December 05, 2025 01:21 pm (IST)
Follow us:
facebook-white sharing button
twitter-white sharing button
instagram-white sharing button
youtube-white sharing button
'Mamata fooled Muslims': Humayun Kabir explodes after TMC suspends him over 'Babri Masjid-style mosque' demand; announces new party | Mosque in the middle of Kolkata airport? Centre confirms flight risks, BJP fires at Mamata | Sam Altman is betting big on India! OpenAI in advanced talks with Tata to build AI infrastructure | Government removes mandatory pre-installation of Sanchar Saathi App. Know all details | Calcutta HC overturns controversial Bengal job annulment — 32,000 teachers rejoice! | Bengal SIR shock: 1 lakh ‘deceased voters’ found in Kolkata North! | Massive twist in Bengal voter list: ‘Perfect’ 2,280 booths shrink to just 480 after probe! | ‘Red carpet for intruders?’: Supreme Court raps petitioner in Rohingya case | Sanchar Saathi app row: Scindia shuts down Congress' ‘snooping’ charge — here’s what he said | Layoff alert! Marketing giant Omnicom to slash 4,000 jobs and shut historic ad agencies after IPG takeover
Supernova
WIKIMEDIA COMMONS

Indian astronomers track supernova explosion to one of the hottest kind of stars

| @indiablooms | Apr 07, 2021, at 12:05 am

New Delhi: Indian astronomers have tracked a rare supernova explosion and traced it to one of the hottest kind of stars called Wolf–Rayet stars or WR stars.

The rare Wolf–Rayet stars are highly luminous objects a thousand times that of the Sun and have intrigued astronomers for long.

They are massive stars and strip their outer hydrogen envelope which is associated with the fusion of Helium and other elements in the massive core.

Tracking of certain types of massive luminous supernovae explosion can help probe these stars that remain an enigma for scientists.

A team of astronomers from Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital an autonomous institute under the Department of Science & Technology, Govt. of India with international collaborators have conducted the optical monitoring of one such stripped-envelope supernova called SN 2015dj hosted in the galaxy NGC 7371 which was spotted in 2015.

They calculated the mass of the star that collapsed to form the supernovae as well as the geometry of its ejection. This work has been recently published in ‘The Astrophysical Journal, read a government statement.

The scientists also found that the original star was a combination of two stars – one of them is a massive WR star and another is a star much less in mass than the Sun.

Supernovae (SNe) are highly energetic explosions in the Universe releasing an enormous amount of energy.

Long-term monitoring of these transients opens the door to understand the nature of the exploding star as well as the explosion properties. It can also help enumerate the number of massive stars.

Support Our Journalism

We cannot do without you.. your contribution supports unbiased journalism

IBNS is not driven by any ism- not wokeism, not racism, not skewed secularism, not hyper right-wing or left liberal ideals, nor by any hardline religious beliefs or hyper nationalism. We want to serve you good old objective news, as they are. We do not judge or preach. We let people decide for themselves. We only try to present factual and well-sourced news.

Support objective journalism for a small contribution.