science & techESA/Hubble

A galaxy's brightest X-ray source is a small black hole, not its giant core

the gist

NGC 5643 is a grand design spiral, with two clear winding arms, about 40 million light-years away in the constellation Lupus. Its active galactic nucleus, a supermassive black hole feeding on gas, is not its brightest X-ray source. Researchers using ESA's XMM-Newton found a brighter X-ray object on the outskirts, called NGC 5643 X-1. The evidence points to a black hole about 30 times the Sun's mass, locked in orbit with a companion star that feeds it gas, forming a superheated disc.

how it works

Gas falling toward a black hole collects into a flattened disc, and friction heats it to hundreds of thousands of degrees. At that temperature the gas shines most strongly in X-rays. A small black hole pulling gas from a companion star can therefore look brighter in X-rays than a giant one whose gas supply is sparse.

so what

Stellar-mass black holes can briefly outshine the giant black holes at galaxy centres in X-rays. This is a useful reminder that brightness depends on how fast a system feeds, not only on its size.

ESA/Hubble · CC BY 4.0

Image: ESA/Hubble & NASA, A. Riess, D. Thilker, D. De Martin (ESA/Hubble), M. Zamani (ESA/Hubble)