Astronomers Discovered Lightest Binary Neutron Star Pair
The newly identified PSR J1856-0039 system offers a unique laboratory for testing gravity and extreme-density matter.
Updated on Oct. 2, 2026 in Physics

Astronomers using the Five-hundred-meter Aperture Spherical Telescope (FAST) have identified PSR J1856-0039, a binary neutron star system located within the Milky Way. Researchers confirmed this system as the lightest binary neutron star pair recorded to date.
Why it matters
The discovery provides a new testbed for studying the behavior of matter under extreme conditions and validating predictions of general relativity. By observing such systems, astrophysicists can refine their understanding of gravity in high-density environments.
The system features a pulsar weighing 1.30 solar masses and a companion at 1.19 solar masses, resulting in a 2.36-hour orbital period. These figures mark the lowest combined mass of 2.488 solar masses for any binary neutron star system discovered to date.
The players
FAST
The Five-hundred-meter Aperture Spherical Telescope, a large-scale radio telescope facility used for deep space observation and pulsar research.
Physical Review Letters
A peer-reviewed scientific journal covering fundamental research across all fields of physics.
The details
Researchers utilized the FAST L-band receiver to monitor 19 sky areas simultaneously, employing a snapshot survey mode to scan the Milky Way stellar disk. The system's observed orbital decay aligns with predictions established by general relativity, the theory describing gravity as a curvature of spacetime. Each neutron star — an incredibly dense stellar remnant approximately 20 kilometers in diameter — exerts intense gravitational influence on its partner.
Timeline
October 2, 2026: Study findings published in Physical Review Letters.
82 million years: Estimated timeline until the two stars merge.
The Tech Race
This discovery adds to a global catalog of approximately 30 binary neutron star systems currently identified by radio telescopes. The finding follows an ongoing research effort to map the Milky Way disk and characterize the rarest, most compact stellar binaries.
This discovery advances the theoretical frameworks used in high-energy astrophysics rather than altering current consumer technology. Scientists will continue to monitor the system's orbital decay to provide empirical data for testing gravitational theories.
The takeaway
This discovery highlights the efficiency of snapshot radio surveys in locating rare binary systems. Researchers will now track the system's orbital decay to compare observed gravitational signatures against the predictions of general relativity.
Further reading
For more on the current methods used to observe deep space, visit Physics.
Source note: This article includes information reported by China Daily.






