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Herschel

Revolutionising space telescopes
Revolutionising space telescopes
© EADS Astrium

Launched in May 2009, the European Space Agency’s Herschel Space Observatory is the first of a new generation of space telescopes – bigger than any of its predecessors at approximately seven and a half metres high, four metres wide and weighing around three tons, it will be the first space observatory covering the full far-infrared and submillimetre waveband, and the largest to work at those wavelengths. It will be located 1.5 million kilometres away from Earth, around the second Lagrange point, farther than any previous space telescope.

Astrium’s ground-breaking developments in lightweight silicon-carbide technology are fundamental to the realistion of this programme; the company is responsible for the satellite’s all-silicon carbide (SiC) space telescope mirror, which will collect the light from distant and poorly known objects, such as newborn galaxies thousands of millions of light-years away.

SiC
© EADS Astrium/Patrick Dumas

SiC is an exceptional material whose mecathermal properties allow the manufacture of ultra lightweight but very large instruments: the Astrium mirror, at 3.5 m, will be the largest imaging telescope ever launched, weighing just 350 kg, as opposed to the 1.5 tons required with standard technology.

Under a second contract, Astrium is responsible for the fully integrated payload module, consisting of the cyostat, optical bench, scientific instrument harness, solar array and sun shield, telescope and SVM interface structure, and execution of the satellite assembly, integration and test (AIT) programme.

In order to prevent the instruments' own infrared radiation from drowning out the received signal, they must be cooled inside a cryogenic unit – the cryostat – down to minus 271 degrees Celsius (about two degrees above absolute zero). At this temperature the sensitive science instruments will have the potential to penetrate the unknown areas of the cold, early universe.

The cryostat is the central unit of the payload module and is being built under the leadership of Astrium. The low temperature is achieved using superfluid helium.

For the construction of cryostat, Astrium was able to draw on the experience it gained from Herschel's precursor, the European Infrared Space Observatory (ISO) which was successfully operated from 1996 to 1998.

In the course of the satellite AIT programme Astrium will demonstrate the spacecraft's flight readiness. One particular challenge is that while handling the spacecraft, the cryostat tank is filled with superfluid helium during the entire acceptance test campaign up to launch and flight.

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