Gravitational Wave High-energy Electromagnetic Counterpart All-sky Monitor
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]
References
- v
- t
- e
- Double Star (joint with ESA)
- Fengyun
- Gaofen
- FSW
- Huanjing
- HY
- Jilin
- Shiyan
- SMMS
- TanSat
- Tansuo
- Tianhui
- Yaogan
- Ziyuan
- Dong Fang Hong
- FH-1
- Apstar
- APMT
- Asiasat
- ChinaSat
- ChinaStar
- HKSTG
- LGSP
- OlympicSat
- Shijian
- Sinosat
- Tiantong 1
- Tsinghua-1
- Xiwang 1
- Queqiao and Queqiao 2
- Tiandu 1 and 2
- Tianlian Constellation
- ASO-S
- CHASE
- DAMPE
- GECAM
- HXMT
- Kuafu
- Longjiang-2
- Queqiao
- Einstein Probe (joint with ESA)
- SST
- SVOM
- Xuntian
- SMILE
- Fengniao
- Xinyan
This spacecraft or satellite related article is a stub. You can help Wikipedia by expanding it. |
- v
- t
- e