Home Science Space Doomed Star in Milky Way Threatens Rare Gamma-Ray Burst

Doomed Star in Milky Way Threatens Rare Gamma-Ray Burst

University of Sydney astronomers, working with international colleagues, have found a star system like none seen before in our galaxy. The scientists believe one of the stars — about 8,000 light years from Earth — is the first known candidate in the Milky Way to produce a dangerous gamma-ray burst, among the most energetic events in the universe, when it explodes and dies.

Screenshot 2018-12-03 08.10.23
The scientists believe one of the stars — about 8,000 light years from Earth — is the first known candidate in the Milky Way to produce a dangerous gamma-ray burst, among the most energetic events in the universe, when it explodes and dies. (Image: screenshot / Youtube)

The system, comprising a pair of scorchingly luminous stars, was nicknamed Apep by the team after the serpentine Egyptian god of chaos. One star is on the brink of a massive supernova explosion. The findings, published in Nature Astronomy, are controversial as no gamma-ray burst has ever been detected within our own galaxy, the Milky Way.

Yet in the southern constellation of Norma, nestled just beneath Scorpio’s tail, astronomers have discovered this uniquely beautiful star system. At its heart, wrapped in an elegantly sculpted plume of dust and gas, lies a powerful binary pair. The two hot, luminous stars — known to astronomers as Wolf-Rayets — orbit each other every hundred years or so, according to the research conducted at the Sydney Institute for Astronomy.

This orbital dance is embossed on a fast wind streaming off the stars. Using spectroscopy, the astronomers have measured the velocity of the stellar winds as fast as 12 million kilometers an hour, about 1 percent the speed of light. Dr. Joe Callingham, lead author of the study, said:

That sculpted plume is what makes the system so important, said Professor Peter Tuthill, research group leader at the University of Sydney, adding:

However, the data on the plume presented a conundrum: The stellar winds were expanding 10 times faster than the dust. Professor Tuthill said:

Dr. Benjamin Pope, a co-author from New York University, said:

Wolf-Rayet stars, like those driving Apep’s plume, are known to be very massive stars at the ends of their lives; they could explode as supernovae at any time.

The researchers think this might be the recipe for a perfect stellar storm to produce a gamma-ray burst, which is the most extreme event in the Universe after the Big Bang itself. Fortunately, Apep appears not to be aimed at Earth, because a strike by a gamma-ray burst from this proximity could strip ozone from the atmosphere, drastically increasing our exposure to UV light from the Sun. Professor Tuthill said:

This study was conducted using the Anglo-Australian Telescope at Coonabarabran and the Very Large Telescope in the Atacama Desert, Chile, and involved support from colleagues at the University of Edinburgh, the University of Sheffield, and the University of New South Wales.

This animated gif is intended to illustrate the geometry of the structure that we have witnessed in the Apep system. From a single image, it is harder to understand the 3-D structure. The central binary (only, not the wider Northern companion in the triple) is illustrated as the blue star at the center. The geometry given is that believed typical for a Wolf-Rayet colliding pinwheel system — that is an optically thin dust plume distributed over the surface of a cone that is dictated by the colliding winds. The whole outflow structure is wrapped into a spiral by the orbital motion of the presumed central binary. Further, the dust formation has a specific onset and cessation, which truncate the spiral at the outer and inner limits (for example, giving rise to the notable elliptical hole). Note: this is a toy animation to illustrate a fly-around of the structure and not a model fitted to the data that describes the dust flow process. The looping animation proceeds for about half an orbit (say roughly 60 years) with a pause at about the present epoch. Note that the motion we actually recorded with VISIR in the real data only spans 3 years. (Image: Peter Tuthill / University of Sydney / ESO)

Read more at: https://phys.org/news/2018-11-doomed-star-milky-threatens-rare.html#jCp

Provided by: University of Sydney [Note: Materials may be edited for content and length.]

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Troy Oakes
Troy was born and raised in Australia and has always wanted to know why and how things work, which led him to his love for science. He is a professional photographer and enjoys taking pictures of Australia's beautiful landscapes. He is also a professional storm chaser where he currently lives in Hervey Bay, Australia.

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