A star explodes every second or so somewhere out in the universe, but the death of one named throes was watched by astronomers – a first in the scientist community.
The team, led by Northwestern University and the University of California, Berkeley (UC Berkeley), saw the dramatic, and violent, show of the red supergiant self-destruct, die and collapse into a type II supernova.
A type II supernova, or the so-called classic explosion, is the result of a rapid collapse and explosion of a massive star.
Prior to this historic event, it was thought red supergiants showed no evidence of their soon-to-be explosions, but throes was found to emit a bright radiation leading up to its final days.
‘This suggests at least some of these stars must undergo significant changes in their internal structure, which then result in the tumultuous ejection of gas moments before they collapse,’ the researchers shared in a press release.
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The team, led by Northwestern University and the University of California, Berkeley (UC Berkeley), saw the dramatic, and violent, show of the red supergiant self-destruct, die and collapse into a type II supernova (pictured)
Wynn Jacobson-Galán, the study’s lead author, said in a statement: ‘This is a breakthrough in our understanding of what massive stars do moments before they die.
‘Direct detection of pre-supernova activity in a red supergiant star has never been observed before in an ordinary type II supernova. For the first time, we watched a red supergiant star explode.
‘I am most excited by all of the new ‘unknowns’ that have been unlocked by this discovery.’
Stars classified as red supergiant have a mass that is more than 10 times that of Earth’s sun, have a very cool surface below 6,920 degrees Fahrenheit and enormous radii.
Prior to this historic event, it was thought red supergiants showed no evidence of their soon-to-be explosions, but throes was found to emit a bright radiation (pictured) leading up to its final days
The radius of most red giants is between 200 and 800 times that of the sun.
The bright radiation was detected last summer of 2020 by astronomers at the University of Hawaiʻi Institute for Astronomy.
A few months later, in fall of 2020, a supernova lit the sky, allowing the team to capture the violent event in real time using the W.M. Keck Observatory’s Low Resolution Imaging Spectrometer on Maunakea, Hawai’I, which was also used to image the event in real time.
The researchers created an animation of what they saw when throes (left) self-destructed (right) and collapsed into a supernova
Pictured is an animation of the supernova, which the researchers named supernova 2020tlf (SN 2020tlf)
They were able to capture the powerful and energetic explosion, which the researchers named supernova 2020tlf (SN 2020tlf).
Senior study author Raffaella Margutti, an associate professor of astronomy and astrophysics at UC Berkeley, said in a statement: ‘It’s like watching a ticking time bomb.
‘We’ve never confirmed such violent activity in a dying red supergiant star where we see it produce such a luminous emission, then collapse and combust, until now.’
SUPERNOVAE OCCUR WHEN A GIANT STAR EXPLODES
A supernova occurs when a star explodes, shooting debris and particles into space.
A supernova burns for only a short period of time, but it can tell scientists a lot about how the universe began.
One kind of supernova has shown scientists that we live in an expanding universe, one that is growing at an ever increasing rate.
Scientists have also determined that supernovas play a key role in distributing elements throughout the universe.
In 1987, astronomers spotted a ‘titanic supernova’ in a nearby galaxy blazing with the power of over 100 million suns (pictured)
There are two known types of supernova.
The first type occurs in binary star systems when one of the two stars, a carbon-oxygen white dwarf, steals matter from its companion star.
Eventually, the white dwarf accumulates too much matter, causing the star to explode, resulting in a supernova.
The second type of supernova occurs at the end of a single star’s lifetime.
As the star runs out of nuclear fuel, some of its mass flows into its core.
Eventually, the core is so heavy it can’t stand its own gravitational force and the core collapses, resulting in another giant explosion.
Many elements found on Earth are made in the core of stars and these elements travel on to form new stars, planets and everything else in the universe.
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