Sgr A* is the name we’ve given to the supermassive black hole that sits at the center of the Milky Way. We’ve known about its presence since the 1970s but only managed to image it within the past few years. In the intervening time, most of our understanding of the object was obtained by watching a group of stars that orbit the black hole, helping us get a good estimate of its mass and size. In essence, those stars acted as instruments that let us peer into an environment we couldn’t study any other way.
In Wednesday’s issue of Nature, researchers describe a recently discovered star that is on an extremely eccentric orbit that takes it closer to Sgr A* than anything we’ve previously identified. It gets so close that it may help us get our first measurements of the spin of the black hole.
Reading the spin
There’s an entire population of stars that orbit relatively close to Sgr A*. We can estimate their mass based on their brightness and spectral features. Using their masses and a reconstruction of their orbits using several years of data, we can figure out just how supermassive Sgr A* is (nearly 1037 kilograms).
Figuring out a black hole’s mass doesn’t seem to tell us much about it. But there isn’t exactly much else to tell. Our understanding of relativity says that, beyond mass, there are only two distinct properties of black holes. One of them is charge, and the other is spin. There’s no way to get information about charge. But spin is a different matter. We know that the materials that form black holes have momentum that has to be conserved by the spin of the resulting body. And our detection of gravitational waves from black hole mergers tells us something about the spin.
So, we know there’s almost certainly some spin in Sgr A*. And it’s possible to learn something about it. The spin of Sgr A* should influence the precession of the orbit of any stars that pass sufficiently close. Unfortunately, that effect diminishes with the cube of the radius, which means we have to do one of two things: either find a star that goes close enough to the black hole, or do observations for long enough that the effects become apparent. Unfortunately, for all the stars we’re aware of near Sgr A*, “long enough” means thousands of years.
So, without a new discovery, we’d either need to up our imaging game in order to get finer-scaled information about the orbits of the stars we know about, or be very, very patient.
An extreme orbit
The new discovery comes out of a program that uses the GRAVITY instrument on the Very Large Telescope at the European Southern Observatory. GRAVITY combines light from four individual telescopes, giving it the resolution of a single telescope with a 130-meter diameter. Since 2017, a team has been using the instrument to track stars in the immediate vicinity of Sgr A*. While GRAVITY doesn’t natively return image data, the team could convert it to images.
In 2023, this allowed them to spot a star moving away from the black hole, which they termed S301. After several months of observations, they were able to estimate an orbit, which they used to predict its position in earlier data, allowing them to confirm they were looking at an actual star. This orbit suggested that, early in 2023, it had its closest approach to the black hole, one that took it closer than any star we had previously identified.
The best orbital model suggests that this star takes only 8.7 years to complete an orbit, more than three years less than any other star in the area. The orbit is extremely eccentric, meaning that it is tracing a severely squashed oval. A circle has an eccentricity of zero, while any value over one means that an object isn’t orbiting, but rather taking a one-way trip around a gravitational attractor. S301’s eccentricity is 0.9832, suggesting it is close to escaping the gravitational grasp of Sgr A*. (For context, Pluto’s eccentricity is 0.25.)
This leads to some pretty outrageous consequences. For example, at its closest approach, the star is moving at about 25,000 kilometers a second, which is over 8 percent of the speed of light.
At this closest approach, the star passes 10 times closer to Sgr A* than the previously identified closest star. The researchers estimate that the distance may be as small as 11 Astronomical Units (one AU is the typical distance between the Earth and Sun). That would make the separation between the two just a bit beyond Saturn’s distance from the Sun.
That’s close enough that, if S301 were a larger star (it appears to be about 1.5 times larger than the Sun), it would be disrupted by the gravity of the black hole.
A new tool
The researchers think that S301 got there by being part of a binary system that wandered too close to Sgr A*, with its partner having been ejected from the neighborhood of the black hole.
But the more significant aspect of the discovery is what it could tell us in the future. The researchers estimate that we already have instruments that can track S301’s orbit with enough precision to provide an estimate of the spin of Sgr A* with about a decade of data.
Further improvements in resolution or even a longer time series would let us start exploring even finer details of the supermassive black hole. These include whether it deviates from a perfect sphere, and whether the black hole has any additional properties beyond spin that influence its behavior.
In short, finding S301 may be like developing a higher-precision instrument to study a supermassive black hole.
Nature, 2026. DOI: 10.1038/s41586-026-10894-w (About DOIs).
