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Herschel Space Observatory
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The Herschel Space Observatory is a European Space Agency (ESA) mission originally proposed in 1982 by a consortium of European scientists that included Thijs de Graauw (Netherlands Institute for Space Research), Gisbert Winnewisser (University of Cologne), Michael Rowan-Robinson (Imperial College, London), Glenn White (Open University and The Rutherford Appleton Laboratory), and Malcolm Longair (University of Cambridge). Launch is currently targeted for 16 April 2009 from Kourou, French Guiana. The spacecraft was transported to French Guiana onboard an Antonov An-124 aircraft on 10 February 2009.
The satellite, built in the Cannes Mandelieu Space Center with a joint launch cost of €1.1 billion (1.7 billion), will be carried with the Planck satellite into space by an Ariane 5 ECA rocket.

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Encyclopedia
The Herschel Space Observatory is a European Space Agency (ESA) mission originally proposed in 1982 by a consortium of European scientists that included Thijs de Graauw (Netherlands Institute for Space Research), Gisbert Winnewisser (University of Cologne), Michael Rowan-Robinson (Imperial College, London), Glenn White (Open University and The Rutherford Appleton Laboratory), and Malcolm Longair (University of Cambridge). Launch is currently targeted for 16 April 2009 from Kourou, French Guiana. The spacecraft was transported to French Guiana onboard an Antonov An-124 aircraft on 10 February 2009.
The satellite, built in the Cannes Mandelieu Space Center with a joint launch cost of €1.1 billion (1.7 billion), will be carried with the Planck satellite into space by an Ariane 5 ECA rocket. It is then meant to enter a Lissajous orbit of 700,000 km diameter around the second Lagrangian point (L2) of the Earth-Sun system, 1.5 million kilometres distant from the Earth. The mission is named after Sir William Herschel, the discoverer of the infrared spectrum.
Instrumentation
The mission, formerly titled the Far Infrared and Sub-millimetre Telescope (FIRST), will be the first space observatory to cover the full far infrared and submillimetre waveband. At 3.5 meters wide, its telescope will incorporate the largest mirror ever deployed in space. The light will be focused onto three instruments with detectors kept at temperatures below 2 K. The instruments will be cooled with liquid helium, boiling away in a near vacuum at a temperature of approximately 1.4 K. The 2,000 litres of helium on board the satellite will limit its operational lifetime. The satellite is expected to be operational for at least 3 years.
Herschell will carry aboard three detectors:
PACS (Photodetecting Array Camera and Spectrometer): An imaging camera and low-resolution spectrometer covering 55 to 210 micrometres. The spectrometer will have a resolution between 1000 and 5000 and be able to detect signals as weak as a few times 10-18 W/m². The imaging camera will be able to image simultaneously in two bands (either 60-85/85-130 micrometres and 130-210 micrometres) with a detection limit of a few millijanskys.
SPIRE (Spectral and Photometric Imaging Receiver): An imaging camera and low-resolution spectrometer covering 194 to 672 micrometres. The spectrometer will have a resolution between 40 and 1000 at wavelengths of 250 micrometres and be able to image point sources with brightnesses around 100 millijanskys (mjy) and extended sources with brightnesses of around 500 mjy. The imaging camera has three bands, centered at 250, 350 and 500 micrometres, each with 139, 88 and 43 pixels respectively. It should be able to detect point sources with brightness above 2 mjy and between 4 and 9 mjy for extended sources.
HIFI (Heterodyne Instrument for the Far Infrared): A detector with a spectral resolution as high as 107. The spectrometer can be operated within two wavelength bands, from 157 to 212 micrometres and from 240 to 625 micrometres.
Science
Herschel will specialise in collecting light from objects in our Solar System as well as the Milky Way and even extragalactic objects billions of light-years away, such as newborn galaxies, and is charged with four primary areas of investigation:
- Galaxy formation in the early universe and the evolution of galaxies;
- Star formation and its interaction with the interstellar medium;
- Chemical composition of atmospheres and surfaces of Solar System bodies, including planets, comets and moons;
- Molecular chemistry across the universe.
See also
Further reading
External links
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