Researchers from the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) and their collaborators at home and abroad have discovered a binary pulsar with a 53-minute orbital period using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The discovery of this binary system—named PSR J1953+1844 or M71E—fills the gap in the evolution of spider pulsar systems. The findings were published in Nature on June 20.