Gaggle of small black holes

How galaxies and blackholes grow

Hubble researchers find a gaggle of small black holes

background pattern

Gaggle of small black holes, Larger black holes may be the usual attention-getters, but the smaller ones may be at least as important.

A team using the Hubble Space Telescope has discovered a concentration of small black holes in the NGC 6397 globular star cluster (pictured above) 7,800 light-years away —

the first to have its mass and extent recorded. While the researchers had hoped to find an elusive intermediate-mass black hole, this represents a breakthrough of its own.

Part of the challenge came from determining the mass.

Scientists used the velocities of stars in the cluster, gathered over several years from both Hubble

and the ESA’s Gaia observatory, to find the masses of the black holes.

The normally invisible bodies tugged stars around in “close to random” orbits rather

than the neatly circular or elongated paths you’d normally see with black holes.

The group likely formed as the black holes fell toward the cluster’s center through gravitational interactions with smaller stars. Heavier stars tend to gravitate toward the middle even when they haven’t collapsed into black holes.

The findings could expand humanity’s understanding of black holes and the phenomena they create. A bunch like this may be a key source of gravitational waves, for instance. So long as researchers can collect more data, this surprise discovery might pay plenty of dividends

Read more

From their studies, the researchers concluded that there’s an invisible mass of about 1,000 to 2,000 solar masses, and it would be contained inside a swarm of mostly black holes, but possibly also some white dwarfs or neutron stars. These dense objects appear to have sunk towards the center of the cluster.

“Ours is the first study to provide both the mass and the extent of what appears to be a collection of mostly black holes in the center of a core-collapsed globular cluster,” says Vitral.

The study could shed new light on the evolution of black holes of all sizes, and suggests that these tightly packed black holes could be a common source of gravitational waves as they collide.

The research was published in the journal Astronomy & Astrophysics.

Leave a Reply

Your email address will not be published. Required fields are marked *