Original title: Timing Gravity with Pulsars in the Strong Field
Riccardo Della Monica, Ivan de Martino · September 2026
Measuring gravity near a giant black hole is very difficult. Researchers want to study Sagittarius A*, the supermassive black hole at the center of our galaxy, by tracking pulsarsA pulsar is a rapidly spinning dead star that emits regular radio pulses, like a lighthouse beam.. Pulsars are dense, rotating stars that flash light like cosmic clocks. The researchers created a new timing method. It calculates the exact travel time of light using the physics of relativity, which describes how extreme gravity bends space and slows time. They tested this method by simulating arrival times for hypothetical pulsars on tight orbits near the black hole. They found that future telescopes could track these signals to measure the black hole's mass at least three orders of magnitude better than today's best star and event-horizon observations.
Imagine trying to weigh a heavy dumbbell by watching a child bounce a ball near it. The ball's path bends, but the bend is far too small to see. Now suppose the ball circles the dumbbell again and again, and you can record every pass to the microsecond. Here the dumbbell is the heavy object at the center of our galaxy, the ball is a flashing star, and the recorded pass times are the moments its flashes reach Earth.
A supermassive black hole sits at the center of our galaxy, and its mass is not known as precisely as astronomers would like. Pulsars orbiting it could improve the measurement by at least three orders of magnitude — a thousandfold — compared with current observations. That would give the sharpest possible picture of the black hole's properties.
The abstract doesn't say much about limitations, but it does make clear this is a proof-of-concept forecast based on mock data, not real observations. The predicted accuracy depends on future facilities and assumes several pulsars exist in tight orbits around Sgr A*, which have not been detected yet.
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Timing Gravity with Pulsars in the Strong Field — Riccardo Della Monica, Ivan de Martino
Abstract licence: CC0
Explanation generated by Synthesis from the abstract — it is not the original paper. This is a preprint, so it hasn't necessarily been peer reviewed.