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In Development
Compton Spectrometer and Imager (COSI)
COSI would scan our Milky Way galaxy, measuring gamma rays from radioactive elements produced during stellar explosions to map the recent history of star death and element production. It would also measure polarization, to improve our understanding of how distant energetic cosmic explosions produce gamma rays.
Organization
Launch Date
November 2027
Class
Flight Project
Website
--
Key Staffs
- Science Team Member Carolyn Ann Kierans
- Science Team Member
- Principal Investigator
- Co Investigator Dr. Alan P Smale
- Co Investigator Terri J Brandt
COSI would scan our Milky Way galaxy, measuring gamma rays from radioactive elements produced during stellar explosions to map the recent history of star death and element production. It would also measure polarization, to improve our understanding of how distant energetic cosmic explosions produce gamma rays.
Related Publications
2023. "The Compton Spectrometer and Imager.", arXiv e-prints, arXiv:2308.12362 [10.48550/arXiv.2308.12362] [Journal Article/Letter]