Astronomers think big all the time: its their job. And on 13th December, at a meeting hosted by the Royal Astronomical Society in London, a group of them will juggle with some truly astounding large numbers. On this occasion, though, they wont be discussing the distances to remote galaxies, but the phenomenal sizes of the telescopes they want to build so they can explore the universe to a level of detail previous generations of astronomers would never have dreamt possible. Announcing a significant development, Professor Gerry Gilmore of Cambridge University will tell the meeting that Europes astronomers have just agreed to join forces in a single project to design a new generation of ground-based optical/infrared telescopes, the Extremely Large Telescope.
The largest telescopes operating currently (the two Keck Telescopes in Hawaii) have segmented mirrors 10 metres across. Now, astronomers around the world are working towards a giant leap for astronomy - extremely large telescopes (ELTs) up to 100 metres across, 10 times bigger than the Kecks. According to Dr Adrian Russell, Director of the UK Astronomy Technology Centre (UK ATC) in Edinburgh, a telescope that large will take up more glass than has been used in all the telescopes built in the history of astronomy put together.
In Europe, several projects have been under study for some years, each aimed at identifying the key technological and organisational advances that must be met to achieve such a big step . From this month, the two main projects - Euro-50, led from Sweden, and OWL, led from the European Southern Observatory (ESO) - are joining forces with colleagues throughout Europe to create a single project, which will develop a proposal for substantial additional funding from the European Union.
Jacqueline Mitton | alfa
The taming of the light screw
22.03.2019 | Max-Planck-Institut für Struktur und Dynamik der Materie
21.03.2019 | Max-Planck-Institut für Polymerforschung
DESY and MPSD scientists create high-order harmonics from solids with controlled polarization states, taking advantage of both crystal symmetry and attosecond electronic dynamics. The newly demonstrated technique might find intriguing applications in petahertz electronics and for spectroscopic studies of novel quantum materials.
The nonlinear process of high-order harmonic generation (HHG) in gases is one of the cornerstones of attosecond science (an attosecond is a billionth of a...
Nano- and microtechnology are promising candidates not only for medical applications such as drug delivery but also for the creation of little robots or flexible integrated sensors. Scientists from the Max Planck Institute for Polymer Research (MPI-P) have created magnetic microparticles, with a newly developed method, that could pave the way for building micro-motors or guiding drugs in the human body to a target, like a tumor. The preparation of such structures as well as their remote-control can be regulated using magnetic fields and therefore can find application in an array of domains.
The magnetic properties of a material control how this material responds to the presence of a magnetic field. Iron oxide is the main component of rust but also...
Due to the special arrangement of its molecules, a new coating made of corn starch is able to repair small scratches by itself through heat: The cross-linking via ring-shaped molecules makes the material mobile, so that it compensates for the scratches and these disappear again.
Superficial micro-scratches on the car body or on other high-gloss surfaces are harmless, but annoying. Especially in the luxury segment such surfaces are...
The Potsdam Echelle Polarimetric and Spectroscopic Instrument (PEPSI) at the Large Binocular Telescope (LBT) in Arizona released its first image of the surface magnetic field of another star. In a paper in the European journal Astronomy & Astrophysics, the PEPSI team presents a Zeeman- Doppler-Image of the surface of the magnetically active star II Pegasi.
A special technique allows astronomers to resolve the surfaces of faraway stars. Those are otherwise only seen as point sources, even in the largest telescopes...
Researchers at Chalmers University of Technology and the University of Gothenburg, Sweden, have proposed a way to create a completely new source of radiation. Ultra-intense light pulses consist of the motion of a single wave and can be described as a tsunami of light. The strong wave can be used to study interactions between matter and light in a unique way. Their research is now published in the scientific journal Physical Review Letters.
"This source of radiation lets us look at reality through a new angle - it is like twisting a mirror and discovering something completely different," says...
11.03.2019 | Event News
01.03.2019 | Event News
28.02.2019 | Event News
25.03.2019 | Trade Fair News
25.03.2019 | Life Sciences
25.03.2019 | Information Technology