The formation of stars in distant galaxies is still largely unexplored. For the first time, astron-omers at the University of Geneva have now been able to closely observe a star system six billion light-years away. In doing so, they are confirming earlier simulations made by the University of Zurich. One special effect is made possible by the multiple reflections of images that run through the cosmos like a snake.
Today, astronomers have a pretty accurate idea of how stars were formed in the recent cosmic past. But do these laws also apply to older galaxies? For around a decade, the Hubble telescope has been allowing astronomers to observe solar systems that are six or seven billion light years away.
The cosmic snake as observed by the Astronomic Institute of the University of Geneva.
(Image: Université de Genève)
Hubble suggests that there are existing galaxies of nebulae and star clusters with a diameter of over 3000 light-years. These huge accumulations (“clumps”) of stars and gas – around a thousand times larger than the Milky Way, which is relatively new in the terms of the history of the universe – seem to be the norm for older galaxies.
A gravitational lens that detects details of distant galaxies
It is very difficult to investigate these phenomena in detail over such long distances. A team from the Observatory at the University of Geneva and the Center for Theoretical Astrophysics and Cosmology at the University of Zurich are now making use of one special effect of the universe that follows its own laws:
The telescope is directed at a very massive object whose gravitational field influences the light of a faraway galaxy lying behind it. When viewed through this ‘gravitational lens’, the propagation direction of the light of the object behind it is altered. This enlarges the image and multiplies it several times.
By these means, the researchers were able to perceive distorted, elongated images that almost touched and that looked like a ‘cosmic snake’. “The image enlarged by the lens is much more accurate and brighter. We can detect galactic details that are a hundred times smaller and compare five different resolutions to determine the structure and size of these gigantic clusters”, says Daniel Schaerer, professor at the Observatory of the University of Geneva.
Observations confirm the University of Zurich’s simulations
The international research group discovered that the clumps of stars were not quite as large and massive as the first Hubble images had suggested. With this, they corroborated Valentina Tambu-rello’s earlier simulations made on a supercomputer at the University of Zurich’s Institute of Computa-tional Science. “Thanks to the incredibly high resolution of the cosmic snake, we were able to com-pare our calculations with the observations that had already been made. This was a huge stroke of luck for us”, explains the last author of the study.
The conclusion: Contrary to what had previously been assumed, the galaxy studied is not composed of one large clump of stars, but of a number of smaller ones. “Obviously, gigantic clumps in such dis-tant galaxies can only develop under very special conditions, for instance through smaller fusions or under the influence of cold gas,” Ms. Tamburello says. The fact that this was not the case had previously been impossible to detect due to the great distance involved. In her doctoral thesis, Ms. Tambu-rello had already concluded at the end of 2016 that the actual mass and size of the clumps could only be detected at a higher resolution.
Lucio Mayer, professor at the Institute of Computational Science, emphasizes: “The observations made by the University of Geneva therefore substantiate the new results from the simulations. This shows that numerical simulations can predict and anticipate astronomical observations.”
Antonio Cava, Daniel Schaerer; Johan Richard, Pablo G. Perez-Gonzalez, Miroslava Dessauges-Zavadsky, Lucio Mayer and Valentina Tamburello. The nature of giant clumps in distant galaxies pro-bed by anatomy of the Cosmic Snake. November 13, 2017, Nature Astronomy, DOI: 10.1038/s41550-017-0295-x
Prof. Lucio Mayer
Institute for Computational Science
University of Zurich
Phone +41 44 635 61 98
Department of Astronomy
Phone +41 22 379 24 02
Beat Müller | Universität Zürich
Meteoritic stardust unlocks timing of supernova dust formation
19.01.2018 | Carnegie Institution for Science
Artificial agent designs quantum experiments
19.01.2018 | Universität Innsbruck
On the way to an intelligent laboratory, physicists from Innsbruck and Vienna present an artificial agent that autonomously designs quantum experiments. In initial experiments, the system has independently (re)discovered experimental techniques that are nowadays standard in modern quantum optical laboratories. This shows how machines could play a more creative role in research in the future.
We carry smartphones in our pockets, the streets are dotted with semi-autonomous cars, but in the research laboratory experiments are still being designed by...
What enables electrons to be transferred swiftly, for example during photosynthesis? An interdisciplinary team of researchers has worked out the details of how...
For the first time, scientists have precisely measured the effective electrical charge of a single molecule in solution. This fundamental insight of an SNSF Professor could also pave the way for future medical diagnostics.
Electrical charge is one of the key properties that allows molecules to interact. Life itself depends on this phenomenon: many biological processes involve...
At the JEC World Composite Show in Paris in March 2018, the Fraunhofer Institute for Laser Technology ILT will be focusing on the latest trends and innovations in laser machining of composites. Among other things, researchers at the booth shared with the Aachen Center for Integrative Lightweight Production (AZL) will demonstrate how lasers can be used for joining, structuring, cutting and drilling composite materials.
No other industry has attracted as much public attention to composite materials as the automotive industry, which along with the aerospace industry is a driver...
Scientists at Tokyo Institute of Technology (Tokyo Tech) and Tohoku University have developed high-quality GFO epitaxial films and systematically investigated their ferroelectric and ferromagnetic properties. They also demonstrated the room-temperature magnetocapacitance effects of these GFO thin films.
Multiferroic materials show magnetically driven ferroelectricity. They are attracting increasing attention because of their fascinating properties such as...
08.01.2018 | Event News
11.12.2017 | Event News
08.12.2017 | Event News
19.01.2018 | Materials Sciences
19.01.2018 | Health and Medicine
19.01.2018 | Physics and Astronomy