.
  3. ^ Ardila, David R. (13 March 2023). "SPARCS: The Star-Planet Activity Research CubeSat" (PDF). JPL. Retrieved 12 September 2023.
  4. ^ "Home page | SPARCS". sparcs.asu.edu. Retrieved 2023-12-12.
  5. ^ University, Arizona State. "Astronomers to build space telescope to explore nearby stars". phys.org. Retrieved 2021-12-18.
  6. ^ "Onboard Dynamic Image Exposure Control for the Star-Planet Activity Research CubeSat (SPARCS)". www.spaceref.com. 22 November 2021. Retrieved 2021-12-18.[permanent dead link]
  7. ^ SPARCS: The Star-Planet Activity Research CubeSat
  8. ^ "TSIS-2 & Others". Retrieved 20 November 2025.