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Integral operations
 
 
  The mission
 
Integral
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The task of Integral, ESA's International Gamma-Ray Astrophysics Laboratory, is to gather the most energetic radiation that comes from space. The spacecraft was launched October 2002 and will help to solve some of the biggest mysteries in astronomy. Gamma rays are even more powerful than the X-rays used in medical examinations. Fortunately, the Earth's atmosphere acts as a shield to protect us from this dangerous cosmic radiation. However this means that gamma rays from space can only be detected by satellites. Integral is currently the most sensitive gamma-ray observatory ever launched. It detects radiation from the most violent events far away and from processes that made the Universe habitable.

Credits: ESA. Illustration by D. Ducros
 
  The Flight Control Team
 
Integral Spacecraft Operations Manager (SOM) Richard Southworth
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Integral Spacecraft Operations Manager (SOM) Richard Southworth

Credits: ESA/J. Mai http://www.juergenmai.com
 
  Mission operations overview
 
Integral launch
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Integral launched at 06:41 CEST 17 October 2002 from Baikonur in Kazakhstan.

Credits: ESA - S.Corvaja
 
  The ground stations
Redu, Goldstone
 
Redu facilities
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The Redu site, which hosts multiple ground stations, is located in the Ardennes region of Belgium, about 1 km from the village of Redu which is in the Belgian province of Luxembourg. The stations provide tracking capabilities in VHF, C-band, L-band, S-band, Ku-band and Ka-band, and provide in-orbit tests (IOT) of telecommunication satellites. The S-band station is presently used for W3 (Eutelsat). The next ESA Science project to use the S-band station is Integral. The station co-ordinates, measured at the brass plate on the interferometer patch are 5.146231°E longitude, 50.002685°N latitude. This reference point is 378.3 m above sea level. The co-ordinates of the TMS-1 antenna are 5.14518047°E longitude, 50.00205516°N latitude. The antenna is sited at 385.583 m with respect to the WGS-84 reference ellipsoid [2]. The geostationary visibility above 10° elevation, is between 54.9°W and 65.1°E.

Credits: ESA - A. Van Der Geest
 
 
The Goldstone antenna in California - one of NASA's Deep Space Network antennae
 
  Ground segment & mission control system
 
SCOS-2000 MCS
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This mission uses SCOS-2000, the European standard mission control system developed at ESOC.

Credits: ESA
 
 
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The Integral mission and its interfaces with the Principal Investigators/Instrument Teams and the scientific community.

Credits: ESA
 
 
Integral instruments
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Integral will have two such detectors on board: an imager and a spectrometer. These instruments are supported by two monitor instruments: an X-ray monitor and an optical camera. All four instruments are co-aligned and will observe the same region of the sky simultaneously. This allows scientists to clearly identify gamma-ray sources, a key feature in studying high-energy processes in the violent Universe.

All instruments are provided by large collaborations encompassing many scientific institutes in the ESA member states, United States, Russia, Czech Republic and Poland. Principal investigators in different European countries lead the nationally funded collaborations.

Credits: ESA

 
  Last update: 15 March 2011 


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Related missions
XMM-Newton operations Related videoClick here
Related
Gamma rays (Wikipedia)
 
 
 
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