Herschel promises to bring in spectacular images from a variety of sources. Its mission qualifies four very different, very important fields: galaxy formation in the early universe, star formation and how it interacts with the interstellar medium, chemical composition of a variety of bodies within our own Solar System, and molecular chemistry in general anywhere in the universe where it can peer. Check out this page from Herschel's ESA site for more on the Herschel's key programmes.
To accomplish this, Herschel is outfitted with the largest mirror ever to be deployed in space, feeding into three different detectors. The first of these is the PACS, or Photodetecting Array Camera and Spectrometer, which will cover wavelengths from 55 to 210 micrometers. Next up is the SPIRE, or Spectral and Photometric Imaging Receiver, which covers 194 to 672 micrometers. Third and finally is the HIFI, Heterodyne Instrument for the Far Infrared, which will operate from the 157 to 212 and the 240 to 625 micrometers wavelength. Some of these wavelengths have never been observed before, bringing new depth to the field of infrared astronomy.
All of this is cooled by liquid helium—which dictates the length of Herschel's mission. Herschel is due to run out of this coolant in approximately four years, and due to its complex, hard-to-reach orbit, there will be no astronauts replacing that coolant anytime soon. The current Herschel observing mission is planned for three years. Maybe not the longest time for a telescope—but scientists are hoping to make the most of it.
For more information Herschel, from the latest news to the technical nitty gritty to the future home of its infrared photographs, check out ESA's Herschel homepage.