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| 3 December 2011 Integral is Europe's latest gamma ray observatory and continues the pioneering work begun in 1975 with ESA's Cos-B gamma ray satellite. Its acronym stands for the International Gamma ray Astrophysics Laboratory. Gamma rays are a million times more energetic than visible light and can pass through matter with hardly any interaction. Integral uses two specially designed gamma ray telescopes to register these elusive rays. One provides the sharpest images of the gamma ray sky ever seen and the other measures the energies of the gamma rays with unprecedented accuracy.
These telescopes are complemented by two other instruments: an X-ray monitor and an optical camera. All four instruments work simultaneously and point at the same region of the sky. This is the first time scientists have been routinely able to take measurements concurrently and it will allow a clearer identification of the gamma ray sources.
Scientific highlights to date
Cost The mission cost to ESA was 330 million Euros. This includes the spacecraft and the two years of ground operations but excludes the launch and the payload. The launch was provided by Russia in exchange for observing time. As is usual for ESA science missions, the payload was provided by national funds. Launch 17 October 2002, using a Russian Proton rocket from the Baikonour Cosmodrome in Kazakhstan. The Proton is Russia's largest operational launch vehicle. It is more than 57 metres tall and its mass at liftoff is around 700 tonnes. Orbit Integral was first placed in a low parking orbit around the Earth. About 50 minutes after launch, an attached upper stage rocket fired, putting Integral into a transfer orbit. The upper stage rocket then separated and Integral used its own manoeuvring rockets to reach its operational orbit of 72 hours. Its lowest point is 9000 kilometres and its highest point is 153 000 kilometres. Such an elongated orbit is essential to keep Integral as much as possible out of the Earth's harmful radiation belts, which distort the view of the high-energy Universe. Planned mission lifetime Integral is designed to have a mission lifetime of at least five years. At present, the mission is funded until end 2014 subject to 2012 mid-term review. Spacecraft Design Integral consists of two main sections: the service module and the payload module. The payload module contains the four scientific instruments and is joined to the service module, which houses essentials such as power distribution, communications and satellite control. To keep costs down, the service module design is the same as that used in XMM-Newton. The whole spacecraft is three-axis stabilised, allowing it to be pointed with a high degree of accuracy at its targeted celestial objects. Mass 4 tonnes at launch, including 2 tonnes of payload. Dimensions 5 x 3.7 x 3.7 metres. The deployed solar panels are 16 metres across. Industrial involvement The prime contractor is Alenia Spazio leading an industrial consortium involving 26 companies from 12 European countries and one company in the United States. Approximately 1400 people were involved in the production of Integral, including the scientists and engineers responsible for the instruments, ground segment, and science data centre. What's on board? Imager on Board the Integral Satellite - IBIS IBIS provides sharper gamma ray images than any previous gamma ray instrument. It can locate sources to a precision of 30 arcseconds, the equivalent of measuring a person standing in a crowd, 1.3 kilometres away. Principal Investigators: P. Ubertini (IAS/CNR Rome, Italy), F. Lebrun (CEA Saclay, France), G. Di Cocco (ITESRE Bologna, Italy). Spectrometer on Integral - SPI SPI measures the energy of incoming gamma rays with extraordinary accuracy. It is more sensitive to faint radiation than any previous gamma ray instrument and allows the precise nature of gamma ray sources to be determined. Principal Investigators: J.-P. Roques, (CESR Toulouse, France), V. Schönfelder (MPE Garching, Germany). Optical Monitoring Camera - OMC OMC automatically takes an image of the sky at optical wavelengths whenever the gamma ray telescopes are working. This allows astronomers to match the gamma ray source with an optical counterpart, thus permitting further investigation with ground-based optical telescopes. Principal Investigators: M. Mas-Hesse (INTA/LAEFF Madrid, Spain). Joint European X-Ray Monitor - JEM-X JEM-X performs a similar task to the OMC but at X-ray wavelengths. It provides X-ray images with similar positional accuracy as IBIS. These data allow astronomers to simultaneously study the behaviour of gamma ray sources at X-ray wavelengths. Previously, such investigations have never been routinely possible.
Principal Investigator: N. Lund (DSRI Copenhagen, Denmark).
Science operations
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