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Home / Science / Rare Glimpse into Dying Star's Explosive Demise Sheds Light on Stellar Evolution

Rare Glimpse into Dying Star's Explosive Demise Sheds Light on Stellar Evolution

Summary

  • First-ever observation of a star's inner layers during supernova explosion
  • Dying star's outermost hydrogen and helium layers had peeled away before explosion
  • Innermost layers of silicon and sulfur also shed during the cosmic event
Rare Glimpse into Dying Star's Explosive Demise Sheds Light on Stellar Evolution

In a groundbreaking discovery, scientists have, for the first time, observed the insides of a dying star as it exploded in a supernova. The event, which occurred in our Milky Way galaxy, has provided researchers with a rare peek into the inner workings of stellar evolution.

Typically, the cosmic outbursts of supernovas tend to jumble up a dying star's layers, making it difficult for scientists to observe the star's internal structure. However, the supernova known as 2021yfj was different. The collapsing star's outermost layers of hydrogen and helium had peeled away long ago, which was not surprising. But the researchers were astonished to find that the star's dense, innermost layers of silicon and sulfur had also shed during the explosion.

"We have never observed a star that was stripped to this amount," said Steve Schulze, a member of the discovery team from Northwestern University. This finding lends evidence to scientists' ideas about how large stars look near the end of their lives, with lighter elements on the outside and heavier ones close to the core.

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The discovery offers a rare glimpse into the final stages of a star's life cycle, shedding light on the complex processes that lead to these dramatic cosmic events.

Disclaimer: This story has been auto-aggregated and auto-summarised by a computer program. This story has not been edited or created by the Feedzop team.

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FAQ

The 2021yfj supernova revealed that the collapsing star's dense, innermost layers of silicon and sulfur had shed during the explosion, providing a rare glimpse into the star's internal structure.
The 2021yfj supernova was unique in that it allowed scientists to observe the star's inner layers, which is typically not possible due to the jumbling effect of most cosmic outbursts.
The discovery lends evidence to scientists' ideas about how large stars look near the end of their lives, with lighter elements on the outside and heavier ones close to the core, and offers a rare glimpse into the final stages of a star's life cycle.

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