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Astronomers May Have Found a Cosmic Clock Next to Our Galaxy's Giant Black Hole

February 11, 2026

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Scientists using the Green Bank Telescope have detected a possible millisecond pulsar near the Milky Way's supermassive black hole Sagittarius A star. If confirmed, this rapidly spinning neutron star could become the ultimate tool for testing Einstein's theory of General Relativity in the most extreme gravitational environment accessible to observation.

A Cosmic Needle in a Galactic Haystack

Astronomers may have detected a millisecond pulsar in the innermost region of the Milky Way's Galactic Centre, a discovery that has been described as a "holy grail" for astrophysics. The finding, published in The Astrophysical Journal, emerged from one of the most sensitive pulsar searches ever conducted toward the supermassive black hole Sagittarius A star.

The Search

A research team led by Karen Perez, a recent Columbia University PhD graduate, used the Robert C Byrd Green Bank Telescope in West Virginia as part of the Breakthrough Listen initiative. Over more than twenty hours of observations between May twenty twenty one and December twenty twenty three, the team sifted through over five thousand signal candidates. One stood out: a pulsar candidate spinning once every eight point one nine milliseconds.

Why It Matters

Pulsars are rapidly spinning neutron stars that emit beams of radiation like cosmic lighthouses, making them among the most precise natural timekeepers in the universe. Finding one near Sagittarius A star, which contains roughly four million times the mass of the Sun, would allow scientists to measure the warped spacetime around the black hole with extraordinary precision, providing the strongest test of Einstein's General Relativity ever attempted.

The Missing Pulsar Problem

Despite predictions that thousands of pulsars should exist near the Milky Way's centre, only six radio pulsars have been detected within fifty parsecs of the black hole. Scientists believe strong scattering of radio signals by interstellar material and extreme orbital dynamics may be hiding pulsar signals in this region.

What Comes Next

The candidate was persistent across a one-hour scan but was not detected in subsequent observations, and the researchers caution they cannot yet make a definitive claim. The data has been released publicly so researchers worldwide can conduct independent analyses. Next-generation instruments, including the Square Kilometre Array, may ultimately be needed to confirm the finding and solve the missing pulsar mystery.

Published February 11, 2026 at 3:57am