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A Review of Requirements for Gamma Radiation Detection in Space Using CubeSats

Journal

APPLIED SCIENCES-BASEL
Volume 11, Issue 6, Pages -

Publisher

MDPI
DOI: 10.3390/app11062659

Keywords

X-ray and gamma ray detectors; particle detectors; detectors for astronomy; astrophysics; gravitational waves; silicon photomultipliers; electronic detector readout

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CubeSats provide a unique opportunity for quick and cost-effective access to space for scientific, educational, and commercial purposes. Their small size and low power consumption make them ideal for innovative satellite missions. Utilizing CubeSats for compact and efficient particle detection could be a game changer in astronomy and astroparticle physics.
Initially intended as student-led projects at universities and research institutions, the CubeSats now represent a unique opportunity to access space quickly and in a cost-effective fashion. CubeSats are standard and miniaturized satellites consisting of multiple identical units with dimensions of about 10x10x10cm3 and very limited power consumption (usually less than a few W). To date, several hundreds of CubeSats have been already launched targeting scientific, educational, technological, and commercial needs. Compact and highly efficient particle detectors suitable for payloads of miniaturized space missions can be a game changer for astronomy and astroparticle physics. For example, the origin of catastrophic astronomical events can be pinpointed with unprecedented resolution by measuring the gamma-ray coincidence signals in CubeSats flying in formations, and possibly used as early warning system for multi messenger searches. In this paper, we will discuss and analyze the main features of a CubeSat mission targeting intense and short bursts of gamma-rays.

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