A Binary Star Neighbors Our Galaxy's Supermassive Black Hole

Learn how two orbiting stars endure the gravitational forces of nearby Sagittarius A*, a supermassive black hole at the center of our galaxy.

By Jack Knudson
Dec 17, 2024 4:01 PM
binary-star-black-hole
Credit: (ESO/ F. Peißker et al., S. Guisard)

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For the first time, researchers have spotted a binary star — a system of two stars that orbit each other — near the Sagittarius A* (Sgr A*) supermassive black hole at the center of our galaxy. Binary stars have been observed elsewhere in the universe as a common occurrence, but never in the vicinity of a supermassive black hole. 

The pair of stars, dubbed D9, was revealed from data collected by the European Southern Observatory’s Very Large Telescope (VLT) in Chile. Presented in a new Nature Communications study, the discovery of D9 has proved that binary stars can briefly endure the extreme gravitational forces generated by black holes with substantial proportions like Sgr A*.

“Black holes are not as destructive as we thought,” said Florian Peißker, lead author of the new study and a researcher at the University of Cologne, Germany, in a statement.

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