<i>Herschel</i>Space Observatory
Abstract
<i>Herschel<i/> was launched on 14 May 2009, and is now an operational ESA space observatory offering unprecedented observational capabilities in the far-infrared and submillimetre spectral range 55–671 <i>μ<i/>m. <i>Herschel<i/> carries a 3.5 m diameter passively cooled Cassegrain telescope, which is the largest of its kind and utilises a novel silicon carbide technology. The science payload comprises three instruments: two direct detection cameras/medium resolution spectrometers, PACS and SPIRE, and a very high-resolution heterodyne spectrometer, HIFI, whose focal plane units are housed inside a superfluid helium cryostat. <i>Herschel<i/> is an observatory facility operated in partnership among ESA, the instrument consortia, and NASA. The mission lifetime is determined by the cryostat hold time. Nominally approximately 20 000 h will be available for astronomy, 32% is guaranteed time and the remainder is open to the worldwide general astronomical community through a standard competitive proposal procedure.
Funding
- National Aeronautics and Space Administration
- California Institute of Technology
- Imperial College London
- Cardiff University
- Centre National d’Etudes Spatiales
- Chalmers Tekniska Högskola
- Eidgenössische Technische Hochschule Zürich
- KU Leuven
- Centre National de la Recherche Scientifique
- Bundesministerium für Verkehr, Innovation und Technologie
- Stockholms Universitet
- Max-Planck-Institut für Astronomie
- Science and Technology Facilities Council
- National Astronomical Observatories, Chinese Academy of Sciences
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