HST image in the F814W (I-band) filter of an 800 ×800 region centered on MOA-11-191/OGLE-11-0462, obtained at our final epoch in 2017 August. North is at the top, east on the left. Encircled in green is the source star, now returned to baseline luminosity. The site is resolved into the source, a much brighter neighboring star 0.004 to the WNW, and several nearby fainter stars. The inner cyan circle has a diameter of 100, corresponding to the typical best seeing in ground-based microlensing survey images; the outer cyan circle’s diameter is 200, which is not unusual seeing. The source, bright neighbor, and several fainter stars are generally blended in ground-based frames, and the blending increases with seeing. Credit: https://arxiv.org/pdf/2201.13296.pdf

An international team of researchers has confirmed that a possible microlensing event witnessed in 2011 was due to the presence of a free-floating black hole roaming through interstellar space—the first of its kind ever observed. The group has published a paper describing their findings on the arXiv preprint server.

Scientists have assumed for some time that there are many wandering around in , but until now they had not found one. This is due to the very nature of a black hole—they are difficult to spot against the black backdrop of . Still, the evidence for their existence was strong. Prior research has shown that black holes are often formed when stars reach the end of their lives and their cores collapse, generally producing a supernova. And because many such supernova have been observed, it seemed clear that many black holes must have been created as a result.

But finding them has meant looking for effects, when light from is bent by the pull of the black hole. Given the great distances, the lensing effect is slight, making it nearly impossible to detect using even the best modern telescopes. But prevailed in 2011 when two project teams looking for such lensing spotted a star that appeared to brighten for no apparent reason. Intrigued, the researchers with this new effort began analyzing the data from Hubble. For six years, they watched as the light changed, hoping that the change was due to magnification from a black hole. Then, they found something else—the position of the star appeared to change. The researchers suggest the change could only be due to an unseen moving object exerting a force that was pulling on the light as it passed by—an interstellar black hole. The researchers continued to study the star and its light, and eventually ruled out the possibility of any coming from the lensing and also confirmed that the magnification had a long duration, both of which are prerequisites to confirming the existence of a black hole.

Taken altogether, the evidence is strong enough to confirm the sighting of a free-floating black hole. The researchers were even able to measure its size, at seven solar masses. They also found that it is traveling at approximately 45 km/second.

More information: Kailash C. Sahu et al, An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing. arXiv:2201.13296v1 [astro-ph.SR], arxiv.org/abs/2201.13296