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The task of INTEGRAL will be to gather the most energetic radiation that comes from space. INTEGRAL will be the most sensitive gamma-ray observatory ever launched. It will detect radiation from the most violent events far away and from processes that made the universe habitable. |
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International Gamma-Ray Astrophysics Laboratory. |
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| Type | INTEGRAL big and heavy gamma ray observatory, three-axis stabilised. It is made up of two modules: the Service module provides the housekeeping equipment, i.e. power generation, conditioning and control, stabilisation and ground-satellite link, and the Payload Module carries the scientific instruments. The service module will be identical for the two ESA scientific missions, Integral and XMM | ||
| Mass | Total launch mass is more 4.1 tonnes including 2 tonnes of the scientific payload. | ||
| Size | The spacecraft size is 4x4x6 m (solar arrays undeployed) | ||
| Gamma-ray imaging | High angular resolution of 12 arcmin over an energy range between 15 keV and 10 MeV | ||
| Gamma-ray spectrometry | Perform spectral analysis of gamma-ray point sources and extended regions over an energy range between 20 keV and 8 MeV with energy resolution of 2 keV at 1 MeV | ||
| X-ray optics | Provide images in the energy range of 3 - 35 keV with an angular resolution of 3 arcmin | ||
| SPI | Spectrometer on INTEGRAL will perform spectral analysis of gamma-ray point sources and extended regions over an energy range between 20 keV and 8 MeV with an unprecedented energy resolution of 2 keV at 1 Me. Principal Investigators are Gilbert Vedrenne, CESR, Toulouse, France and Volker Schoenfelder, MPE, Garching, Germany | ||
| Jem-X | X-Ray Monitor will make observations simultaneously with the main gamma-ray instruments and will provide images in the energy range of 3 - 35 keV with an angular resolution of 3 arcmin. Principal Investigator Niels Lund, DSRI, Copenhagen, Denmark | ||
| IBIS | Gamma Ray Imager on Board the INTEGRAL Satellite will achieve a high angular resolution of 12 arcmin over an energy range between 15 keV and 10 MeV. Sources can be located to 1 arcmin. Pietro Ubertini, IAS, Frascati, Italy | ||
| OMC | optical camera on board of INTEGRAL offers the first opportunity to make long observations of the visible light coming from the gamma-ray and X-ray sources. Alvaro Gimenez, INTA, Madrid, Spain | ||
| Date | Baikonur Cosmodrome in the Republic of Kazakhstan, October 2002 | ||
| Vehicle | Russian Proton rocket | ||
| Eccentric 72-hour orbit around the Earth. 10 000 - 153 000 km altitude, 51.6° inclination. The spacecraft will spend most of its time above an altitude of 40 000 km outside Earth's radiation belts thus minimising background radiation effects. | |||
| Operational lifetime of 2 years with possible extension to up to 5 years, controlled by by the European Space Operations Centre (ESOC, Darmstadt Germany) using ground stations at ESA's Redu (Belgium) and NASA's Goldstone (USA). | |||