‘30 times bigger than our Sun’: Scientists discover a new star with unusual chemical elements 

Produced by: Tarun Mishra Designed by: Manoj Kumar

Astronomers Discover Star 30 Times Larger Than the Sun

A newly discovered star, designated J0524-0336, is found to be 30 times the size of the sun and is located about 30,000 light-years from Earth. This discovery could lead to significant revisions in current stellar evolution theories.

High Lithium Concentration Puzzles Scientists

The star J0524-0336 has an unusually high concentration of lithium, much higher than what is expected in stars at its stage of evolution. This challenges existing models of how stars evolve and produce heavier elements through nuclear fusion.

Lithium Presence Conflicts with Established Theories

Lithium is a light element typically lost during the nuclear fusion process as stars age, replaced by heavier elements like carbon and oxygen. The presence of such a high amount of lithium in J0524-0336 is contrary to these established theories.

Discovery Made During Search for Older Stars

J0524-0336 was identified during a survey for older stars in the Milky Way. As an “evolved star,” it is currently in the later stages of its life, expanding in size and brightness.

Spectroscopy Reveals Star’s Chemical Makeup

Using spectroscopy, researchers analyzed the star’s light spectrum to determine its chemical composition. The findings showed J0524-0336 contains 100,000 times more lithium than the sun does at its current age.

Hypotheses on the Unusual Lithium Levels

Scientists propose that the star may be in an unobserved stage of stellar evolution, or it could have absorbed a lithium-rich planet or star, which could explain the high lithium levels.

Ongoing Research to Uncover the Mystery

The research team plans to continue observing J0524-0336 to determine whether the lithium abundance is due to a new internal process in the star or external factors such as the absorption of another celestial body.

Further Studies to Focus on Mass Loss Events

Future studies will focus on detecting dust buildup in the star’s circumstellar disk. This could indicate a mass loss event, such as a stellar interaction, or confirm that an unknown internal process is responsible for the lithium enrichment. The research has been published on arXiv and will appear in The Astrophysical Journal.