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XMM-Newton is a 10.8-metre (35 ft) long space telescope, and is 16.16 m (53 ft) wide with solar arrays deployed. At launch it weighed 3,764 kilograms (8,298 lb). [ 2 ] The spacecraft has three degrees of stabilisation, which allow it to aim at a target with an accuracy of 0.25 to 1 arcseconds .
XMM-Newton: ESA: 10 Dec 1999 ... NASA: 2030: Highly elliptical orbit [232] Taiji: CNSA/CAS: 2033: Heliocentric orbit [233] Advanced Telescope for High Energy ...
The XMM Cluster Survey (XCS) is a serendipitous X-ray galaxy cluster survey being conducted using archival data taken by ESA’s XMM-Newton satellite. Galaxy clusters trace the large scale structure of the universe, and their number density evolution with redshift provides a way to measure cosmological parameters, independent of cosmic microwave background experiments or supernovae cosmology ...
Cornerstone 2 – XMM-Newton, launched December 1999, operational – An X-ray space telescope, studying the full range of cosmic X-ray sources. [ 4 ] [ 5 ] Cornerstone 3 – Rosetta , launched March 2004, completed – 67P/Churyumov–Gerasimenko orbiter mission, studying comets and their evolution.
GRB 221009A was subsequently observed by the Neutron Star Interior Composition Explorer (NICER), [14] the Monitor of All-sky X-ray Image (MAXI), the Imaging X-ray Polarimetry Explorer (IXPE), [30] [31] [8] the International Gamma-ray Astrophysics Laboratory (INTEGRAL), the XMM-Newton space telescope, [32] the Large High Altitude Air Shower ...
It is a mission of the Japan Aerospace Exploration Agency (JAXA) in partnership with NASA and ESA, intended to study galaxy clusters, outflows from galaxy nuclei, and dark matter. [5] [6] XRISM is a next generation X-ray astronomy spacecraft, succeeding the Chandra X-ray Observatory and XMM-Newton.
Four Great Observatories. NASA's series of Great Observatories satellites are four large, powerful space-based astronomical telescopes launched between 1990 and 2003. They were built with different technology to examine specific wavelength/energy regions of the electromagnetic spectrum: gamma rays, X-rays, visible and ultraviolet light, and infrared light.
Many space experiments have been tested at CSL, up from METEOSAT satellite Planck, through the instruments of Hipparcos and XMM / Newton. The facilities allow CSL and implement environmental testing in a space environment but also on mechanical testing machine for vibration required to certify the equipment during launches.