
Official website (https://www.geo600.org/)
GEO600
Sign in to saveGEO600 is a gravitational wave detector located near Sarstedt, a town to the south of Hanover, Germany. It is designed and operated by scientists from the Max Planck Institute for Gravitational Physics, Max Planck Institute of Quantum Optics and the Leibniz Universität Hannover, along with University of Glasgow, University of Birmingham and Cardiff University in the United Kingdom, and is funded by the Max Planck Society and the Science and Technology Facilities Council (STFC).
Official website

Home | GEO600 Gravitational-wave Detector
GEO600 is a key technology development center of the international gravitational-wave research community.
geo600.org →Link to the official site · 3,512 chars · not written by Vinony
Wikidata facts
- Diameter
- 600
- Official website
- www.geo600.org
- Image
- 2015 GEO 600.jpg
Show 4 more facts
- Commons category
- GEO600
- maximum wavelength of sensitivity
- 10000
- minimum wavelength of sensitivity
- 43
- inception
- 1995-00-00
Sources (1)
via Wikidata · CC0
~12 min read
Article
12 sectionsContents
- History
- Hardware
- Suspensions and seismic isolation
- Optics
- Advanced
- Sensitivity and measurements
- Joint science run with LIGO
- Claims on holographic properties of spacetime
- Data and Einstein@home
- See also
- References
- External links
GEO600 is a gravitational wave detector located near Sarstedt, a town to the south of Hanover, Germany. It is designed and operated by scientists from the Max Planck Institute for Gravitational Physics, Max Planck Institute of Quantum Optics and the Leibniz Universität Hannover, along with University of Glasgow, University of Birmingham and Cardiff University in the United Kingdom, and is funded by the Max Planck Society and the Science and Technology Facilities Council (STFC).
GEO600 is capable of detecting gravitational waves in the frequency range 50 Hz to 1.5 kHz, and is part of a worldwide network of gravitational wave detectors. This instrument, and its sister interferometric detectors, when operational, are some of the most sensitive gravitational wave detectors ever designed. They are designed to detect relative changes in distance of the order of 10−21, about the size of a single atom compared to the distance from the Sun to the Earth. Construction on the project began in 1995.