NASA Herschel Science Center's Portal to the Cool Universe
The Herschel Space Observatory's principal objectives are to help scientists study and understand:
With its unique ability to detect light in the full 60-670 micron range, Herschel will be able to gather information that has previously been unavailable.
Much of the universe is extremely cold, and shines only at far-infrared and submillimeter wavelengths beyond the reach not only of the human eye, but of most telescopes to date.
Most wavelengths in that range are readily absorbed by moisture in Earth's atmosphere, and so are inaccessible to earthbound telescopes. No previous space-based telescope was designed to detect the full range of light frequencies in that portion of the spectrum.
Herschel's large mirror and new generation of detector instruments will enable it to unveil new information about how galaxies first came into being; the symbiotic relationships among galaxies, stars, and the interstellar medium; the origins and evolution of chemicals; the mechanisms by which dense molecular clouds begin to collapse into stars; the engines behind the powerhouses at galactic cores; and the origins of planetary systems, including our own.
And much of this knowledge about the cosmos will come from observing dust and water.
Vast, cold clouds of smokelike dust and gas lie between us and many of the objects we'd most like to observe, like the early stages of star formation and the hearts of galaxies. And these clouds have a real penchant for infrared light.
They allow only infrared and longer wavelengths of light to pass through them. Visible light from stars and other luminous sources behind them is absorbed and reradiated at far-infrared and submillimeter wavelengths. And the dust and gas themselves radiate in that same range of long wavelengths.
But Herschel will enable scientists to measure the dust's temperature, analyze its composition, calculate its density, determine its motion - and deduce information about what lies around and behind it, whether it's the birth of a new star or the formation of a primordial galaxy.
Water, too, radiates in the far-infrared and submillimeter wavelengths that Herschel is designed to detect. And water has two features that make it very valuable to astronomers: it appears to be fairly commonplace in the cosmos, and its spectral signature can be interpreted to provide information about its environment.
By analyzing the emission and absorption lines in spectrographs of water, which vary in distinctive ways with density and temperature, scientists will be able to deduce information about interstellar clouds and other environments in which they detect water.
Herschel is expected to obtain a complete inventory of water in its various manifestations in space.
One of Herschel's prime objectives is to study the "Dark Age" of the universe, when the first galaxies began to form. Light from this early epoch has traveled for as much as 8.5 billion years before reaching us, and has been redshifted into Herschel's range by the expansion of the universe.
Herschel's ultra-high resolution spectrometer, HIFI, is uniquely suited to identify the chemical composition of the interstellar medium and the atmospheres of comets and planets in our solar system. It will help scientists understand the chemical history of the Galaxy and our solar system.
The universe reveals different things by the light of different wavelengths. Herschel will have the opportunity to see things in the far-infrared and submillimeter portions of the spectrum that have never been seen before.
Herschel's final objective is to achieve its discovery potential. The unexpected may be the most important finding of all.