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Herschel: revolutionising space telescopes
Launched by Ariane 5 in May 2009, the European Space Agency’s Herschel Space Observatory (formerly called Far InfraRed and Submillimetre Telescope or FIRST) is the first of a new generation of space telescopes – bigger than any of its predecessors at approximately seven and a half metres high and four metres wide and weighing around three tons, it is the first space observatory covering the full far-infrared and sub-millimetre waveband, and the largest to work at those wavelengths. It is located 1.5 million kilometres away from Earth, around the second Lagrangian point, farther than any previous space telescope.

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

SiC is an exceptional material whose mechanical-thermal properties allow the manufacture of ultra lightweight but very large instruments: the Astrium mirror, at 3.5m, is the largest imaging telescope ever launched, and yet the Herschel telescope weighs just 350kg, as opposed to the 1.5 tons which would be required with standard technology.

Under a second contract, Astrium was responsible for the fully integrated payload module that consisted of the:

  • cryostat
  • optical bench
  • scientific instrument harness
  • solar array & sun shade (supplied by Astrium subsidiary Dutch Space)
  • telescope & SVM interface structure, and performance of the satellite assembly, integration & test (AIT) programme.

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

The cryostat is the central unit of the payload module and was 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.

 

Did you know ?
Lagrange point
From its orbit around the Lagrange point L2 (situated around 1.5 million km from the Earth in the opposite direction to the sun), it takes about 10 seconds for Herschel to communicate with Earth (two-way).

A Lagrange point or libration point is a position in space where the gravitational fields of two massive bodies orbiting around each other, such as the Earth and the sun, combine in such a way as to create a point of balance for a third body of negligible mass, so that the relative positions of the three bodies are fixed. Lagrange points, therefore, are positions in space where a third body such as a satellite can remain fixed in relation to the two others. Space missions essentially use the L1 and L2 points:

SoHO (Solar and Heliospheric Observatory) has been positioned at the L1 point, 1.5 million km from Earth (between the Earth and the sun) since 1995

The L2 point, 1.5 million km from Earth on the opposite side from L1, is particularly well adapted for observing the cosmos. Planck Surveyor and Herschel, are positioned at the L2 point, as will the James Webb Space Telescope, slated for launch in 2013.

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