It is normal for globular clusters to have dark centres made up of many dead stars. But the mass at the centre of Messier 4 looks different - despite being especially large, it seems to be squeezed into a surprisingly small volume of space.

"Using the latest Gaia and Hubble data, it was not possible to distinguish between a dark population of stellar remnants and a single larger point-like source," says Eduardo Vitral from the Space Telescope Science Institute, who led this research. "So one of the possible theories is that rather than being lots of separate small dark objects, this dark mass could be one medium-sized black hole."

Astronomers have been pondering these 'intermediate-mass black holes' for over two decades, but conclusive proof that they exist remains elusive. Most black holes that we know of are either the smaller 'stellar-mass' remnants of giant stars (up to 100 times the mass of the Sun) or the supermassive central anchors of large galaxies (billions of times the mass of the Sun). Weighing in at about 100 to 1 million Suns, intermediate-mass black holes would be the link between the two.

"Science is rarely about discovering something new in a single moment. It's about becoming more certain of a conclusion step by step, and this could be one step towards being sure that intermediate-mass black holes exist," explains Gaia mission scientist Timo Prusti.

"Data from Gaia Data Release 3 on the proper motion of stars in the Milky Way was essential in this study. Future Gaia Data Releases, as well as follow-up studies from the Hubble and James Webb Space Telescopes could shed further light."

A paper summarising the research was published in Monthly Notices of the Royal Astronomical Society. The research also used data from the Hubble Space Telescope.

Research Report:An elusive dark central mass in the globular cluster M4

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Gaia at ESA
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