Integral in brief Integral overviewIntegral factsheetA truly international missionAbout Integral The spacecraft The launcherThe launch site - BaikonurThe journey Integral's mission Multimedia Image galleryPre-launch images, Sept 2002Pre-launch images, October 2002Video gallery3D Flash 'model'Make a model
|  | | | | | | | | SPI will gauge gamma-ray energies with exceptional precision | |
The spacecraft
Standing 5 metres high and more than 4 tonnes in weight, the Integral spacecraft is impressive. The satellite has two main parts. The service module is the lower part of the satellite and contains all spacecraft subsystems. The payload module is mounted on the service module and carries the scientific instruments.
To limit the costs of the mission the service module is a rebuild of the one developed for XMM-Newton, ESA's X-ray Multi-Mirror satellite. It is a closed structure made of composite material, a combination of aluminium and carbon fibre. It houses the satellite systems, including solar power generation, power conditioning and control, data handling, telecommunications and thermal, attitude and orbit control.
| | The sharpest gamma-ray images to this day will come from IBIS | |
The four scientific instruments of Integral's payload module weigh 2 tonnes, making this payload the heaviest ever placed in orbit by ESA. This is due to the need to shield the detectors from background radiation in order to make them sensitive. There are two main instruments detecting gamma rays. An imager will give the sharpest gamma-ray images so far. A spectrometer will gauge gamma-ray energies extremely precisely. Two other instruments, an X-ray monitor and an optical camera, will help to identify the gamma-ray sources.
There is a special support structure 4 metres above the platform with the instrument detectors. This carries so-called 'coded masks'. These metal masks produce the images of the gamma-ray sources. Since gamma rays cannot be focussed by conventional lenses or mirrors, Integral has to use an entirely different technique to make its images, known as the coded mask technique. A coded-mask telescope is a pinhole camera with not just one but many pinholes.
Last update: 14 September 2004 | |
| | ESA's gamma-ray astronomy mission Observations: Seeing in the gamma-ray wavelengthsObservations: Seeing in X-ray wavelengthsRelated links Sci & Tech Integral pageIntegral Science Operations CentreIntegral Science Data CentreIntegral video  Integral spacecraft
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