SWINDON, 17-Oct-2017 — /EuropaWire/ — In a galaxy far away, two dead stars begin a final spiral into a massive collision. The resulting explosion unleashes a huge burst of energy, sending ripples across the very fabric of space. In the nuclear cauldron of the collision, atoms are ripped apart to form entirely new elements and scattered outward across the Universe.
It could be a scenario from science fiction, but it really happened 130 million years ago — in the NGC 4993 galaxy in the Hydra constellation, at a time here on Earth when dinosaurs still ruled and flowering plants were only just evolving.
Today, dozens of UK scientists and their international collaborators representing 70 observatories worldwide announced the detection of this event and the significant “scientific firsts” it has revealed about our Universe.
Those ripples in space finally reached Earth at 1.41pm UK time, on Thursday 17 August 2017, and were recorded by the twin detectors of the US-based Laser Interferometer Gravitational-wave Observatory (LIGO) and its European counterpart Virgo.
A few seconds later, the gamma-ray burst from the collision was recorded by two specialist space telescopes, and over following weeks, other space- and ground-based telescopes recorded the aftermath of the massive explosion. UK developed engineering and technology is at the heart of many of the instruments used for the detection and analysis.
Dr John Veitch, who is co-chair of LIGO’s Compact Binary Coalescence Search Group and Research Fellow at the University of Glasgow’s School of Physics and Astronomy and played a leading role in the GW170817 data analysis said: “One key difference between the gravitational wave signals from binary black holes and binary neutron stars is that neutron stars are many times lighter than black holes. This means that the gravitational wave signal from neutron stars linger for a much greater period in the detector – for around 100 seconds as opposed to just a fraction of a second for binary black holes. A longer signal means we can glean much more information about the source.”
Studying the data confirmed scientists’ initial conclusion that the event was the collision of a pair of neutron stars – the remnants of once gigantic stars, but collapsed down into approximately the size of a city.
UK Science Minister, Jo Johnson, said “Today’s announcement of the latest detection of gravitational waves is another important development in our understanding of the universe which has been made possible by UK research and technology.
“The recent awarding of the Nobel Prize for Physics to gravitational waves research is clear recognition of the importance of this area. The UK plays a significant role in these detections, enabling us to continue building our reputation as a world leader in science and innovation which is a core part of our Industrial Strategy.”
There are a number of “firsts” associated with this event, including the first detection of both gravitational waves and electromagnetic radiation (EM) – while existing astronomical observatories “see” EM across different frequencies (eg, optical, infra-red, gamma ray etc), gravitational waves are not EM but instead ripples in the fabric of space requiring completely different detection techniques. An analogy is that LIGO and Virgo “hear” the Universe.
The announcement also confirmed the first direct evidence that short gamma ray bursts are linked to colliding neutron stars. The shape of the gravitational waveform also provided a direct measure of the distance to the source, and it was the first confirmation and observation of the previously theoretical cataclysmic aftermaths of this kind of merger – a kilonova.
Additional research papers on the aftermath of the event have also produced new understanding of how heavy elements such as gold and platinum are created by supernova and stellar collisions and then spread through the Universe. More such original science results are still under current analysis.
By combining gravitational-wave and electromagnetic signals together, researchers also used a new technique to measure the expansion rate of the Universe. This technique was first proposed in 1986 by University of Cardiff’s Professor Bernard Schutz.
UK astronomers using the VISTA telescope in Chile were among the first to locate the new source. “We were really excited when we first got notification that a neutron star merger had been detected by LIGO,” said Professor Nial Tanvir from the University of Leicester, who leads a paper in Astrophysical Journal Letters today. “We immediately triggered observations on several telescopes in Chile to search for the explosion that we expected it to produce. In the end we stayed up all night analysing the images as they came in, and it was remarkable how well the observations matched the theoretical predictions that had been made.”
Dr Kate Maguire, from Queen’s University Belfast was part of the team studying the burst of light from the smashing together of the two neutron stars “Using rapid-response triggering at some of the world’s best telescopes, we have discovered that this neutron-star merger scattered heavy chemical elements, such as gold and platinum, out into space at high speeds. These new results have significantly contributed to solving the long-debated mystery of the origin of elements heavier than iron in the periodic table.”
Once the location of the collision was pin-pointed, scientists quickly maneuvered the Swift satellite to examine the aftermath with its X-ray and UV/optical telescopes.
“We didn’t detect any X-rays from the object, which was surprising given the gamma ray detection,” said Dr Phil Evans from the University of Leicester, lead-author of a paper published today in Science. “But we did find bright ultra-violet emission, which most people were not expecting. This discovery helped us to pin down what happened after the neutron star collision was detected by LIGO and Virgo.”
Professor Alberto Vecchio from the University of Birmingham’s Institute of Gravitational Wave Astronomy said: “Detecting for the first time gravitational waves from the coalescence of a binary neutron star is fantastic, and even more so that we could do it almost in real time and precisely locate this source in the sky. If fact, telescopes around the world could then point at that little patch in the sky and show us over hours, days and weeks extra-ordinary events set in motion by this cataclysmic collision as the emerging radiation swept the whole electromagnetic spectrum.”
Chief Executive Designate of UK Research and Innovation, Sir Mark Walport said: “Over a hundred years ago Einstein introduced his revolutionary General Theory of Relativity. In this, space and time were no longer absolute, no longer a fixed background to events, he proposed the existence of gravitational waves as a way to understanding the origins of the Universe.
“The latest gravitational waves announcement, today, includes the first direct evidence that short gamma ray bursts are linked to colliding neutron stars and is the result of outstanding international collaboration. This spectacular discovery is built on ambition and tenacity of international partnerships. I am proud that UK Science is at the heart of many of the instruments and detectors used for today’s historic announcement”
Dr Brian Bowsher, Chief Executive of the UK’s Science and Technology Facilities Council, said: “This new gravitational wave discovery will inspire many young people into the world of science as it reinforces the fact that there is still so much we can learn about how the Universe works. It offers new insights into the field of astronomy as well as showcasing how technological breakthroughs made by UK engineers and scientists made this latest understanding possible.”
Media contacts
Jake Gilmore; STFC Media Manager – 07970994586
Mike Bishop; Senior Communications Officer, Cardiff University – Tel: 02920 874499 / 07713 325300
Luke Sullivan; Communications Manager (Science), University of Birmingham – Tel: 0121 414 5134 / 07789 921165
Liz Buie; Communications and Public Affairs Office, University of Glasgow – 0141 330 2702 / 07527 335373
Ather Mirza; Division of External Relations, University of Leicester – Tel: +44 (0)116 2523335 / m: +44 (0) 7711 927821
Emma Gallagher; Communications Officer, Queen’s University Belfast – Tel: 028 9097 5384
Tom Frew; Senior Press and Media Relations Manager, University of Warwick – Tel: 02476575910 / 07785433155
Notes to Editors
The first detection of gravitational waves, made on September 14, 2015 and announced on February 11, 2016, was a milestone in physics and astronomy; it confirmed a major prediction of Albert Einstein’s 1915 general theory of relativity, and marked the beginning of the new field of gravitational-wave astronomy. The UK played a leading role in that detection and key technological and computing advances were made in the UK which enabled the historic first detection.
Since then, there have been three more confirmed detections, one of which (and the most recently announced) was the first confirmed detection seen jointly by both the LIGO and Virgo detectors. In addition the 2017 Nobel Prize for Physics was last week awarded to the team behind the gravitational waves breakthrough.
The published articles announcing LIGO’s first, second, and third confirmed detections have been cited more than 1,700 times (total), according to the Web of Science citation counts. A fourth paper on the three-detector observation was published on October 6; a manuscript was made publicly available on September 27.
Gravitational waves are ripples in space caused by massive cosmic events such as the collision of black holes or the explosion of supernovae. They are not electromagnetic radiation, and as a result have been undetectable until the technological breakthroughs at LIGO enabled by UK technology. The waves carry unique information about the origins of our Universe and studying them is expected to provide important insights into the evolution of stars, supernovae, gamma-ray bursts, neutron stars and black holes. However, they interact very weakly with particles and require incredibly sensitive equipment to detect.
More information on Gravitational Waves:
STFC – Gravitational waves: everything you need to know
More about the UK’s involvement in gravitational wave research:
STFC – Working together to ride the gravitational waves
The University of Glasgow’s Institute for Gravitational Research (IGR)
Supported by STFC funding, is focused on the development of detector hardware and software for sensing gravitational waves from astrophysical sources. The work of the IGR includes materials characterisation, advanced interferometry, precision manufacture and novel data processing. They also carry out research related to Advanced LIGO, GEO600, LISA Pathfinder and other gravitational wave detectors.
The Institute of Gravitational Wave Astronomy at Birmingham
The Institute of Gravitational Wave Astronomy at Birmingham brings together expertise from a wide spectrum of disciplines to open a new window on the Universe. As part of the UK Advanced LIGO project they have built sensors and control electronics for the suspension systems. They currently are working on a wide range of aspects – quantum measurements, interferometry and optics, sensors and metrology – for upgrades of Advanced LIGO and future generation instruments. They also have a very large involvement in data analysis and observations, for example, they have co-led on the inception, development and implementation of the methods and software used to compute many of the numbers around the masses, spins, distances, location in the sky, rates of binary black hole (and now neutron star) mergers as well as the actual analysis and science interpretation.
Gravitational Physics Group at Cardiff University
For the past decade, the Gravitational Physics Group at Cardiff University have laid the foundations for how we go about detecting gravitational waves and have developed novel algorithms and software that have now become standard search tools for detecting the elusive signals.
The Group also includes world-leading experts in the collision of black holes, who have produced large-scale computer simulations to imitate these violent cosmic events and predict how gravitational waves are emitted as a consequence. These calculations were instrumental in decoding all four of the observed gravitational-wave signals to date and to measure the properties of the black holes that were detected.
SOURCE: Science and Technology Facilities Council
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- Hong Kong’s Innovation and Technology Venture Fund Becomes Strategic Financial Investor of Ignatica
- Cure for prostate cancer on the horizon
- Fanpictor signs multi-year partnership with Royal Belgian Football Association
- Fanpictor unterzeichnet mehrjährige Partnerschaft mit dem Königlich Belgischen Fussballverband
- Fanpictor signe un partenariat pluriannuel avec la Royal Belgian Football Association
- Fanpictor firma una colaboración de varios años con la Real Federación Belga de Fútbol
- Fanpictor firma una partnership pluriennale con la Royal Belgian Football Association
- Fanpictor tekent meerjarige partnership met Koninklijke Belgische Voetbalbond
- Launch of the New Akenza Platform
- De zelflerende algoritme DBLG1®: eenvoudig te gebruiken voor een optimale en gepersonaliseerde behandeling van diabetes type 1
- Launch of the Anna Lindh Foundation Virtual Marathon for Dialogue!
- Digi Communications N.V. announces the exercise of stock options by the Executive Director of the Company pursuant to the decision of the Company’s general meeting of shareholders dated 30 April 2020 and in accordance with the stock option plan approved at the level of the Company in 2017
- New research unlocks long tail growth opportunity for the tech industry
- Digi Communications NV announces the availability of the instructions on the 2020 share dividend payment
- Digi Communications NV announces that conditional stock options were granted to several Directors of the Company based on the approval of the general meeting of shareholders from 18 May 2021
- Digi Communications N.V. Announces the Company’s General Shareholders Meeting resolutions adopted on 18 May 2021 approving, amongst others, the 2020 Annual Accounts
- Digi Communications N.V. (“Digi”) announces the Q1 2021 Financial results
- Digi Communications NV announces Investors Call for the Q1 2021 Financial Results
- Digi Communications N.V. announces an Amendment to the 2021 Financial Calendar
- Fastpayhotels Hits an Industry Milestone by Connecting 500 Hotels Per Day Through DerbySoft Technology
- 4 ways to build a more flexible supply chain
- Join the world's leading virtual CBD event for FREE
- DEEPENING STRATEGIC RELATIONSHIP BETWEEN UBC AND PIONEERING DECENTRALISED PLATFORM, MANYONE
- Mono Solutions recognizes Norwegian small business agency with best website 2021 award
- Mono Solutions and Xrysos Odigos unlock new opportunities for small businesses
- Behind the scenes of a 10,000-people online conference: creating a live-event atmosphere and leveraging cybersecurity software
- Largest Supply Chain for Face masks, FFP2, FFP3 and cloth masks
- TRANSMAR AND TRANSMETRICS SIGN DEAL FOR STATE-OF-THE-ART LOGISTICS COLLABORATION
- Amendment of Digi Communications N.V. Financial Calendar for 2021
- 4iG and Digi Communications NV’s Romanian subsidiary have entered into a term sheet with regards to a potential acquisition by 4iG of DIGI Group’s Hungarian operations
- “Building Healthy Relationships and Enhancing Gender Equality”: Young women from Cyprus, Egypt, Lebanon and Jordan come together
- Bring Ventures investit dans Crossborderit (CBIT), DDP et une solution de commerce électronique
- Bring Ventures investiert in Crossborderit (CBIT), eine DDP (geliefert verzollt) und E-Commerce Lösung
- Bring Ventures invests in Crossborderit (CBIT), DDP and ecommerce solution
- Lionspeed GP with Patrick Kolb and Lorenzo Rocco joins forces with CarCollection Motorsport in 2021
- Eurekos, ein klassenbester LMS-Anbieter, hat seine Position im renommierten Fosway 9-Grid™ für Lernsysteme verbessert
- Eurekos, en førsteklasses LMS-udbyder, har forstærket sin position på den prestigefyldte Fosway 9-Grid™ for læringssystemer
- Eurekos, ein erstklassiger LMS-Anbieter, hat seine Position auf dem renommierten Fosway 9-Grid™ für Lernsysteme weiter ausgebaut
- Digi Communications N.V. announces Share transaction made by an executive director of the Company with class B shares
- Digi Communications N.V.: Announces an Amendment to the Financial Calendar for 2021
- Ideanomics Invests $13M in Italian EV Motorcycle Company, Energica
- DigiSky and Asman Technology Announce Global Reseller Agreement
- Neowintech - O Marketplace Da Sua Próxima Solução Financeira
- Neowintech - Il Marketplace per la tua prossima soluzione finanziaria
- PIONEERING DECENTRALISED SECURE MESSAGING PLATFORM MANYONE ANNOUNCES STRATEGIC RELATIONSHIP WITH UNIVERSITY COLLEGE LONDON CENTRE BLOCKCHAIN TECHNOLOGY
- Digi Communications NV announces the release of the 2020 Preliminary Financial Results
- Fraunhofer IGD develops automated robotic arm to scan cultural objects in 3D, now cooperating with Phase One
- Adapt Fast or Disappear – Choosing the Right Supplier
- Digi Communications NV announces Investors Call for the 2020 Preliminary Financial Results
- A URSAPHARM Arzneimittel e a CEBINA anunciam uma parceria com vista a reaproveitar o anti-histamínico azelastina para combater a COVID-19
- URSAPHARM Arzneimittel et CEBINA annoncent un partenariat pour reconvertir l'antihistaminique azélastine afin de lutter contre la COVID-19
- URSAPHARM Arzneimittel y CEBINA anuncian una colaboración para readaptar el antihistamínico azelastine para combatir la COVID-19
- URSAPHARM Arzneimittel and CEBINA announce partnership to repurpose the antihistamine azelastine to combat COVID-19
- ANIL UZUN Will Launch Bass Guitar Lessons Series on Youtube
- Henrik Stampe Appointed CEO for Mono Solutions
- Anna Mossberg leder Nordens största privata AI-lab i Sverige: "Utan AI riskerar svenska företag att förlora sin konkurrensfördel."
- What COVID-19 has taught us about manufacturing & the importance of a digital online marketplace
- Digi Communications N.V. announces: the Supreme Court of Hungary dismissed the Company’s appeal related to the 5G Tender procedure
- Customer Data Platform Industry to Reach $1.5 Billion in 2021: CDP Institute Report
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GreenMantra Technologies Announces Exclusive Distribution Relationship with HARKE GROUP