Astronomers reveal the largest cosmic explosion ever seen
IEEC experts at the Institute of Space Sciences (ICE-CSIC) have studied the explosion, which is more than ten times brighter than any known supernova.
It took place nearly 8 billion light years away, when the universe was around 6 billion years old.
An international team of astronomers, led by the University of Southampton and with the participation of researchers from the Institute of Space Studies of Catalonia (IEEC — Institut d’Estudis Espacials de Cataluya) at the Institute of Space Sciences (ICE-CSIC), have uncovered the largest cosmic explosion ever witnessed in an article published today in Monthly Notices of the Royal Astronomical Society.
The explosion is more than ten times brighter than any known supernova (exploding star) and three times brighter than the brightest tidal disruption event, an astronomical phenomenon where a star ‘falls’ into a supermassive black hole.
The stellar explosion, known as AT2021lwx, has currently lasted over three years, compared to most supernovae which are only visibly bright for a few months. It took place nearly 8 billion light years away, when the universe was around 6 billion years old, and is still being detected by a network of telescopes.
The researchers believe that the explosion is a result of a vast cloud of gas, possibly thousands of times larger than our sun, that has been violently disrupted by a supermassive black hole. Fragments of the cloud would be swallowed up, sending shockwaves through its remnants, as well as into a large dusty ‘doughnut’ surrounding the black hole. Such events are very rare and nothing on this scale has been witnessed before.
In 2022, astronomers witnessed the brightest explosion on record – a gamma-ray burst known as GRB 221009A. While this was brighter than AT2021lwx, it lasted for just a fraction of the time, meaning the overall energy released by the AT2021lwx explosion is far greater.
“It is really shocking when you find a transient, check its brightness and you realise it is an order of magnitude brighter than any other supernova”, says Lluís Galbany, IEEC researcher at the ICE-CSIC. “When our collaborators told us the existence of this transient, we rapidly prepared a fast-turnaround proposal to observe the transient with the Gran Telescopio Canarias (GTC)”, he adds.
Detected thanks to a network of telescopes
AT2021lwx was first detected in 2020 by the Zwicky Transient Facility in California, and subsequently picked up by the Asteroid Terrestrial-impact Last Alert System (ATLAS) based in Hawaii. These facilities survey the night sky to detect transient objects that rapidly change in brightness indicating cosmic events such as supernovae, as well as finding asteroids and comets. Until now the scale of the explosion has been unknown.
“We came upon this by chance, as it was flagged by our search algorithm when we were searching for a type of supernova,” says Dr Philip Wiseman, Research Fellow at the University of Southampton, who led the research. “Most supernovae and tidal disruption events only last for a couple of months before fading away. For something to be bright for two plus years was immediately very unusual.”
The team investigated the object further with several different telescopes: the Neil Gehrels Swift Telescope (a collaboration between NASA, the UK and Italy), the New Technology Telescope (operated by the European Southern Observatory) in Chile, and the Gran Telescopio Canarias in La Palma, Spain.
“Given the uniqueness of this event, we observed it at different wavelengths with the aim of understanding its nature. In particular, our successful proposal to Gran Telescopio Canarias (GTC) allowed us to observe the presence and absence of different spectral lines, and compare these to those from other known transients to better understand the physical processes behind this bright source”, said Tomás E. Müller Bravo, IEEC postdoctoral researcher at the ICE-CSIC and Principal Investigator of the GTC proposal.
Measuring the distance to the explosion
By analysing the spectrum of the light, splitting it up into different wavelengths and measuring the different absorption and emission features of the spectrum, the team were able to measure the distance to the object.
The only things in the universe that are as bright as AT2021lwx are quasars – supermassive black holes with a constant flow of gas falling onto them at high velocity.
“When you find a transient with properties different from those you are used to monitoring, your first reaction is to try to explain what events can produce them and how. Consequently, multiple alternatives appear, but only very few can describe your observations”, says Claudia Gutiérrez, ICE-CSIC postdoctoral researcher. “This is what happened with this event”, she adds.
What caused the explosion?
There are different theories as to what could have caused such an explosion, but the team believe the most feasible explanation is an extremely large cloud of gas (mostly hydrogen) or dust that has come off course from its orbit around the black hole and been sent flying in.
The team are now setting out to collect more data on the explosion – measuring different wavelengths, including X-rays which could reveal the object’s surface and temperature, and what underlying processes are taking place. They will also carry out upgraded computational simulations to test if these match their theory of what caused the explosion.
Press release prepared in collaboration with the Institute of Space Sciences (ICE-CSIC).
Main Image
Caption: Artist impression of a black hole accretion.
Credits: John A. Paice.
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More information
This research is presented in a paper entitled “Multiwavelength observations of the extraordinary accretion event AT2021lwx”, by P. Wiseman et al., including L. Galbany, T. Müller-Bravo and C. Gutiérrez, to appear in the journal Monthly Notices of the Royal Astronomical Society on 12 May 2023. Doi.org/10.1093/mnras/stad1000
The Institute of Space Studies of Catalonia (IEEC — Institut d’Estudis Espacials de Catalunya) promotes and coordinates space research and technology development in Catalonia for the benefit of society. IEEC fosters collaborations both locally and worldwide and is an efficient agent of knowledge, innovation and technology transfer. As a result of more than 25 years of high-quality research, done in collaboration with major international organisations, IEEC ranks among the best international research centres, focusing on areas such as: astrophysics, cosmology, planetary science, and Earth Observation. IEEC’s engineering division develops instrumentation for ground- and space-based projects, and has extensive experience in working with private or public organisations from the aerospace and other innovation sectors.
IEEC is a private non-profit foundation, governed by a Board of Trustees composed of Generalitat de Catalunya and four other institutions that each have a research unit, which together constitute the core of IEEC R&D activity: the Universitat de Barcelona (UB) with the research unit ICCUB — Institute of Cosmos Sciences; the Universitat Autònoma de Barcelona (UAB) with the research unit CERES — Center of Space Studies and Research; the Universitat Politècnica de Catalunya · BarcelonaTech (UPC) with the research unit CTE — Research Group in Space Sciences and Technologies; the Spanish Research Council (CSIC) with the research unit ICE — Institute of Space Sciences. The IEEC is a CERCA (Centres de Recerca de Catalunya) centre.
Contacts
IEEC Communication Office
Barcelona, Spain
E-mail: comunicacio@ieec.cat
Lead Researcher at IEEC
Barcelona, Spain
Lluís Galbany
Institute of Space Studies of Catalonia (IEEC)
Institute of Space Sciences (ICE-CSIC)
E-mail: lgalbany@ieec.cat