Hubble telescope captures rare ‘light echo’ from star explosion
New paper in Astrophysical Journal Letters featuring IFA's Max Stritzinger as main author.
- An international team of astronomers in Dublin, Barcelona, Aarhus, New York and Garching studying supernovae caught the cosmic phenomenon
- The study is based on observations with the Hubble Space Telescope
When a star explodes (a supernova), it sends its intense burst of light out in all directions. On rare occasions, rings of light or ‘light echoes’ spread out from the original supernova position, in the months and years that follow, as described in a recently published article at the Astrophysical Journal Letters journal.
The study is based on observations with the Hubble Space Telescope (HST) by a collaboration of astronomers from Aarhus, Barcelona, Dublin, New York and Garching. The scientists merged the HST images in a short gif-video, showing first the supernova explosion at the very centre, followed by light rings which appeared when light from the explosion hit various layers of dust in the vicinity.
Lead scientist Professor Maximillian Stritzinger of Aarhus University, Denmark, said: "The data set is remarkable and enabled us to produce very impressive colored images and animations that exhibit the evolution of the light echoes over a five-year period. It is a rarely seen phenomenon previously only documented in a handful of other supernovae."
Dublin-based astrophysicist Dr Morgan Fraser, UCD School of Physics, said: “While the James Webb Space Telescope has drawn much attention, its predecessor Hubble continues to provide incredible images of the universe. HST has now been observing the sky for over three decades, so we can find things like this light echo that evolve slowly over many years.
Co-author Dr. Stephen Lawrence of Hofstra University in Hempstead, New York, notes that “a good everyday analogy is to imagine the finale of a fireworks show---the bright burst of light from a shell at the end of the show will light up the smoke from earlier shells that is still lingering in the area. By comparing a series of photographs taken over several minutes, you could measure all sorts of information that is not directly related to the most recent explosion that is lighting up the scene, things like how many shells had previously exploded, how opaque is the smoke from a given shell, or how fast and in what direction was the wind blowing.”
Co-author Dr. Lluis Galbany from Institute of Space Sciences (ICE-CSIC) and the Institute of Space Studies in Catalonia (IEEC) wrote in a provided statement: “The blast wave from this powerful supernova explosion is racing outwards at over 10,000 kilometers per second. Ahead of this blastwave is an intense flash of light emitted by the supernova, and this is what is causing the expanding rings we can see in the images. Supernovae are of interest as these cosmic explosions produce many of the heavy elements such as carbon, oxygen and iron, which make up our galaxy, stars and our planet.”
The supernova in question, named SN 2016adj, was first seen in 2016 and belongs to the well-known peculiar galaxy Centaurus A, situated between 10 and 16 million lightyears from Earth. For five and a half years, the astronomers watched the area around the supernova after it slowly faded away.
Centaurus A is full of dust lanes and when the sideways spreading light from the supernova hit these dusty areas over time, they lit up further and further away from the original supernova position, creating a series of expanding rings of emission called light echoes.
The variations in these rings during the years of observation enables researchers to probe the lay-out of the dust lanes in the galaxy near the explosion. The data suggests that they consist of columns of dust with large holes in between, resembling a chunk of Swiss cheese.
Professor Stritzinger said: “Centaurus A is a huge elliptical galaxy. These are mostly quiet, dust free and without younger stars prone to go off as supernovae, but Centaurus A is obviously different. It is a strong radioastronomical source and it contains prominent dust lanes with new stars forming within. This is a sign that it has "recently" gobbled up another smaller spiral galaxy, and matters have not yet settled down, as it might in a couple of hundreds of millions of years. Observing the development of these light echoes will help us gain more insight into these violent galaxy collisions.”
Up to now, four distinct light echoes produced by four different sheets of dust have been observed. The team plans to follow up on the observations with the HST in the future, hoping that more light rings will emerge. Furthermore, it might be possible to obtain a spectrum of the light echoes, showing in effect the spectrum of the underlying supernova.