The first sign that Albert Einstein’s theory of gravity was correct has made a repeat appearance, this time near a supermassive black hole.
In 1915, Einstein realized that his newly formulated general theory of relativity explained a weird quirk in the orbit of Mercury. Now, that same effect has been found in a star’s orbit of the enormous black hole at the heart of the Milky Way, researchers with the GRAVITY collaboration report April 16 in Astronomy & Astrophysics.
The star, called S2, is part of a stellar entourage that surrounds the Milky Way’s central black hole. For decades, researchers have tracked S2’s elliptical motion around the black hole. The researchers previously had used observations of S2 to identify a different effect of general relativity, the reddening of the star’s light due to what’s called gravitational redshift (SN: 7/26/18).
Now, they’ve determined that the ellipse rotates over time, what’s known as Schwarzschild precession. That precession is the result of the warping of spacetime caused by massive objects, according to general relativity. A similar precession in Mercury’s orbit had stumped scientists before Einstein came along (SN: 4/11/18).
While physicists have never found a case where general relativity fails, they are searching for any cracks in the theory that could help lead to a new, improved theory of gravity. The new study confirms that Einstein’s theory checks out once again, even in the intense gravitational environment around a supermassive black hole.
