Gravitational Wave High-energy Electromagnetic Counterpart All-sky Monitor (GECAM) (Chinese: 引力波暴高能电磁对应体全天监测器) is a space observatory composed of a constellation of two X-ray and gamma-ray all-sky observing small satellites, called GECAM A (aka KX 08A or Xiaoji, COSPAR 2020-094A) and GECAM B (aka KX 08B or Xiaomu, COSPAR 2020-094B), for research in electromagnetic counterparts of gravitational waves (GWs). It was launched on 9 December 2020 from the Xichang Satellite Launch Center at 20:14 UTC by a Long March 11 rocket. GECAM will focus on detecting electromagnetic counterparts of gravitational waves. In addition to signals from GWs, the observatory studies Ultra-long GRBs, X-ray Flashes, X-ray-rich GRBs, Magnetars and Terrestrial Gamma-ray Flashes.[1][2][3]
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- Future missions marked in italics. Failed missions marked with † sign
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- Category:Space telescopes
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- ION-SCV 001 (Flock-4v × 12), ÑuSat 6, UPM-Sat 2, Flock-4v × 14, Lemur-2 × 8, NAPA-1, SpaceBEE × 12
- Starlink V1.0-L11 (60 satellites)
- Chinese reusable experimental spacecraft
- Gaofen 11-02
- Jilin-1 Gaofen-02C†
- Jilin-1 Gaofen-03B × 6, Jilin-1 Gaofen-03C × 3
- HaiYang 2C
- Huanjing 2A, Huanjing 2B
- Gonets-M × 3, ICEYE X6, ICEYE X7, Kepler 4, Kepler 5, LacunaSat-3, Lemur-2 × 4
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Launches are separated by dots ( • ), payloads by commas ( , ), multiple names for the same satellite by slashes ( / ). Crewed flights are underlined. Launch failures are marked with the † sign. Payloads deployed from other spacecraft are (enclosed in parentheses). |