FAST is the world’s largest single-dish radio telescope. Its main scientific fields include conducting large sky neutral hydrogen survey, observing pulsars, detecting interstellar molecules, and searching for extraterrestrial intelligence. Its unparalleled sensitivity and excellent survey speed will help astronomers further explore the universe.

Through studying the observation data of China's gigantic radio telescope located in the country's southwestern Guizhou Province, an international research team has uncovered compelling new evidence supporting a binary-system origin for at least some fast radio bursts (FRBs), one of the most enigmatic phenomena in modern astrophysics.

Using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), or the "China Sky Eye", Chinese and international astronomers observed a complex filamentary structure network dominated by supersonic turbulence within an interstellar gas cloud moving at ultrahigh speed in the Milky Way.

Using China's Five-hundred-meter Aperture Spherical Radio Telescope (FAST), researchers have uncovered new magnetic field structures in a rare class of binary star systems known as spider pulsars, offering valuable insights into their evolution and the mechanisms behind mass loss in their companion stars.