Europe is playing a key role in this global programme with three new instruments, including the €1 billion Herchel Space Observatory (HSO), and the European Science Foundation (ESF) has been helping to coordinate the effort by bringing many of the principle users of these facilities together at an international conference. Delegates included leading specialists in all aspects of galaxy and star formation.
Galaxies are formed when areas of dust and gas collapse under gravity, forming clumps within which densities become sufficient to trigger the nuclear fusion required for star formation. But the devil is in the detail, and this has been obscured from optical telescopes by clouds of dust that absorb visible light. However the dust re-emits this visible light absorbed from galaxies at longer wavelengths, and the latest telescopes are now able to detect this at sufficient sensitivity to unravel the processes being observed, as Eelco van Kampen, chair of the ESF Research Conference The Origin of Galaxies: Exploring Galaxy Evolution with the New Generation of Infrared-Millimeter Facilities, pointed out. “The main reason for a new golden age is the sheer number of new instruments that will become available over the next few years, literally opening up the universe in the far-infrared to millimeter wavelengths,” said van Kampen.
It is not just that galaxy formation can now be observed indirectly via the radiation emitted from the dust that obscures a direct view, but the new telescopes are also able to span a much broader spectrum of wavelengths. This is crucial for understanding what is happening, because many processes, and also individual chemical elements, only reveal themselves via the radiation they emit across multiple wavelengths, rather than their intensity at a particular point of the spectrum, or single “colour”. “The main gain is that the whole 'spectral energy distribution' (SED for short) can be mapped for each source, which means that one does not only measure total luminosity, but also 'colours' and emission from specific molecules,” said van Kampen. “From the SED one can derive many properties of the sources, including temperatures and composition.”
Although there is great confidence that dramatic progress will be made, there is uncertainty over the exact nature of the discoveries to come, creating eager anticipation among astronomers. “There will be many surprises, as this is still a relatively uncharted wavelength range,” said van Kampen. “It is hard to predict whether surprises will be on the same scale as those in gamma-rays, where many short-lived bursts appeared quite unexpectedly, but there is great potential for the unexpected!” Gamma ray bursts lasting a split second are caused by the most powerful explosions known, and provided evidence of black holes – objects whose gravity is so intense that even light does not travel fast enough to escape.
For European researchers, there is an additional aspect to the challenge – all the observations from the crucial HSO telescope have to be made within about three years before the equipment runs out of its vital helium cooling fluid, which cannot practically be replenished. The telescope has to be kept cool to avoid emitting infra red radiation from its own fabric, which would swamp the faint signals from distant dust clouds. “The Herschel Space Telescope has to be cooled significantly to reduce background noise, and for this purpose will be housed in a superfluid helium cryostat,” said van Kampen. “The need for cooling means that the telescope lifetime is limited by its helium supply. We are promised at least 3 years of routine operations, but this could be somewhat longer if we are lucky.”
Apart from the HSO, Europe is contributing to two other instruments to the international galaxy observing effort: SCUBA-2, which is a wide field camera for the James Clerk Maxwell Telescope (JCMT) on Mauna Kea, Hawaii, and the Atacama Large Millimetre Array (ALMA) 16400 feet up in the Chilean Andes.
The conference, which was one of the series of research conferences organised by the ESF Research Conferences Scheme, was held at Universitätszentrum Obergurgl near Innsbruck in Austria, from 24-29 March 2007. This event was organised by the ESF in partnership with the Fonds zur Förderung der wissenschaftlichen Forschung in Österreich (FWF) and the Leopold-Franzens-Universität Innsbruck (LFUI).
The European Science Foundation is based in Strasbourg, France, see www.esf.org The ESF is an association of 75 member organisations from 30 European countries. Since its inception in 1974, it has co-ordinated a wide range of pan-European scientific initiatives.
More information: www.esf.org/activities/esf-conferences/details/confdetail224.html?conf=224
Thomas Lau | alfa
SF State astronomer searches for signs of life on Wolf 1061 exoplanet
20.01.2017 | San Francisco State University
Molecule flash mob
19.01.2017 | Technische Universität Wien
An important step towards a completely new experimental access to quantum physics has been made at University of Konstanz. The team of scientists headed by...
Yersiniae cause severe intestinal infections. Studies using Yersinia pseudotuberculosis as a model organism aim to elucidate the infection mechanisms of these...
Researchers from the University of Hamburg in Germany, in collaboration with colleagues from the University of Aarhus in Denmark, have synthesized a new superconducting material by growing a few layers of an antiferromagnetic transition-metal chalcogenide on a bismuth-based topological insulator, both being non-superconducting materials.
While superconductivity and magnetism are generally believed to be mutually exclusive, surprisingly, in this new material, superconducting correlations...
Laser-driving of semimetals allows creating novel quasiparticle states within condensed matter systems and switching between different states on ultrafast time scales
Studying properties of fundamental particles in condensed matter systems is a promising approach to quantum field theory. Quasiparticles offer the opportunity...
Among the general public, solar thermal energy is currently associated with dark blue, rectangular collectors on building roofs. Technologies are needed for aesthetically high quality architecture which offer the architect more room for manoeuvre when it comes to low- and plus-energy buildings. With the “ArKol” project, researchers at Fraunhofer ISE together with partners are currently developing two façade collectors for solar thermal energy generation, which permit a high degree of design flexibility: a strip collector for opaque façade sections and a solar thermal blind for transparent sections. The current state of the two developments will be presented at the BAU 2017 trade fair.
As part of the “ArKol – development of architecturally highly integrated façade collectors with heat pipes” project, Fraunhofer ISE together with its partners...
19.01.2017 | Event News
10.01.2017 | Event News
09.01.2017 | Event News
20.01.2017 | Awards Funding
20.01.2017 | Materials Sciences
20.01.2017 | Life Sciences