UK: Indian-Origin Astrophysicist, Professor Vik Dhillon, Shines Light on Universe’s Mysteries

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UK: Indian-Origin Astrophysicist, Professor Vik Dhillon, Shines Light on Universe’s Mysteries


Last Updated: October 28, 2023, 06:24 IST

London, United Kingdom (UK)

Professor Vik Dhillon is from the University of Sheffield’s Department of Physics and Astronomy. He leads the ULTRACAM undertaking.

Indian astrophysicist, Prof. Vik Dhillon, leads groundbreaking analysis, utilizing ULTRACAM, pinpointing gamma-ray bursts and kilonovae for heavy factor insights

Professor Vik Dhillon, an Indian-origin astrophysicist from the University of Sheffield within the UK, is a part of a workforce that has introduced humanity nearer to understanding how the heaviest chemical components are created within the universe utilizing a high-end digital camera.

Dhillon, a key determine within the University’s Physics and Astronomy Department, and chief of the ULTRACAM undertaking, notes that the digital camera is the primary software to exactly find the gamma-ray burst, marking the initiation of the kilonova explosion. A kilonova, ensuing from the fusion of two dense neutron stars, holds significance because it’s considered the supply of the heaviest components on the periodic desk, together with gold, platinum, and uranium discovered on Earth.

“Our camera ULTRACAM was the first instrument to pinpoint the location of the gamma-ray burst, the second brightest one ever observed, that indicated the start of the kilonova explosion,” Dhillon was quoted as saying by PTI. “This is only the second secure kilonova that has been found. Kilonovae are particularly important because it is where most of the heaviest elements in the periodic table are believed to be produced, including gold platinum and uranium, for example. This means we are now one step closer to understanding how the heaviest chemical elements are created in the universe,” he mentioned.

The discovery permits scientists to set off different telescopes all over the world for follow-up observations, together with the James Webb Space Telescope (JWST). In the findings printed within the ‘Nature’ journal this week, the scientists together with these on the University of Sheffield noticed the tell-tale purple mild from the kilonova, because of the absorption of blue mild by the heavy components produced within the explosion.

The presence of heavy components was confirmed by observations with the JWST, which found tellurium within the infrared spectrum of the kilonova. Tellurium is subsequent to iodine within the periodic desk, implying important portions of iodine – important for all times on Earth – have been additionally fashioned within the explosion.

Dr Stuart Littlefair, from the University of Sheffield’s Department of Physics and Astronomy who was concerned within the analysis, mentioned: “The role ULTRACAM played was one of being in the right place at the right time. These objects fade away very quickly and it takes a sensitive camera mounted on a large telescope to detect the optical light from the merging compact objects.”

“ULTRACAM was able to find the faint optical counterpart and allow follow-up with other telescopes. In addition, ULTRACAM can take pictures in several wavelengths of light at once, and the colour was one of the first hints that this event was something special.” Scientists noticed the merger of two neutron stars, ensuing within the explosion generally known as a kilonova. These occasions are uncommon, quick and faint, making them very tough to seek out – just one different confirmed kilonova has been noticed earlier than.

Professor Vik Dhillon’s work on kilonovae is vital as a result of the neutron-rich environments of their explosions are believed to be the place the heaviest components present in nature, corresponding to gold, platinum and uranium, are fashioned. The Indian-origin scientist is well-known within the subject of astrophysics.

He was awarded the Royal Astronomical Society Jackson-Gwilt Medal in 2013. From 2014-2019, he was an ERC Advanced Grant holder. His major analysis pursuits are within the subject of shut binary stars, through which a minimum of one stellar part is a white dwarf, neutron star or black gap. This work has led him and his collaborators to develop a collection of high-speed cameras, ULTRACAM, ULTRASPEC and HiPERCAM, in addition to a robotic telescope.

(With company inputs)



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