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|  |  |  |  | | | Is life the rule or the exception? The answer may be in the interstellar clouds 28 May 2002
 | In addition to forming in comets and asteroids, amino acids, the 'building blocks' of life, may form in dust grains in the space between the stars
Credits: ESA 2002. Illustration by Medialab |  |  |  |  |
| | | |  | | An artist's impression of the Rosetta spacecraft, its target Comet 67P/Churyumov-Gerasimenko, and the Philae lander being delivered onto its surface.
Rosetta’s 11-year expedition began in March 2004, with an Ariane 5 launch from Kourou in French Guiana, and the spacecraft was then sent towards the outer Solar System. The long journey includes three gravity assists at Earth (2004, 2007, 2009), one at Mars (2007), and two asteroid encounters: (2867) Steins (2008) and (21) Lutetia (2010).
Rosetta will reach Comet 67/P Churyumov-Gerasimenko in 2014, and will be the first mission ever to orbit a comet’s nucleus and to deliver a lander, called Philae, on its surface.
Credits: ESA |  |  |  |  |
| | | |  | Herschel is the only space facility dedicated to the submillimetre and far infrared part of the spectrum. Its vantage point in space provides several decisive advantages, including a low and stable background and full access to this part of the spectrum.
Herschel has the potential of discovering the earliest epoch proto-galaxies, revealing the cosmologically evolving AGN-starburst symbiosis, and unraveling the mechanisms involved in the formation of stars and planetary system bodies. The key science objectives emphasise specifically the formation of stars and galaxies, and the interrelation between the two, but also includes the physics of the interstellar medium, astrochemistry, and solar system studies.
Herschel will carry a 3.5 metre diameter passively cooled telescope. The science payload complement - two cameras/medium resolution spectrometers (PACS and SPIRE) and a very high resolution heterodyne spectrometer (HIFI) - will be housed in a superfluid helium cryostat.
Herschel will be placed in a transfer trajectory towards its operational orbit around the Earth-Sun L2 point by an Ariane 5 (shared with Planck) in early 2007. Once operational FIRST will offer a minimum of 3 years of routine observations; roughly 2/3 of the available observing time is open to the general astronomical community through a standard competitive proposal procedure. |  |  |  |  |
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|  | Related links ESA ScienceRosetta Home PageESA's Herschel homepage
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