13 September 2021

Astronomers spot the same supernova three times — and predict a fourth sighting in 16 years


The enormous gravitation of a cluster of galaxies warps space to the extent that light from distant galaxies is deflected and brought to us from multiple directions. This effect has enabled astronomers from the University of Copenhagen and their collaborators to see the same exploding star at no fewer than three different locations in the sky. Moreover, they predict that a fourth image of the same explosion will appear in the sky in the year 2037. The study, recently published in the journal Nature Astronomy, provides a unique opportunity to explore not only the supernova, but also the nature of the expansion of the Universe itself.

Gravity from the MACS J0138 galaxy cluster curves space so much that light from a galaxy behind it is bent down towards us in several different ways. To the left is a picture of the cluster from 2016 in which light from the same exploding star – a supernova – is seen in three places in the night sky. To the right, is the same area in 2019, where the supernova is now gone. Astronomers from the Niels Bohr Institute have calculated that it will reappear in 2037 (credit: S. Rodney (U. of S. Carolina), G. Brammer (Cosmic Dawn Center), J. DePasquale (STScI), P. Laursen (Cosmic Dawn Center)).

One of the most fascinating aspects of Einstein's famous theory of relativity is that gravity is no longer described as a force, but as a "curvature" of space itself. Massive objects curve space, and this curvature not only causes planets to revolve around stars, but also deflect the path of light rays.

The most massive structures in the Universe — galaxy clusters with hundreds or thousands of galaxies — can deflect light from distant background galaxies so much that they appear to be located in a completely different place than they actually are.

And not only that: The light can follow multiple different routes around the cluster, so we may be lucky and see two or more images of the same galaxy, several different locations in the sky through a powerful telescope.

Supernova on repeat

Some paths around the cluster are longer than others, and hence take a longer time for the light to complete. Moreover, the higher the gravity, the slower time passes; another astonishing consequence of relativity. Therefore, it does not take exactly the same time for the light to reach us, meaning that we see the different images slightly shifted in time.

This marvelous effect has allowed astronomers from the Cosmic Dawn Center — a basic research center under the Niels Bohr Institute and DTU Space — and their international team of collaborators to observe a galaxy no fewer than four different places in the sky. The observations were performed in the infrared wavelength region with the Hubble Space Telescope.

Analyzing the Hubble data, the research team noticed three light sources in the background galaxy that were apparent in an earlier set of observations obtained in 2016, but that had disappeared by the time Hubble revisited the field in 2019. These three sources turned out to be multiple views of a star that ended its life in a colossal explosion — a so-called supernova.

"A single star exploded 10 billion years ago, long before even our own Sun had formed, and the flash of light from that explosion has only just reached us", says associate professor Gabriel Brammer of the Cosmic Dawn Center, Gabriel Brammer, who led the study along with Prof. Steven Rodney of the University of South Carolina, USA.

The supernova, nicknamed “SN-Requiem”, can be seen in three of the four “mirror images” of the galaxy, and because the light in these images have arrived with a couple of month's shift, they provide three different views of the evolution of the explosion. Looking at the last image the supernova has not yet exploded, but examining the distribution of galaxies in the cluster, as well as how the images are distorted by the curved space, it is in fact possible to calculate how far "behind in time" this image is.

In this way, the astronomers have been able to come up with a remarkable prediction:

"The fourth image of the galaxy is approximately 21 years behind those observed in 2016, and we should therefore see the supernova explode, once again, around the year 2037", Brammer explains.

The light of a galaxy with an exploding star takes different paths around an intermediate galaxy cluster before it reaches us. Astronomers from the Cosmic Dawn Center, among others, have calculated that one route is about 21 light years longer than the other. As such, they predict that come 2037, we should be able to spot the supernova yet again. Click here for an animated version (illustration: Peter Laursen, Cosmic Dawn Center).

Can teach us more about the universe

If we really see the supernova explode in the year 2037 it will not only confirm our understanding of gravitation, but can also shed light on another cosmological puzzle, namely the expansion of the Universe.

We know that the Universe is expanding, and with various methods we can measure just how fast. However, the methods currently don't give the same result, even when considering measurement uncertainties. Could our observational techniques be flawed, or — more excitingly — will we have to modify fundamental physics and our understanding of cosmology?

"Understanding the structure of the Universe is a top priority of the largest ground-based observatories and international space agencies over the next decade. Planned future surveys will cover a large fraction of the sky and are expected to reveal dozens or even hundreds of rare lensed supernovae like SN Requiem," Brammer elaborates:

"Precise time delay measurements from such sources provide unique and reliable tracers of the cosmic expansion history that can help reveal the nature of dark matter and dark energy".

Dark matter and dark energy are the mysterious stuff thought to comprise 95% of the contents of our Universe, whereas everything we see is but 5%. Indeed the prospects of gravitational lenses are promising.

Read the scientific article here


Gabriel Brammer
Associate professor 
Niels Bohr Institute
University of Copenhagen
Telefon: 31 57 55 85
Mail: gabriel.brammer@nbi.ku.dk

Peter Laursen
Scientific Assistent
Niels Bohr Institute
University of Copenhagen
Mobil: 30 26 59 69
Mail: pela@nbi.ku.dk 

Michael Skov Jensen
Faculty of Science
University of Copenhagen
Mobil: 24 26 82 96
Mail: msj@science.ku.dk 

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