This brilliant and rare beacon, powered by a black hole with a mass two billion times that of the Sun, is by far the brightest object yet found from a time when the Universe was less than 800 million years old — just a fraction of its current age.
The object that has been found, named ULAS J1120+0641, is around 100 million years younger than the previously known most distant quasar. It lies at a redshift of 7.1 which corresponds to looking back in time to a Universe that was only 770 million years old, only five per cent of its current age. Prior to this discovery, the most distant quasar known has a redshift of 6.4, the equivalent of a Universe that was 870 million years old.
With only an estimated 100 bright quasars with a redshift of higher than 7 in the whole sky, their discovery is an extremely rare find.
Nottingham's Dr Simon Dye was on the team which made the discovery, detailed in the June 30 2011 edition of the journal Nature.
Dr Dye said: "Objects that lie at such large distance are almost impossible to find in visible-light surveys because their light is stretched by the expansion of the universe. This means that by the time their light gets to Earth, most of it ends up in the infrared part of the electromagnetic spectrum.
"It took us five years to find this object. We were looking for a quasar with a redshift higher than 6.5. Finding one this far away, at a redshift higher than 7, was an exciting surprise. This quasar provides a unique opportunity to explore a 100 million year window of the cosmos that was previously out of reach."
Quasars are very bright and distant galaxies that are believed to be powered by supermassive black holes at their centres. Their great brilliance makes them powerful probes to help study the period in the history of the Universe when the first stars and galaxies were forming.
The astronomers initially detected the record-holding quasar using the UK Infra-Red Telescope (UKIRT) located in Hawaii, as part of the UKIRT Infrared Deep Sky Survey (UKIDSS). The distance to the quasar was confirmed by observations made with the FORS2 instrument on the European Southern Observatory's Very Large Telescope (VLT) and instruments on the Gemini North Telescope. Because the object is comparatively bright, it is possible to perform a spectroscopic analysis, which entails splitting the object's light into its component colours, which in turn allows astronomers to determine the quasar's physical characteristics.
The observations show that the mass of the black hole at the centre of the new quasar was about two billion times that of the Sun. This very high mass is hard to explain to early on after the Big Bang. Current theories for the growth of supermassive black holes show a slow build up in mass as the compact object pulls in matter from its surroundings. According to these models, the mass of the quasar's black hole is not expected to be higher than one-quarter of the value now determined for ULAS J1120+0641.
The team is now speculating that the existence of such a massive black hole so early on in the history of the Universe means that current models for the growth of these objects may need to be revised.
The research was led by the Astrophysics Group at Imperial College London and also involved the European Southern Observatory in Germany, the Institute of Astronomy in Cambridge, the Astrophysics Research Institute at Liverpool John Moores University, the Institute for Computational Cosmology at the University of Durham, Universiteit Antwerpen in Belgium and the Joint Astronomy Centre in Hawaii.
Emma Thorne | EurekAlert!
A better way to weigh millions of solitary stars
15.12.2017 | Vanderbilt University
A chip for environmental and health monitoring
15.12.2017 | Friedrich-Alexander-Universität Erlangen-Nürnberg
DNA molecules that follow specific instructions could offer more precise molecular control of synthetic chemical systems, a discovery that opens the door for engineers to create molecular machines with new and complex behaviors.
Researchers have created chemical amplifiers and a chemical oscillator using a systematic method that has the potential to embed sophisticated circuit...
MPQ scientists achieve long storage times for photonic quantum bits which break the lower bound for direct teleportation in a global quantum network.
Concerning the development of quantum memories for the realization of global quantum networks, scientists of the Quantum Dynamics Division led by Professor...
Researchers have developed a water cloaking concept based on electromagnetic forces that could eliminate an object's wake, greatly reducing its drag while...
Tiny pores at a cell's entryway act as miniature bouncers, letting in some electrically charged atoms--ions--but blocking others. Operating as exquisitely sensitive filters, these "ion channels" play a critical role in biological functions such as muscle contraction and the firing of brain cells.
To rapidly transport the right ions through the cell membrane, the tiny channels rely on a complex interplay between the ions and surrounding molecules,...
The miniaturization of the current technology of storage media is hindered by fundamental limits of quantum mechanics. A new approach consists in using so-called spin-crossover molecules as the smallest possible storage unit. Similar to normal hard drives, these special molecules can save information via their magnetic state. A research team from Kiel University has now managed to successfully place a new class of spin-crossover molecules onto a surface and to improve the molecule’s storage capacity. The storage density of conventional hard drives could therefore theoretically be increased by more than one hundred fold. The study has been published in the scientific journal Nano Letters.
Over the past few years, the building blocks of storage media have gotten ever smaller. But further miniaturization of the current technology is hindered by...
11.12.2017 | Event News
08.12.2017 | Event News
07.12.2017 | Event News
15.12.2017 | Power and Electrical Engineering
15.12.2017 | Materials Sciences
15.12.2017 | Life Sciences