Astronomers have managed to peer into the past of a nearby star millions of years before its famous explosion, using a telescope in remote outback Australia at a site free from FM radio interference.
Research by an international team including astronomers at the International Centre of Radio Astronomy Research (ICRAR) observing the region at the lowest-ever radio frequencies has helped fine-tune our understanding of stellar explosions.
The research paints a picture of the star's life long before its death in what was the closest and brightest supernova seen from Earth, now known as supernova remnant 1987A, which collapsed spectacularly almost 30 years ago.
Much had been known about the immediate past of this star through studying the cosmic ruins resulting from the star's collapse in 1987, which occurred in neighbouring galaxy, the Large Magellanic Cloud. However it was the detection of the very faintest of hisses through low-frequency radio astronomy that has provided the latest insights.
Previously, only the final fraction of the dead star's multi-million-year-long life, about 0.1% or 20,000 years, had been observable.
This latest research - which has enabled astrophysicists to probe the supernova's past life millions of years further back than was previously possible - was led by Joseph Callingham, a PhD candidate with the University of Sydney and the ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO).
The findings are published today in the Monthly Notices of the Royal Astronomical Society, Oxford University Press.
Operating the Murchison Widefield Array in the West Australian desert, the radio astronomers were able to 'see' right back to when the star was in its long-lasting red supergiant phase. Mr Callingham explained previous studies focused on material that was ejected into space when the star was in its final blue supergiant phase.
"Just like excavating and studying ancient ruins that teach us about the life of a past civilisation, my colleagues and I have used low-frequency radio observations as a window into the star's life," Mr Callingham said.
The star's secret past and deadly explosion are depicted in a video compiled by CAASTRO.
The team of researchers found the red supergiant lost its matter at a slower rate and generated slower winds that pushed into its surrounding environment than was previously assumed.
"Our new data improves our knowledge of the composition of space in the region of supernova 1987A; we can now go back to our simulations and tweak them, to better reconstruct the physics of supernovae," Mr Callingham said.
Professor Lister Staveley-Smith, co-author of this study and Deputy Director of CAASTRO and ICRAR, explained that the Murchison Radio-astronomy Observatory is one of the most radio quiet places on the planet and has enabled these sensitive observations to be made.
"Low-frequency radio waves are very sensitive to the presence of intervening plasma, so tell us a great deal about the density of matter immediately in front of the supernova remnant. Their presence also tells us about the in-situ acceleration of very high-energy particles called cosmic rays, many of which are believed to be created in young remnants such as this." Professor Staveley-Smith said.
CAASTRO is a collaboration of The University of Sydney, The Australian National University, The University of Melbourne, Swinburne University of Technology, The University of Queensland, The University of Western Australia and Curtin University, the latter two participating together as the International Centre for Radio Astronomy Research (ICRAR). CAASTRO is funded under the Australian Research Council (ARC) Centre of Excellence program, with additional funding from the seven participating universities and from the NSW State Government's Science Leveraging Fund.
Media enquiries: Dr Wiebke Ebeling, CAASTRO, +61 8 9266 9174, +61 423 933 444, email@example.com
Prof Lister Staveley-Smith, CAASTRO & ICRAR, +61 8 6488 4550, firstname.lastname@example.org
Dr Giovana Zanardo, ICRAR - UWA, +61 414 531 081, Giovanna.Zanardo@gmail.com