A nearby star could measure Sagittarius A*'s spin for the first time
Astronomers identified a star whose close orbit around our galaxy's central black hole makes relativistic frame-dragging measurable with current instruments. The finding, published in Nature, offers the first credible route to determining the spin of Sagittarius A*.
- Frame-dragging causes the orbital plane of a nearby star to precess; the precession rate encodes the black hole's spin
- The star completes its orbit in roughly 9.9 years, short enough for multiple observational passes with existing facilities
- Measuring the spin would constrain models of black hole formation and the assembly history of the Milky Way's centre