Amsterdam, June 11 : Astronomers have re-discovered one of the youngest and brightest supernova remnants in the Milky Way, the corpse of a star that exploded around 1000 years ago.

The supernova was observed by ESA’s (European Space Agency’s) orbiting X-ray observatory XMM-Newton.

Exploding stars seed the Universe with heavy chemical elements necessary to build planets and create life. The expanding cloud of debris that each explosion leaves behind, known as a supernova remnant (SNR), is a bright source of X-rays and radio waves.

Generally, the debris is thought to appear as an expanding bubble or ring.

When astronomers took the first high-resolution radio images of a celestial object known as ‘G350.1-0.3’ in the 1980s, they saw an irregular knot of gases that did not seem to meet these expectations.

So it was classified as a probable background galaxy and was quietly forgotten.

Now, Bryan Gaensler and Anant Tanna, both at the University of Sydney, have used the X-ray capabilities of XMM-Newton with their colleagues to prove that appearances can be deceptive.

G350.1-0.3 is indeed the debris of an exploded star despite its misshapen configuration. In fact, it turns out to be one of the youngest and brightest supernova remnants in the Milky Way.

To explain its shape, the team looked at radio surveys and discovered that G350.1-0.3 had exploded next to a dense cloud of gas about 15 000 light-years from Earth.

The cloud prevented the blast from expanding evenly in all directions, resulting in an example of a rare kind of misshapen supernova remnant.

G350.1-0.3 is incredibly small and young in astronomical terms, only eight light years across and about 1000 years old.

“Only a handful of such young supernova remnants are known. So even having one more is important,” said Tanna.

That is because young supernova remnants are highly luminous, with the newly-formed chemical elements glowing brightly, making them easier to study.

The re-discovered supernova’s shape, age and chemical composition will allow astronomers to better understand the violent ways in which stars end their lives.

Young supernova remnants exhibit the newly created elements and also contain clues about the way the original star exploded.

Gaensler and Tanna hope that further investigations of G350.1-0.3 will yield clues as to exactly what kind of star exploded.

“It may turn out that many of the youngest supernova remnants have these strange shapes,” said Tanna. “The hunt to find more is now on,” he added. (ANI)