London, March 18: Scientists have discovered a pulsating white dwarf in a double star system, which they say holds import clues on how our Sun evolved and will eventually die.
The discovery by scientists at the University of Sheffield in the UK means the team can see how binary evolution has affected the internal structure of a white dwarf star in detail for the first time.
An eclipsing binary, or double star system, is made up of two stars orbiting each other and periodically passing in front of each other as seen from the Earth.
White dwarf stars are the burnt out cores left behind when a star like the Sun dies.
This particular white dwarf could provide key insights into the structure, evolution and death of these stars for the first time, according to the study published in the journal Nature Astronomy.
Most white dwarfs are thought to be made primarily of carbon and oxygen, but this particular white dwarf is made mostly of helium.
The researchers think this is a result of its binary companion cutting off its evolution early, before it got a chance to fuse the helium into carbon and oxygen.
The pulsations from this star were discovered using HiPERCAM, a high-speed camera developed by a team led by Professor Vik Dhillon from the University of Sheffield.
HiPERCAM can take one picture every millisecond simultaneously in five different colours and is mounted on the 10.4m Gran Telescopio Canarias (GTC), the world’s largest optical telescope on La Palma.
This allowed the researchers to detect the rapid and subtle pulsations from this particular white dwarf.
The pulsations of the white dwarf star and the eclipsing binary system allowed the team to investigate the structure of it using two techniques, asteroseismology and eclipse studies.
Asteroseismology involves measuring how fast sound waves travel through the white dwarf.
“Determining what a white dwarf is made of is not straightforward because these objects have about half of the mass of the Sun, packed into something about the size of the Earth,” said Steven Parsons, from the University of Sheffield, who led the study.
This means that gravity is extremely strong on a white dwarf, around one million times larger than here on Earth, so on the surface of a white dwarf an average person would weigh about 60,000,000kg, the researchers said.
The gravity causes all of the heavy elements in the white dwarf to sink to the centre, leaving only the lightest elements at the surface and so the true composition of it remains hidden underneath, they said.
“This pulsating white dwarf we discovered is extremely important since we can use the binary motion and the eclipse to independently measure the mass and radius of this white dwarf, which helps us determine what it is made of,” Parsons said.
“Even more interestingly, the two stars in this binary system have interacted with each other in the past, transferring material back and forth between them. We can see how this binary evolution has affected the internal structure of the white dwarf, something that we’ve not been able to do before for these kinds of binary systems,” he said. (PTI)
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