The COmpton Spectrometer and Imager (COSI) is an Astrophysics Small Explorer satellite mission that will probe the origins of our galaxy’s antimatter, uncover sites in our galaxy where complex atomic nuclei form, perform pioneering studies of gamma-ray polarization, and find counterparts to sources detected by means other than light, such as gravitational waves. COSI will employ a soft gamma-ray telescope using new technology to provide groundbreaking science.
The COSI satellite design is the result of extensive technology development that has been tested on scientific balloons over the past two decades. The latest flight was in 2016 aboard a NASA super pressure balloon, which is designed for long flights and heavy lifts.
COSI will help us advance our understanding of the creation and destruction of matter in the Milky Way and beyond. It operates at gamma-ray energies up to millions of times greater than visible light — between 0.2 and 5 million electron volts (MeV) — that uniquely probe astrophysical processes occurring among atomic nuclei, allowing us to directly see where new elements are being formed in our galaxy.
