Herschel Follows The Trail Of Cosmic Water
Herschel’s HIFI instrument was especially designed to follow the water trail in the Universe over a wide range of scales, from the Solar System out to extragalactic sources. Early results, presented this week at the Herschel First Results Symposium, demonstrate how HIFI uses water to probe the physical and chemical conditions in different regions of the cosmos.
Water is an extremely important molecule in the Universe, abundant in a large variety of cosmic environments “” from our own blue planet and its neighborhood, the Solar System, through interstellar clouds where new stars and planets are formed, and even beyond the Milky Way, in star-forming galaxies. Due to the large amount of water vapor present in the Earth’s atmosphere, however, astronomical observations of water from ground-based facilities are virtually impossible, even from the driest and highest deserts; they need to be carried out with space observatories.
The presence of water in a celestial object is revealed through its very distinctive fingerprints, or lines, in the object’s spectrum at far-infrared and sub-millimeter wavelengths. Only high resolution spectrographs, such as HIFI on board ESA’s Herschel Space Observatory, are able to obtain spectra sufficiently precise to track down the abundance of water in great detail.
HIFI, or the Heterodyne Instrument for the Far Infrared, was designed with the quest of water and other molecules very much in mind. Based on the heterodyne detection principle, it basically translates, without loss of information, the high-frequency signal received from astronomical sources to a lower frequency, where measurements are easier to perform. “With its superb spectral resolution, HIFI is ideally suited to detect and characterize molecular lines, and is currently performing a chemical census of the cosmos,” says Göran Pilbratt, Herschel Project Scientist.
“Water is an excellent diagnostic tool to probe the chemical and physical structure of the interstellar medium,” explains Alexander Tielens from Leiden University. “Early detection of this important molecule on all cosmic scales highlights that HIFI is working extremely well.”
With its superb resolution, HIFI can target about 40 different lines, each coming from a different transition of the water molecule and thus sensitive to a different temperature. This plethora of water lines in the spectra is anything but redundant information: it actually helps to overcome one of the natural drawbacks of astronomical observations, which yield two-dimensional images due to the projection on the celestial vault. As each line comes from a slightly different area in the interstellar clouds, putting all the information together gives a three-dimensional view of them. “HIFI data represent a sort of MRI scan through these regions, examining them slice-by-slice in a tomographic approach,” explains Frank Helmich, Principal Investigator for Herschel-HIFI.
The role of water is crucial in the processes of star formation, because this molecule contributes to the cooling of the gas and dust mixture from which stars are born. Early results, reported this week at the Herschel First Results Symposium, demonstrate the detection of water in various proto-stellar systems. Along with upcoming data from star-forming clouds throughout the Milky Way, these data will help astronomers understand the mechanisms of star formation in great detail. Beyond our Galaxy, water signatures have been found in nearby galaxies which are known to be undergoing intense bursts of star formation.
Water trails go all the way from vast star-forming clouds down to stars and planets on much smaller scales. In the proto-planetary discs surrounding stars in the process of forming, water vapor may in fact freeze onto dust grains; these cold grains would then condense into icy planetesimals, the seeds of planet formation.
“In our very own planetary system, HIFI has observed a handful of comets, which are dusty conglomerates held together by icy water,” notes Tielens. These cosmic ‘ice balls’ are living fossils in the Solar System, since they spend most of their lifetime at its boundaries and their chemical composition closely reflects the pristine conditions when the planets were formed about 4.5 billion years ago. “Further analysis of these early data collected by HIFI will shed new light on the early history of the Solar System,” Tielens adds.
Image 1: This HIFI spectrum shows water lines toward low-mass protostars in the NGC 1333 star-forming region. IRAS-2A, -4A and -4B refer to different members of the NGC 1333 cluster. The spectrum is superimposed on a Spitzer image of the region. Details of the study from which the spectrum is taken can be found in the paper of Kristensen et al., (in preparation) to appear in a special issue of Astronomy & Astrophysics dedicated to first scientific results from HIFI. Credits: ESA and the HIFI consortium; L.E. Kristensen for the WISH Key Program. Background image: NASA/JPL-Caltech/R. Gutermuth (Harvard-Smithsonian CfA)
Image 2: This HIFI spectrum shows water lines toward an intermediate-mass protostar in the NGC 7129 region. The spectrum is superimposed on a Spitzer image of the region. Details of the study from which the spectrum is taken can be found in the paper of Johnstone et al., (in preparation) to appear in a special issue of Astronomy & Astrophysics dedicated to first scientific results from HIFI. Credits: ESA and the HIFI consortium; D. Johnstone for the WISH Key Program. Background image: NASA/JPL-Caltech/S.T. Megeath (Harvard-Smithsonian CfA)
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