The Mysterious Disappearance of a Star: Insights into a Failed Supernova Explosion

A massive star in the Andromeda galaxy has seemingly vanished instead of exploding, resulting in the formation of a black hole in a peculiar manner.

Typically, black holes originate from stars that explode as supernovas. However, they can also emerge from stars that collapse due to their own gravity, directly creating black holes without the explosive phase.

In 2024, Kisharai De from Columbia University, along with his team, investigated the case of M31-2014-DS1, an exceptionally bright star located in the Andromeda galaxy, approximately 20 times the mass of our Sun. The star exhibited an initial brightening in 2014, followed by a significant dimming from 2017 to 2020. This behavior aligned with predictions for a supernova that would fail to result in a black hole, yet no direct evidence of the black hole was observed, such as X-ray emissions.

Currently, De and his colleagues are utilizing the James Webb Space Telescope (JWST) and Chandra X-ray Observatory to study M31-2014-DS1. They have detected a faint red object at the star’s previous location, which is only about 8% brighter than the original star and enveloped in rapidly expanding dust. This finding aligns with the expected characteristics of a supernova that fails to produce a black hole. However, De and his team have refrained from commenting further, as their research has not yet undergone peer review.

Another group studying the same JWST data, including Emma Beasor from Liverpool John Moores University, UK, suggested that the case for M31-2014-DS1 failing to explode may also indicate a stellar merger, which could result in small explosions followed by dimming and dust formation.

“Predictions for the appearance of a failed supernova significantly overlap with what we might expect from a collision of two stars creating vast amounts of dust,” Beasor explained.

However, both scenarios are rare, she noted, as it is uncommon to observe such drastic color changes in a star.

“No matter the explanation, it’s fascinating that the visible star has essentially vanished,” stated Gerald Gilmore from Cambridge University. “For years, the search for extinct massive stars has produced ambiguous outcomes, but now, advancements in multi-wavelength time-domain astronomy are paving the way for clarity.”

The definitive method for confirming black hole formation is through the identification of X-ray emissions, Gilmore noted, which are currently absent at the M31-2014-DS1 location. Nevertheless, if advanced telescopes like JWST can analyze the remnants of dimmed stars, we could soon uncover what occurred. “We are on the verge of discovering at least one of the ultimate fates of a massive star, which is intriguingly akin to the Cheshire Cat’s disappearance,” he remarked.

References: arXiv, DOI: 10.48550/arXiv.2601.05774 and DOI: 10.48550/arXiv.2601.05317

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