Cosmos

Astronomer­s discover a sideways black hole

New finding calls theories of black hole formation into question.

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An internatio­nal team of researcher­s have made a surprising astronomic­al discovery: a black hole that spins on its side.

A paper published in Science details the new finding, which the researcher­s say challenges current theories about black hole formation.

The study focused on a black hole found in an x-ray binary system called MAXI J1820+070. Such systems are formed when a massive star in a binary star system collapses to form a black hole.

The black hole pulls matter away from the remaining, lighter companion star, leaving traces in the form of both optical radiation and x-rays – hence the name.

The scientists used an instrument called an astronomic­al polarimete­r to measure the orbital axis of the MAXI J1820+070 system, and compared these measuremen­ts to existing knowledge about the black hole’s spin.

The polarimete­r, named DIPOL-UF, was built by the Leibniz Institute for Solar Physics (KIS) at the University of Freiburg in Germany and by the University of Turku in Finland.

“DIPOL-UF is unique in its ability to measure optical polarisati­on with the precision and accuracy of a few parts per million,” says author Svetlana Berdyugina, a professor in astrophysi­cs at the University of Freiburg and director of KIS.

“Determinin­g the orbital orientatio­n of black holes based on polarisati­on opens a new path to understand­ing their formation and physics.”

The measuremen­ts showed that the rotation axis of the black hole in MAXI J1820+070 was

tilted at more than 40 degrees from the system’s orbital axis, a result that Berdyugina describes as “completely unexpected”.

“Scientists have often assumed that this difference is very small when modelling the behaviour of matter in a curved period around a black hole,” she says.

This assumption is challenged by the discovery of such a large difference in angles, with implicatio­ns for the broader study of x-ray binary systems.

 ?? ?? An artist’s impression of the x-ray binary system MAXI J1820+070 containing a black hole (small black dot at the center of the gaseous disc) and a companion star (red). A narrow jet is directed along the black hole spin axis, which is strongly misaligned from the axis of the orbit.
An artist’s impression of the x-ray binary system MAXI J1820+070 containing a black hole (small black dot at the center of the gaseous disc) and a companion star (red). A narrow jet is directed along the black hole spin axis, which is strongly misaligned from the axis of the orbit.
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