Herschel/SPIRE Infrared Astronomy Schools Ask an Astronomer Media
 
The Herschel Space Observatory - artist's impression.
©ESA
Herschel, an infrared space observatory, was launched on an Ariane 5 space rocket from French Guyana on May 14, 2009. After a few short weeks it reached its nominal orbit 1.5 million km away from the Earth, facing away from both Earth and Sun. From this vantage point Herschel will direct its giant telescope not only towards our own galaxy, the Milky Way, but also at very young galaxies in the far reaches of the universe.

Since Herschel’s useful life is limited to four years, infrared astronomers will be exceedingly busy during this time. The brief lifetime is due to the fact that Herschel consumes its liquid Helium to keep its science instruments cold. After the coolant runs out, Herschel's three instruments, which only function close to absolute zero temperatures (-273°C), will become useless.
Stars as seen through the Hubble Space Telescope.
©STSCI
  During its short but intense life Herschel will allow astronomers to see far-infrared and sub-millimeter light from stars, galaxies, and other matter in space, such as cold and dark material between stars. The primary focus of Herschel's mission will be to determine how stars and galaxies are born. Star formation occurs in our own galaxy (the Milky Way), and Herschel will closely examine regions where dust and gas is in the process of turning into a new star. Herschel will also look beyond our Milky Way Galaxy, much deeper into space and time, studying remote (very old) galaxies of our universe, providing information infrared astronomers require to determine how galaxies are born.

Herschel / SPIRE

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This website was made possible through funding from the Canadian Space Agency
 

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