Generated by DeepSeek V3.2| Herschel Space Observatory | |
|---|---|
| Name | Herschel Space Observatory |
| Caption | Artist's impression of the observatory in space |
| Mission type | Astronomy / Infrared astronomy |
| Operator | European Space Agency |
| Cospar id | 2009-026A |
| Satcat | 34937 |
| Website | http://sci.esa.int/herschel/ |
| Mission duration | Planned: 3 years, Final: 4 years, 1 month |
| Spacecraft | Herschel |
| Manufacturer | Thales Alenia Space |
| Launch mass | 3,400 kg (7,500 lb) |
| Dimensions | Height: 7.5 m (25 ft), Width: 4.0 m (13 ft) |
| Power | 1 kW |
| Launch date | 14 May 2009, 13:12 UTC |
| Launch rocket | Ariane 5 ECA |
| Launch site | Guiana Space Centre ELA-3 |
| Deployment date | 14 May 2009 |
| Entered service | June 2009 |
| Disposal type | Decommissioned |
| Deactivated | 29 April 2013 |
| Last contact | 17 June 2013 |
| Orbit regime | Lissajous orbit |
| Orbit reference | Sun–Earth L2 point |
| Orbit periapsis | 800,000 km (500,000 mi) |
| Orbit apoapsis | 1,200,000 km (750,000 mi) |
| Orbit period | 1 year |
| Orbit epoch | Planned |
| Telescope type | Ritchey–Chrétien telescope |
| Telescope diameter | 3.5 m (11 ft) |
| Telescope focal length | 28.5 m (94 ft) f/8.7 |
| Telescope wavelengths | 55–672 µm (Far-infrared / Submillimetre astronomy) |
| Instruments | HIFI – Heterodyne Instrument for the Far-Infrared, PACS – Photodetector Array Camera and Spectrometer, SPIRE – Spectral and Photometric Imaging Receiver |
| Insignia caption | Mission patch |
Herschel Space Observatory was a cornerstone mission of the European Space Agency designed to explore the cold and distant universe in the far-infrared and submillimetre wavelengths. It was the largest infrared telescope ever launched, featuring a 3.5-meter primary mirror, and operated from 2009 to 2013. Named after the pioneering astronomer William Herschel, who discovered infrared radiation, the observatory provided unprecedented data on the formation of stars and galaxies, as well as the molecular chemistry of the cosmos.
The observatory was a flagship mission within the ESA Science Programme, representing a major advancement in space-based astronomy. Its primary scientific goal was to study the formation and evolution of stars and galaxies in the early universe by observing in spectral ranges largely inaccessible from Earth. Operating at the Sun–Earth L2 Lagrange point, it offered a stable thermal environment crucial for its sensitive cryogenic instruments. The mission was part of a broader international effort in Infrared astronomy, complementing other major observatories like the Spitzer Space Telescope and the James Webb Space Telescope.
The development of the observatory, initially known as the Far Infrared and Submillimetre Telescope, was led by the European Space Agency with major contributions from NASA and instrument consortia across Europe and North America. The prime contractor for the spacecraft was Thales Alenia Space, with the telescope's silicon carbide mirror manufactured by French firm Sagem. After extensive testing at facilities like the European Space Research and Technology Centre, it was launched on 14 May 2009 aboard an Ariane 5 rocket from the Guiana Space Centre in French Guiana. The launch, which also carried the Planck spacecraft, successfully placed it on a trajectory to its operational orbit around the L2 point.
The observatory carried three sophisticated instruments housed in a superfluid liquid helium cryostat that cooled them to near absolute zero. The Heterodyne Instrument for the Far-Infrared was a high-resolution spectrometer built by a consortium led by the Netherlands Institute for Space Research, designed to study the chemistry of interstellar clouds. The Photodetector Array Camera and Spectrometer, developed under the leadership of the Max Planck Institute for Extraterrestrial Physics, provided imaging and spectroscopic capabilities in the shorter wavelength bands. The Spectral and Photometric Imaging Receiver, led by Cardiff University, served as a camera and spectrometer for the longest wavelengths, mapping extended cold dust emission.
Following launch, the spacecraft underwent a several-week journey to its operational orbit, a Lissajous orbit around the Sun–Earth L2 point, approximately 1.5 million kilometers from Earth. Mission control was conducted from the European Space Operations Centre in Darmstadt, with scientific data processed by the Herschel Science Centre at the European Space Astronomy Centre in Madrid. Routine science operations began in late 2009, with the mission's lifetime limited by its cryogenic helium supply. The helium was exhausted as predicted in April 2013, after which the observatory was placed into a permanent parking orbit around the Sun and decommissioned by the European Space Agency.
The observatory made transformative contributions to astrophysics, including detailed surveys of star-forming regions in the Milky Way like the Orion Nebula and the Galactic plane. It traced the distribution of cold dust and gas in nearby galaxies such as Andromeda and provided critical data on the role of water in the universe, detecting it in locations from comets to distant starburst galaxies. Its observations of ultra-luminous infrared galaxies in the distant universe helped constrain models of Galaxy formation and evolution. The vast public archive of data continues to fuel research, serving as a foundational resource for future missions like the James Webb Space Telescope and the Atacama Large Millimeter Array.
Category:Space telescopes Category:European Space Agency spacecraft Category:Infrared telescopes