Exploring Bella Junior’s Supernova, also referred to as RX J0852.0-4622 or G266.2-1.2, scientists have revealed the mysteries surrounding its explosive past. This ancient nebula, once a brilliant supernova, has perplexed researchers regarding its distance and the magnitude of its explosion. Recently, however, groundbreaking discoveries linked a newly formed star, Ve 7-27, with the remnants of Bella Junior. By utilizing the Multi-Unit Spectroscopic Explorer (MUSE) on the ESO’s Very Large Telescope, astronomers have captured unprecedented detailed images of Ve 7-27.
“This is the first evidence ever connecting a newborn star to the remnants of a supernova,” stated Dr. Samar Safi Harb, an astrophysicist from the University of Manitoba.
“This discovery resolves a decades-long debate, enabling us to calculate the distance of Bella Junior, its size, and the true power of the explosion.”
By examining the gas emissions from Ve 7-27, Dr. Safi Harb and his team confirmed that it shares the same chemical signature as materials from the Vela Junior supernova.
This correlation established a physical connection between the two celestial bodies, allowing astronomers to accurately determine Bella Junior’s distance.
Both Ve 7-27 and Vela Junior are approximately 4,500 light-years away.
“The gas present in this young star mirrors the chemical composition of stars that exploded in the past,” remarked Dr. Safi Harb.
“Isn’t it poetic? Those same elements eventually contributed to Earth and now play a role in forming new stars.”
Recent findings indicate that Bella Junior is larger, more energetic, and expanding at a rate quicker than previously thought, marking it as one of the most potent supernova remnants in our galaxy.
“Stars are constructed in layers, much like onions,” Dr. Safi Harb explained. “When they explode, these layers are propelled into space.”
“Our research indicates that these layers are now becoming visible in the jets of nearby young stars.”
“This study not only solves an enduring astronomical enigma but also sheds light on stellar evolution, the enrichment of galaxies with elements, and how extreme cosmic events continue to shape our universe.”
This research was published today in a study featured in the Astrophysics Journal Letters.
Source: www.sci.news
