Artist impression of a black hole accretion. Credit John A. Paice.
An international team of astronomers, led by the University of Southampton and with the participation of 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, 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.
Last year, 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, researcher from the Institute of Space Sciences (ICE-CSIC) and member of the Institute of Space Studies of Catalonia (IEEC). “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.
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, ICE-CSIC and IEEC postdoctoral researcher and Principal Investigator of the GTC proposal.
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.
Professor Mark Sullivan, also of the University of Southampton and another co-author of the paper, explains: "With a quasar, we see the brightness flickering up and down over time. But looking back over a decade there was no detection of AT2021lwx, then suddenly it appears with the brightness of the brightest things in the universe, which is unprecedented."
"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.
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.
Dr Philip Wiseman added: "With new facilities, like the Vera Rubin Observatory’s Legacy Survey of Space and Time, coming online in the next few years, we are hoping to discover more events like this and learn more about them. It could be that these events, although extremely rare, are so energetic that they are key processes to how the centres of galaxies change over time."
This research is presented in a paper entitled "Multiwavelength observations of the extraordinary accretion event AT2021lwx", P. Wiseman et al., including L. Galbany, T. Müller-Bravo and C. Gutiérrez, Monthly Notices of the Royal Astronomical Society. Doi.org/10.1093/mnras/stad1000