Names | COSI SMEX-17 |
---|---|
Mission type | Gamma-ray astronomy |
Operator | University of California, Berkeley NASA |
Website | https://cosi.ssl.berkeley.edu/ |
Spacecraft properties | |
Spacecraft | COSI |
Payload mass | < 400 kg |
Start of mission | |
Launch date | August 2027 (planned)[1] |
Rocket | Falcon 9[1] |
Launch site | Cape Canaveral Space Force Station[1] |
Contractor | SpaceX[1] |
Orbital parameters | |
Reference system | Geocentric orbit |
Regime | Low Earth orbit |
Main Germanium detectors | |
Name | Compton telescope |
Collecting area | 25% field of view of the sky |
Transponders | |
Band | Gamma Rays |
Bandwidth | 0.2–5 MeV |
Logo of COSI with all the participating institutions. |
The Compton Spectrometer and Imager (COSI) is a NASA SMEX astrophysics mission that will launch a soft gamma-ray telescope (0.2–5 MeV) in 2027.[2][3] It is a wide-field compact Compton telescope (CCT) that is uniquely suited to investigate the "MeV gap" (0.1–10 MeV).[4] It provides imaging, spectroscopy, and polarimetry of astrophysical sources, and its germanium detectors provide excellent energy resolution for emission line measurements.[5]
The germanium detectors have an instantaneous field of view of more than 25% of the sky, and they are surrounded on the sides and bottom by active shields, which provide background rejection while also allowing for detection of gamma-ray bursts and other gamma-ray flares across the majority of the sky.[5]
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