The likely location of the imtermediate-mass black hole.
The likely location of the imtermediate-mass black hole.

Astronomers amazed by black hole discovery

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A massive black hole ­– about 20,000 times the size of the sun – has been confirmed as the closest to our solar system by an international study involving University of Queensland researchers.

Journal/conference: Nature

Organisation/s: The University of Queensland

Funder: S.K. acknowledges funding from UKRI in the form of a Future Leaders Fellowship (grant no. MR/T022868/1). A.S., M.W. and A.B. acknowledge support from HST grant GO-16777. A.B. acknowledges support from STScI grants GO-15857 and AR-17033. A.F.K. acknowledges funding from the Austrian Science Fund (FWF) (https://doi.org/10.55776/ESP542). M.A.C. acknowledges support from Fondecyt Postdoctorado, project no. 3230727. A.M. acknowledges funding from PRIN 2022 2022MMEB9W (principal investigator: A. F. Marino).

Media release

From: The University of Queensland

A massive black hole ­– about 20,000 times the size of the sun – has been confirmed as the closest to our solar system by an international study involving University of Queensland researchers.

This discovery validates decades of speculation about the black hole’s existence, which the team found at the centre of the neighbouring star cluster Omega Centauri in the Milky Way, about 18,000 light-years from our solar system.

The study involved analysing and cataloguing 1.4 million stars in the cluster, which were then compared against theoretical models developed by UQ’s Associate Professor Holger Baumgardt.

“Led by the Max-Planck-Institut für Astronomie in Germany, our team searched for fast-moving stars expected to exist near concentrated masses, like black holes,” Dr Baumgardt said.

“Identifying these stars was the smoking gun evidence we needed to prove the black hole’s existence, and we did.

“When I saw the data, I immediately knew we found something special.

“Astronomers have tried to find one of these black holes for over 20 years, and now we have finally succeeded.”

The team studied more than 500 Hubble space telescope images of the cluster.

“These images were originally produced to calibrate the Hubble’s instruments rather than for scientific use, but they turned out to be the ideal data set for our research and proved to be invaluable,” Dr Baumgardt said.

To fully understand this observational data, researchers needed theoretical models to compare it against – and that’s where Dr Baumgardt’s work came in.

“After an extensive analysis, we found that only an intermediate-mass black hole, about 20,000 times the mass of our sun, could produce the seven fast moving stars we were seeing,” he said.

“This class of black holes has been a theory for decades but is now fully confirmed to exist.”

Dr Baumgardt said he and the team were amazed at the magnitude of the discovery.

“I think this will invigorate the field and lead to a lot of new research in this area,” he said.

“We can begin to speculate how this black hole formed, how it’s related to other massive black holes astronomers have found, and where other intermediate-mass black holes might exist.

“It’s a thrilling time to be an astronomer and we’re excited to see where our discovery will lead.”

This research was published in Nature.

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  • Zoom into Omega Centauri

    Video made by Thomas Müller from "Haus der Astronomie" of a zoom into the center of Omega Centauri and an animation of the measured motion of the stars. Please also note the music that was specifically composed by Klaus Jäger for this animation.

    Attribution: T. Müller, M. Häberle (MPIA)

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    Last Modified: 08 Jul 2024 12:18pm

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    An explainer of how the dataset was collected.

    Attribution: M. Häberle (MPIA)

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    Last Modified: 08 Jul 2024 12:18pm

    Note: High resolution video files are only available for download here by registered journalists who are logged in.

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