Since it first appeared in the southern night sky on February 24th 1987, Supernova 1987A has been one of the most studied objects in the history of astronomy.
The supernova was the cataclysmic death of a blue supergiant star, some 168,000 light-years from Earth, in the Large Magellanic Cloud, a satellite galaxy of our own Milky Way Galaxy. It was the brightest supernova to appear in our skies since Kepler’s Supernova in 1604 and the first since the invention of the telescope.
The brilliant new star was first spotted by two astronomers working at the Las Campanas Observatory in northern Chile the night of the 24th: the University of Toronto’s Ian Shelton, and a telescope operator at the observatory, Oscar Duhalde.
Now, Yvette Cendes, a graduate student with the University of Toronto and the Leiden Observatory, has created a time-lapse showing the aftermath of the supernova over a 25-year period, from 1992 to 2017. The images show the shockwave expanding outward and slamming into debris that ringed the original star before its demise.
Credit: Dunlap Institute for Astronomy & Astrophysics
In an accompanying paper, published in the Astrophysical Journal on October 31st, Cendes and her colleagues add to the evidence that the expanding remnant is shaped—not like a ring like those of Saturn’s—but like a donut, a form known as a torus.
They also confirm that the shockwave has now picked up some one thousand kilometres per second in speed. The acceleration has occurred because the expanding torus has punched through the ring of debris.
Cendes’ co-authors include Dunlap Institute Director Prof. Bryan Gaensler and Dunlap postdoctoral fellow Cherry Ng. The time-lapse was created from radio observations made with the CSIRO Australia Compact Telescope Array at the Paul Wild Observatory, New South Wales, Australia.
Contacts and sources:
Dunlap Institute for Astronomy & Astrophysics
Citation: The Reacceleration of the Shock Wave in the Radio Remnant of SN 1987A.
Y. Cendes, B. M. Gaensler, C.-Y. Ng, G. Zanardo, L. Staveley-Smith, A. K. Tzioumis. The Astrophysical Journal, 2018; 867 (1): 65 DOI: 10.3847/1538-4357/aae261 .